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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Chem.</journal-id>
<journal-title>Frontiers in Chemistry</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Chem.</abbrev-journal-title>
<issn pub-type="epub">2296-2646</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1231431</article-id>
<article-id pub-id-type="doi">10.3389/fchem.2023.1231431</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Chemistry</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Dominant role of excitons in photosynthetic color-tuning and light-harvesting</article-title>
<alt-title alt-title-type="left-running-head">Timpmann et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fchem.2023.1231431">10.3389/fchem.2023.1231431</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Timpmann</surname>
<given-names>K&#xf5;u</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>R&#xe4;tsep</surname>
<given-names>Margus</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1076669/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Freiberg</surname>
<given-names>Arvi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1044761/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Institute of Physics</institution>, <institution>University of Tartu</institution>, <addr-line>Tartu</addr-line>, <country>Estonia</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Estonian Academy of Sciences</institution>, <addr-line>Tallinn</addr-line>, <country>Estonia</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/914039/overview">Malgorzata Biczysko</ext-link>, Shanghai University, China</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1321104/overview">Sarthak Mandal</ext-link>, National Institute of Technology, India</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2346515/overview">Fabrizio Santoro</ext-link>, National Research Council (CNR), Italy</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Arvi Freiberg, <email>arvi.freiberg@ut.ee</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>16</day>
<month>10</month>
<year>2023</year>
</pub-date>
<pub-date pub-type="collection">
<year>2023</year>
</pub-date>
<volume>11</volume>
<elocation-id>1231431</elocation-id>
<history>
<date date-type="received">
<day>30</day>
<month>05</month>
<year>2023</year>
</date>
<date date-type="accepted">
<day>03</day>
<month>10</month>
<year>2023</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2023 Timpmann, R&#xe4;tsep and Freiberg.</copyright-statement>
<copyright-year>2023</copyright-year>
<copyright-holder>Timpmann, R&#xe4;tsep and Freiberg</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>Photosynthesis is a vital process that converts sunlight into energy for the Earth&#x2019;s ecosystems. Color adaptation is crucial for different photosynthetic organisms to thrive in their ecological niches. Although the presence of collective excitons in light-harvesting complexes is well known, the role of delocalized excited states in color tuning and excitation energy transfer remains unclear. This study evaluates the characteristics of photosynthetic excitons in sulfur and non-sulfur purple bacteria using advanced optical spectroscopic techniques at reduced temperatures. The exciton effects in these bacteriochlorophyll <italic>a</italic>-containing species are generally much stronger than in plant systems that rely on chlorophylls. Their exciton bandwidth varies based on multiple factors such as chromoprotein structure, surroundings of the pigments, carotenoid content, hydrogen bonding, and metal ion inclusion. The study nevertheless establishes a linear relationship between the exciton bandwidth and Q<sub>y</sub> singlet exciton absorption peak, which in case of LH1 core complexes from different species covers almost 130&#xa0;nm. These findings provide important insights into bacterial color tuning and light-harvesting, which can inspire sustainable energy strategies and devices.</p>
</abstract>
<kwd-group>
<kwd>exciton transport</kwd>
<kwd>exciton bandwidth</kwd>
<kwd>purple photosynthetic bacteria</kwd>
<kwd>fluorescence excitation anisotropy</kwd>
<kwd>hole-burning</kwd>
</kwd-group>
<contract-sponsor id="cn001">Eesti Teadusagentuur<named-content content-type="fundref-id">10.13039/501100002301</named-content>
</contract-sponsor>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Chemical Physics and Physical Chemistry</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>Photosynthetic organisms&#x2014;plants, algae, and some bacteria - use solar energy to convert the inorganic matter to organic compounds required for survival of all lifeforms on Earth (<xref ref-type="bibr" rid="B4">Blankenship, 2002</xref>). This basic task is carried out by a number of specialized protein units enriched by pigment chromophores, notably by chlorophylls in plants and algae, and bacteriochlorophylls in photosynthetic bacteria (<xref ref-type="bibr" rid="B33">Grimm et al., 2006</xref>). In the Earth&#x2019;s crowded ecosystems, the ability for color adaptation is essential for common thriving of various photosynthetic species. This race is most evident in the red to near infrared part of the solar spectrum, where the absorption maxima of plants and algae at about 700&#xa0;nm appear clearly separated from those of photosynthetic bacteria that span from about 800&#xa0;nm to about 1,000&#xa0;nm, see <xref ref-type="fig" rid="F1">Figure 1</xref>.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Peak-normalized Q<sub>y</sub> absorption spectra of core LH1-RC <bold>(A)</bold> and peripheral LH2 <bold>(B)</bold> light-harvesting complexes from wild type purple bacteria recorded at ambient temperature of 295&#xa0;K. For comparison sake, reciprocal (linear in energy) wavelength scale is applied. Shown in the inset of panel A is the reference terrestrial solar irradiation spectrum. The bacteria under study are evolved to efficiently exploit red-colored part of the solar spectrum.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g001.tif"/>
</fig>
<p>Much of this almost 100-nm wide spectral gap is produced by different dominating light-harvesting chromophores, which in the former case is chlorophyll <italic>a</italic> (Chl) and in the latter case bacteriochlorophyll <italic>a</italic> (BChl). This explanation, however, is not fully satisfactory. For the first, the absorption band positions of native photosynthetic systems are significantly red-shifted (shifted towards longer wavelengths or lower energy) compared with the absorbance of Chl and BChl pigment molecules dissolved in normal solvents. At low concentration the main <italic>Q</italic>
<sub>y</sub> singlet absorption bands of Chl and BChl peak at 660&#xa0;nm and 770&#xa0;nm, respectively (<xref ref-type="bibr" rid="B33">Grimm et al., 2006</xref>; <xref ref-type="bibr" rid="B80">Taniguchi and Lindsey, 2021</xref>). Only long tails of these spectra reach the destined wavelengths (<xref ref-type="bibr" rid="B48">Leiger et al., 2020</xref>), but the weak absorbance there is not adequate for supporting effective photosynthesis.</p>
<p>The above systematic discrepancy known for ages has been motivating numerous studies to understand tuning mechanisms of the spectra of photosynthetic light-harvesting complexes. One mechanism universally observed in all native systems is aggregation of the pigments. Close proximity facilitates energy transfer. In photosynthetic chromoproteins, it also generally supports collective (delocalized) excited states of the pigments called excitons with stabilized energy, thus the red-shifted spectra (<xref ref-type="bibr" rid="B71">Sauer and Austin, 1978</xref>; <xref ref-type="bibr" rid="B72">Scherz and Parson, 1984</xref>; <xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>). The classical molecular exciton model developed for understanding the spectroscopy of simple molecular aggregates and molecular crystals (<xref ref-type="bibr" rid="B14">Davydov, 1971</xref>) involves separate terms of local site energies (transition energies of individual molecules) and inter-molecular (exciton) coupling energies. As a consequence, it is considered that the interactions between molecules and surroundings impact only site energies, leaving the exciton couplings unaffected, while the interactions between molecules modulate just exciton energies. However, straightforward application of this model to more complex photosynthetic pigment-protein complexes may not always be justified (<xref ref-type="bibr" rid="B39">Jang and Mennucci, 2018</xref>). Mixing of the neutral exciton states with charge-transfer states in closely coupled pigment associations constitutes modern variation of the same theme (<xref ref-type="bibr" rid="B1">Alden et al., 1997</xref>; <xref ref-type="bibr" rid="B55">Nottoli et al., 2018</xref>; <xref ref-type="bibr" rid="B5">Bourne-Worster et al., 2023</xref>).</p>
<p>Indeed, most of the mechanisms resulting in tuning the absorption spectra of photosynthetic chromoproteins such as hydrogen (H-) bonding (<xref ref-type="bibr" rid="B18">Fowler et al., 1994</xref>; <xref ref-type="bibr" rid="B76">Sturgis et al., 1997</xref>; <xref ref-type="bibr" rid="B77">Sturgis and Robert, 1997</xref>; <xref ref-type="bibr" rid="B89">Uyeda et al., 2010</xref>), axial ligation (<xref ref-type="bibr" rid="B42">Kania and Fiedor, 2006</xref>) or macrocycle ring distortions (<xref ref-type="bibr" rid="B91">Zucchelli et al., 2007</xref>; <xref ref-type="bibr" rid="B15">De Vico et al., 2018</xref>) simultaneously affect both site energies and exciton couplings. Structural factors that control the position of the Q<sub>y</sub> absorption band of BChl in bacterial pigment-protein complexes have been reviewed, for instance, in (<xref ref-type="bibr" rid="B11">Cogdell et al., 2002</xref>). Besides, continuous fluctuations of the protein environment, thus also the conformations and transition dipole moments of the pigments, necessarily reflect on both site energies and inter-pigment couplings (<xref ref-type="bibr" rid="B52">May and K&#xfc;hn, 2000</xref>; <xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>). Well-known consequences of this dynamics are shifts and broadenings of the exciton states/bands. Less recognized is that the coupling of light-harvesting excitons to fluctuating protein surroundings may lead to exciton self-trapping effect (<xref ref-type="bibr" rid="B82">Timpmann et al., 2001</xref>; <xref ref-type="bibr" rid="B24">Freiberg et al., 2003</xref>). Static disorder only facilitates this phenomenon (<xref ref-type="bibr" rid="B86">Trinkunas and Freiberg, 2006</xref>).</p>
<p>While the concept of photosynthetic excitons is widely recognized (<xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>), the implications of delocalized excited states on color tuning and excitation dynamics of light-harvesting complexes await to be better understood (<xref ref-type="bibr" rid="B73">Scholes et al., 2011</xref>; <xref ref-type="bibr" rid="B16">Fassioli et al., 2014</xref>; <xref ref-type="bibr" rid="B53">Mirkovic et al., 2017</xref>; <xref ref-type="bibr" rid="B74">Sohail et al., 2017</xref>; <xref ref-type="bibr" rid="B70">Reimers et al., 2020</xref>; <xref ref-type="bibr" rid="B8">Cignoni et al., 2022</xref>). One of the main obstacles in achieving this fundamental photobiological goal is the lack of solid experimental data on coupling energies of photosynthetic excitons. To get this information, one as a minimum requires to determine spectral positions of the states that correspond to the high-energy top and low-energy bottom of the manifold of exciton states simply termed as exciton band. This seems easy, but due to structural and other constraints (such as overlapping spectra of different chromoprotein complexes, see below), the top and bottom states are simultaneously rarely available by conventional absorption measurements, requiring application of complementary methods. The methods previously utilized for the study of exciton band structure in separate purple bacterial complexes comprise hole-burning (<xref ref-type="bibr" rid="B69">Reddy and Small, 1991</xref>), circular dichroism (CD) (<xref ref-type="bibr" rid="B46">Koolhaas et al., 1998</xref>; <xref ref-type="bibr" rid="B32">Georgakopoulou et al., 2006b</xref>), non-linear absorption (<xref ref-type="bibr" rid="B49">Leupold et al., 1999</xref>), fluorescence excitation anisotropy (<xref ref-type="bibr" rid="B84">Timpmann et al., 2004</xref>; <xref ref-type="bibr" rid="B85">Timpmann et al., 2005</xref>), two-photon excitation (<xref ref-type="bibr" rid="B75">Stepanenko et al., 2012</xref>; <xref ref-type="bibr" rid="B67">Razjivin et al., 2019</xref>), transient absorption kinetics (<xref ref-type="bibr" rid="B28">Gall et al., 2010</xref>), two-dimensional electronic spectroscopy (<xref ref-type="bibr" rid="B13">Dahlberg et al., 2016</xref>), and self-modeling spectrum fitting (<xref ref-type="bibr" rid="B87">Trinkunas et al., 2012</xref>).</p>
<p>A centerpiece of the bacterial photosynthetic machinery is the LH1-RC super-complex, where the light-harvesting 1 (LH1) complex directly encircles the reaction center (RC) complex (<xref ref-type="bibr" rid="B36">Hunter et al., 2008</xref>). In order to cope with the great variability of terrestrial solar irradiation intensity, many purple bacteria additionally develop peripheral or LH2 light-harvesting complexes. The LH2 complex, usually not in straight contact with the RC, transfers its energy to the RC via the LH1 complex (<xref ref-type="bibr" rid="B20">Freiberg et al., 1989</xref>; <xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>). Both LH1 and LH2 appear as oligomers of basic heterodimeric structures composed of membrane-spanning &#x3b1;-helical &#x3b1;- and &#x3b2;-polypeptides, with each apoprotein unit noncovalently binding three (LH2) or two (LH1) BChl molecules and one (LH2) or two (LH1) carotenoid molecules. The number of apoprotein units and large-scale architecture of the complexes is species dependent, see (<xref ref-type="bibr" rid="B30">Gardiner et al., 2020</xref>; <xref ref-type="bibr" rid="B44">Kimura et al., 2023</xref>) for recent reviews. In the wild type (WT) <italic>Rhodobacter (Rba.) sphaeroides</italic>, for example, the presence of additional pufX polypeptide cuts the apoprotein circle and leads most of the core complexes to assemble into a nonplanar S-shaped array of 28 &#x3b1;&#x3b2;-BChl<sub>2</sub> structural units that enclose 2&#xa0;RCs (<xref ref-type="bibr" rid="B63">Qian et al., 2021a</xref>; <xref ref-type="bibr" rid="B7">Cao et al., 2022</xref>). This is the so-called dimeric core complex. In photosynthetically grown cells the dimeric antenna structures coexist with open-ring monomeric structures comprising 14 &#x3b1;&#x3b2;-BChl<sub>2</sub> subunits (<xref ref-type="bibr" rid="B64">Qian et al., 2021b</xref>). The absence of pufX in certain native and mutant complexes yields 16 &#x3b1;&#x3b2;-BChl<sub>2</sub> structural elements of LH1 fully encircling a single RC, the planar monomeric core complex LH1-RC (<xref ref-type="bibr" rid="B40">Jones et al., 1992</xref>). In LH2, a closed planar ring of apoproteins in the membrane plane is rather typical, albeit the complexes may involve different numbers of subunits counting from 7 (<xref ref-type="bibr" rid="B29">Gardiner et al., 2021</xref>) to 13 (<xref ref-type="bibr" rid="B43">Kere&#xef;che et al., 2008</xref>). The lone BChl pigment cofactor close to cytoplasmic surface of LH2 and a pair of BChls nearer to periplasmic surface form two circular pigment arrangements, named B800 and B850 according to their respective Q<sub>y</sub> exciton absorption band positions at ambient temperature. Carotenoid molecules structurally interconnect the B850 and B800 pigment assemblies. Basic quantum mechanical models to understand spectroscopy of cyclic light-harvesting complexes of purple bacteria can be found in (<xref ref-type="bibr" rid="B56">Novoderezhkin and Razjivin, 1995</xref>; <xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>; <xref ref-type="bibr" rid="B35">Hu et al., 2002</xref>; <xref ref-type="bibr" rid="B9">Cogdell et al., 2006</xref>).</p>
<p>In the current work, we first aimed at evaluation of the top and bottom edges, thus the bandwidth of LH1 and LH2 light-harvesting excitons, for the broad class of photosynthetic purple bacteria comprising purple sulfur and purple non-sulfur bacteria. We show that this task is feasible by simultaneous utilization of a variety of spectroscopic techniques, including absorption, fluorescence excitation, fluorescence excitation anisotropy, circular dichroism (CD), and spectral hole-burning. The bandwidths of excitons were determined for 17 core and 16 peripheral WT and engineered light-harvesting detergent-purified and/or membrane-embedded complexes. A robust linear correlation established between the bandwidths and positions of the Q<sub>y</sub> exciton absorption spectra reveals key role of excitons in enhancing the spectral range of bacterial light-harvesting, confirming the earlier cherished intuition (<xref ref-type="bibr" rid="B90">van Amerongen et al., 2000</xref>).</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>2 Materials and methods</title>
<sec id="s2-1">
<title>2.1 Materials</title>
<p>The various LH1 and/or LH1-RC core, and peripheral LH2/LH3 complexes from sulfur (<italic>Ectothiorhodospira (E.) haloalkaliphila, Thermochromatium (Tch.) tepidum</italic>, <italic>Thiorhodovibrio</italic> strain 970 <italic>(Trv.</italic> 970<italic>)</italic>) and non-sulfur (<italic>Rba. sphaeroides, Rhodoblastus (Rbl.) acidophilus, Rhodospirillum (Rsp.) rubrum</italic>) purple bacteria studied here were kindly donated to the authors by Profs. R. Cogdell (Glasgow University), C. N. Hunter (Sheffield University), A. A. Moskalenko (IBBP, Pushchino), Z.-Y. Wang-Otomo (Ibaraki University), and N. Woodbury (Arizona State University). The purple sulfur and purple non-sulfur bacteria, respectively, use either sulfide and hydrogen or organic compounds as an electron donor (<xref ref-type="bibr" rid="B36">Hunter et al., 2008</xref>). Isolation and purification of the complexes were carried out following standard protocols, as described in refs. provided in bookkeeping <xref ref-type="table" rid="T1">Table 1</xref>. Specific samples investigated are enlisted in <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>. Distinct aspects of the sample preparation and handling are commented at proper places of the manuscript.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>List of the BChl-a containing light-harvesting complexes studied in this work.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" colspan="2" align="center">Strain</th>
<th colspan="2" align="center">Complex</th>
</tr>
<tr>
<th align="center">LH1-RC</th>
<th align="center">LH2</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">
<italic>Trv</italic>. 970<sup>c1</sup>
</td>
<td rowspan="3" align="center">Sulfur bacteria</td>
<td align="center">&#xd7;</td>
<td align="center">N/A<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<italic>Tch. tepidum</italic>
<sup>c2</sup>
</td>
<td align="center">&#xd7;</td>
<td align="center">&#xd7;</td>
</tr>
<tr>
<td align="left">
<italic>E. haloalkaliphila</italic>
<sup>c3</sup>
</td>
<td align="center">NA<xref ref-type="table-fn" rid="Tfn2">
<sup>b</sup>
</xref>
</td>
<td align="center">&#xd7;</td>
</tr>
<tr>
<td align="left">
<italic>Rsp. rubrum</italic>
<sup>c4</sup>
</td>
<td rowspan="3" align="center">Non-sulfur bacteria</td>
<td align="center">&#xd7;</td>
<td align="center">N/A<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<italic>Rba. sphaeroides</italic>
<sup>c5,c6,c7</sup>
</td>
<td align="center">&#xd7;</td>
<td align="center">&#xd7;</td>
</tr>
<tr>
<td align="left">
<italic>Rbl. acidophilus</italic>
<sup>c8</sup>
</td>
<td align="center">&#xd7;</td>
<td align="center">&#xd7;</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn1">
<label>
<sup>a</sup>
</label>
<p>N/A&#x2013;not applicable.</p>
</fn>
<fn id="Tfn2">
<label>
<sup>b</sup>
</label>
<p>NA-not available.</p>
</fn>
<fn id="Tfn3">
<label>
<sup>c</sup>
</label>
<p>References: 1- (<xref ref-type="bibr" rid="B92">Tani et al., 2020</xref>), 2- (<xref ref-type="bibr" rid="B78">Suzuki et al., 2007</xref>), 3- (<xref ref-type="bibr" rid="B2">Ashikhmin et al., 2014</xref>), 4- (<xref ref-type="bibr" rid="B54">Moskalenko et al., 1996</xref>), 5- (<xref ref-type="bibr" rid="B76">Sturgis et al., 1997</xref>), 6- (<xref ref-type="bibr" rid="B40">Jones et al., 1992</xref>), 7- (<xref ref-type="bibr" rid="B57">Olsen et al., 1994</xref>), 8- (<xref ref-type="bibr" rid="B10">Cogdell and Hawthornthwaite, 1993</xref>).</p>
</fn>
</table-wrap-foot>
</table-wrap>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>The Q<sub>y</sub> exciton band parameters for detergent-isolated and membrane-embedded (m-) core light-harvesting complexes recorded at 4.5&#xa0;K.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="left">Strain</th>
<th rowspan="2" align="left">Sample</th>
<th colspan="2" align="center">Absorption peak (nm)<xref ref-type="table-fn" rid="Tfn4">
<sup>a</sup>
</xref>
</th>
<th colspan="2" align="center">Anisotropy dips (nm)</th>
<th colspan="2" align="center">Exciton bandwidth (cm<sup>&#x2013;1</sup>)<xref ref-type="table-fn" rid="Tfn5">
<sup>b</sup>
</xref>
</th>
<th rowspan="2" align="center">&#x393;<sub>IDF</sub> (cm<sup>&#x2013;1</sup>)<xref ref-type="table-fn" rid="Tfn6">
<sup>c</sup>
</xref>
</th>
</tr>
<tr>
<th align="center">&#x3bb;<sub>Q</sub>
</th>
<th align="center">&#x3bb;<sub>0</sub>
</th>
<th align="center">Blue</th>
<th align="center">Red</th>
<th align="center">&#x2206;E</th>
<th align="center">&#x2206;E<sub>0</sub>
</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td rowspan="2" align="left">
<italic>Trv.</italic> 970</td>
<td align="left">LH1-RC WT<sup>d1</sup>
</td>
<td align="center">986.8</td>
<td align="center">1,002.8</td>
<td align="center">770.6</td>
<td align="center">977.9</td>
<td align="center">2,751</td>
<td align="center">3,005</td>
<td align="center">88</td>
</tr>
<tr>
<td align="left">LH1-RC (Ca&#x2212;)<sup>d1</sup>
</td>
<td align="center">900.6</td>
<td align="center">928.5</td>
<td align="center">757.9</td>
<td align="center">894.8</td>
<td align="center">2,020</td>
<td align="center">2,424</td>
<td align="center">218</td>
</tr>
<tr>
<td rowspan="2" align="left">
<italic>Tch. tepidum</italic>
</td>
<td align="left">LH1-RC WT<sup>d1</sup>
</td>
<td align="center">938.4</td>
<td align="center">951.3</td>
<td align="center">765.9</td>
<td align="center">930.8</td>
<td align="center">2,310</td>
<td align="center">2,545</td>
<td align="center">117</td>
</tr>
<tr>
<td align="left">LH1-RC (Ba&#x2b;)</td>
<td align="center">905.9</td>
<td align="center">924.1</td>
<td align="center">760.5</td>
<td align="center">900.1</td>
<td align="center">2,039</td>
<td align="center">2,328</td>
<td align="center">198</td>
</tr>
<tr>
<td rowspan="2" align="left">
<italic>Rsp. rubrum</italic>
</td>
<td align="left">m-LH1-RC WT</td>
<td align="center">897.4</td>
<td align="center">909.8</td>
<td align="center">755.0</td>
<td align="center">889.1</td>
<td align="center">1,998</td>
<td align="center">2,254</td>
<td align="center">123</td>
</tr>
<tr>
<td align="left">m-LH1-RC G9&#x2b;<xref ref-type="table-fn" rid="Tfn8">
<sup>e</sup>
</xref>
</td>
<td align="center">888.6</td>
<td align="center">903.1</td>
<td align="center">754.9</td>
<td align="center">883.4</td>
<td align="center">1,927</td>
<td align="center">2,174</td>
<td align="center">155</td>
</tr>
<tr>
<td align="left">
<italic>Rbl. acid</italic>
</td>
<td align="left">m-LH1-RC WT<sup>d2,d3</sup>
</td>
<td align="center">901.8</td>
<td align="center">NA</td>
<td align="center">765.6</td>
<td align="center">901.6</td>
<td align="center">1,969</td>
<td align="center">NA</td>
<td align="center">NA</td>
</tr>
<tr>
<td rowspan="10" align="left">
<italic>Rba. sphaeroides</italic>
</td>
<td align="left">LH1<sup>d3,d4</sup>
</td>
<td align="center">886.1</td>
<td align="center">896.0</td>
<td align="center">756.0</td>
<td align="center">880.0</td>
<td align="center">1,864</td>
<td align="center">2,067</td>
<td align="center">119</td>
</tr>
<tr>
<td align="left">m-LH1<sup>d3,d4</sup>
</td>
<td align="center">888.4</td>
<td align="center">900.1</td>
<td align="center">749.7</td>
<td align="center">883.8</td>
<td align="center">2,024</td>
<td align="center">2,229</td>
<td align="center">108</td>
</tr>
<tr>
<td align="left">LH1-RC-pufX WT<sup>d3,d4,</sup>
<xref ref-type="table-fn" rid="Tfn9">
<sup>f</sup>
</xref>
</td>
<td align="center">884.0</td>
<td align="center">894.6</td>
<td align="center">749.8</td>
<td align="center">873.3</td>
<td align="center">1,886</td>
<td align="center">2,159</td>
<td align="center">128</td>
</tr>
<tr>
<td align="left">m-LH1-RC-pufX WT<sup>d3,d4,</sup>
<xref ref-type="table-fn" rid="Tfn9">
<sup>f</sup>
</xref>
</td>
<td align="center">885.6</td>
<td align="center">897.6</td>
<td align="center">751.5</td>
<td align="center">876.1</td>
<td align="center">1,892</td>
<td align="center">2,166</td>
<td align="center">118</td>
</tr>
<tr>
<td align="left">m-LH1-RC-pufX WT<xref ref-type="table-fn" rid="Tfn10">
<sup>g</sup>
</xref>
</td>
<td align="center">886.1</td>
<td align="center">897.8</td>
<td align="center">755.1</td>
<td align="center">876.4</td>
<td align="center">1,833</td>
<td align="center">2,105</td>
<td align="center">135</td>
</tr>
<tr>
<td align="left">m-LH1-RC-pufX &#x394;CrtB<xref ref-type="table-fn" rid="Tfn8">
<sup>e</sup>
</xref>
</td>
<td align="center">883.0</td>
<td align="center">897.5</td>
<td align="center">755.1</td>
<td align="center">877.7</td>
<td align="center">1,850</td>
<td align="center">2,101</td>
<td align="center">109</td>
</tr>
<tr>
<td align="left">LH1-RC-pufX<xref ref-type="table-fn" rid="Tfn11">
<sup>h</sup>
</xref>
</td>
<td align="center">861.1</td>
<td align="center">872.8</td>
<td align="center">751.0</td>
<td align="center">855.5</td>
<td align="center">1,627</td>
<td align="center">1,857</td>
<td align="center">186</td>
</tr>
<tr>
<td align="left">LH1-RC-pufX<xref ref-type="table-fn" rid="Tfn12">
<sup>i</sup>
</xref>
</td>
<td align="center">880.3</td>
<td align="center">892.4</td>
<td align="center">744.4</td>
<td align="center">867.2</td>
<td align="center">1,902</td>
<td align="center">2,228</td>
<td align="center">160</td>
</tr>
<tr>
<td align="left">LH1-RC<sup>d4,</sup>
<xref ref-type="table-fn" rid="Tfn13">
<sup>j</sup>
</xref>
</td>
<td align="center">884.5</td>
<td align="center">897.6</td>
<td align="center">752.9</td>
<td align="center">879.6</td>
<td align="center">1,913</td>
<td align="center">2,141</td>
<td align="center">134</td>
</tr>
<tr>
<td align="left">m-LH1-RC<sup>d4,</sup>
<xref ref-type="table-fn" rid="Tfn13">
<sup>j</sup>
</xref>
</td>
<td align="center">885.6</td>
<td align="center">898.0</td>
<td align="center">751.6</td>
<td align="center">880.8</td>
<td align="center">1,952</td>
<td align="center">2,169</td>
<td align="center">120</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn4">
<label>
<sup>a</sup>
</label>
<p>&#x3bb;<sub>Q</sub> and &#x3bb;<sub>0</sub>, respectively, represent the peak wavelength of the Q<sub>y</sub> absorption band and the maximum of the inhomogeneous distribution function (IDF) of the k &#x3d; 0 exciton states; experimental uncertainty of the measurements: &#xb1;(0.4&#x2013;0.8) nm.</p>
</fn>
<fn id="Tfn5">
<label>
<sup>b</sup>
</label>
<p>Uncertainty of the &#x2206;E and &#x2206;E<sub>0</sub> values: &#xb1;20&#xa0;cm<sup>&#x2212;1</sup>.</p>
</fn>
<fn id="Tfn6">
<label>
<sup>c</sup>
</label>
<p>&#x393;<sub>IDF</sub>, full width at half maximum of IDF; uncertainty of the measurements: &#xb1;(10&#x2013;30) cm<sup>&#x2212;1</sup>.</p>
</fn>
<fn id="Tfn7">
<label>
<sup>d</sup>
</label>
<p>References: 1- (<xref ref-type="bibr" rid="B83">Timpmann et al., 2021</xref>), 2- (<xref ref-type="bibr" rid="B47">Kunz et al., 2013</xref>), 3- (<xref ref-type="bibr" rid="B22">Freiberg et al., 2013</xref>), 4 - (<xref ref-type="bibr" rid="B85">Timpmann et al., 2005</xref>). For comparability sake, the data obtained in previous publications have been re-scaled according to the experimental and calculation procedures taken in the present work.</p>
</fn>
<fn id="Tfn8">
<label>
<sup>e</sup>
</label>
<p>Carotenoid-less mutant.</p>
</fn>
<fn id="Tfn9">
<label>
<sup>f</sup>
</label>
<p>Dominant carotenoid spheroidenone.</p>
</fn>
<fn id="Tfn10">
<label>
<sup>g</sup>
</label>
<p>Dominant carotenoid spheroidene.</p>
</fn>
<fn id="Tfn11">
<label>
<sup>h</sup>
</label>
<p>&#x3b1;&#x2b;11&#xa0;H-bond mutant.</p>
</fn>
<fn id="Tfn12">
<label>
<sup>i</sup>
</label>
<p>&#x3b2;&#x2b;9&#xa0;H-bond mutant.</p>
</fn>
<fn id="Tfn13">
<label>
<sup>j</sup>
</label>
<p>Monomeric closed-ring mutant.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<table-wrap id="T3" position="float">
<label>TABLE 3</label>
<caption>
<p>Exciton parameters related to the B850/B820 band of detergent-isolated and membrane-embedded peripheral light-harvesting complexes recorded at 4.5&#xa0;K.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="left">Strain</th>
<th rowspan="2" align="left">Sample</th>
<th colspan="2" align="center">Absorption peak (nm)<xref ref-type="table-fn" rid="Tfn14">
<sup>a</sup>
</xref>
</th>
<th colspan="2" align="center">Anisotropy dips (nm)</th>
<th colspan="2" align="center">Exciton bandwidth (cm<sup>&#x2013;1</sup>)<xref ref-type="table-fn" rid="Tfn15">
<sup>b</sup>
</xref>
</th>
<th align="center">&#x393;<sub>IDF</sub> (cm<sup>&#x2013;1</sup>)<xref ref-type="table-fn" rid="Tfn16">
<sup>c</sup>
</xref>
</th>
</tr>
<tr>
<th align="center">&#x3bb;<sub>Q</sub>
</th>
<th align="center">&#x3bb;<sub>0</sub>
</th>
<th align="center">Blue</th>
<th align="center">Red</th>
<th align="center">&#x2206;E</th>
<th align="center">&#x2206;E<sub>0</sub>
</th>
<th align="left"/>
</tr>
</thead>
<tbody valign="top">
<tr>
<td rowspan="3" align="left">
<italic>Tch. tepidum</italic>
</td>
<td align="left">LH2 WT</td>
<td align="center">875.5</td>
<td align="center">898.4</td>
<td align="center">760.8</td>
<td align="center">865.5</td>
<td align="center">1,590</td>
<td align="center">2,013</td>
<td align="center">178</td>
</tr>
<tr>
<td align="left">LH2 (Ca removed)</td>
<td align="center">NA</td>
<td align="center">NA</td>
<td align="center">760.5</td>
<td align="center">865.5</td>
<td align="center">1,597</td>
<td align="center">NA</td>
<td align="center">NA</td>
</tr>
<tr>
<td align="left">LH2 (Ba exchanged)</td>
<td align="center">NA</td>
<td align="center">NA</td>
<td align="center">761.6</td>
<td align="center">866.7</td>
<td align="center">1,592</td>
<td align="center">NA</td>
<td align="center">NA</td>
</tr>
<tr>
<td rowspan="2" align="left">
<italic>E. haloalkaliphila</italic>
</td>
<td align="left">LH2 WT</td>
<td align="center">862.1</td>
<td align="center">878.8</td>
<td align="center">759.1</td>
<td align="center">850.7</td>
<td align="center">1,418</td>
<td align="center">1,794</td>
<td align="center">254</td>
</tr>
<tr>
<td align="left">LH2 (car-less)</td>
<td align="center">860.5</td>
<td align="center">886.8</td>
<td align="center">757.4</td>
<td align="center">851.6</td>
<td align="center">1,460</td>
<td align="center">1,926</td>
<td align="center">240</td>
</tr>
<tr>
<td rowspan="4" align="left">
<italic>Rbl. acidophilus</italic>
</td>
<td align="left">LH2 WT<sup>d1,d2,d3,d4</sup>
</td>
<td align="center">870.0</td>
<td align="center">885.0</td>
<td align="center">766.5</td>
<td align="center">861.7</td>
<td align="center">1,442</td>
<td align="center">1,747</td>
<td align="center">120</td>
</tr>
<tr>
<td align="left">m-LH2 WT<sup>d1,d4</sup>
</td>
<td align="center">870.4</td>
<td align="center">NA</td>
<td align="center">766.7</td>
<td align="center">863.9</td>
<td align="center">1,471</td>
<td align="center">NA</td>
<td align="center">NA</td>
</tr>
<tr>
<td align="left">LH2 WT (in PVA)<sup>d4</sup>
</td>
<td align="center">855.6</td>
<td align="center">NA</td>
<td align="center">761.4</td>
<td align="center">847.5</td>
<td align="center">1,332</td>
<td align="center">NA</td>
<td align="center">NA</td>
</tr>
<tr>
<td align="left">LH3 (B800-820)<sup>d2</sup>
</td>
<td align="center">821.4</td>
<td align="center">836.0</td>
<td align="center">738.2</td>
<td align="center">816.5</td>
<td align="center">1,300</td>
<td align="center">1,584</td>
<td align="center">240</td>
</tr>
<tr>
<td rowspan="7" align="left">
<italic>Rba. sphaeroides</italic>
</td>
<td align="left">LH2 WT<sup>d1,d5,</sup>
<xref ref-type="table-fn" rid="Tfn18">
<sup>e</sup>
</xref>
</td>
<td align="center">851.0</td>
<td align="center">864.9</td>
<td align="center">763.2</td>
<td align="center">844.1</td>
<td align="center">1,254</td>
<td align="center">1,542</td>
<td align="center">148</td>
</tr>
<tr>
<td align="left">m-LH2 WT<sup>d1,</sup>
<xref ref-type="table-fn" rid="Tfn18">
<sup>e</sup>
</xref>
</td>
<td align="center">853.1</td>
<td align="center">870.0</td>
<td align="center">763.2</td>
<td align="center">845.8</td>
<td align="center">1,279</td>
<td align="center">1,608</td>
<td align="center">202</td>
</tr>
<tr>
<td align="left">LH2<xref ref-type="table-fn" rid="Tfn19">
<sup>f</sup>
</xref>
</td>
<td align="center">849.7</td>
<td align="center">866.4</td>
<td align="center">762.0</td>
<td align="center">844.5</td>
<td align="center">1,282</td>
<td align="center">1,581</td>
<td align="center">150</td>
</tr>
<tr>
<td align="left">LH2 (B800-less)<sup>d5,</sup>
<xref ref-type="table-fn" rid="Tfn19">
<sup>f</sup>
</xref>
</td>
<td align="center">856.8</td>
<td align="center">873.6</td>
<td align="center">758.1</td>
<td align="center">851.8</td>
<td align="center">1,451</td>
<td align="center">1,744</td>
<td align="center">151</td>
</tr>
<tr>
<td align="left">m-LH2 (B800-less)<xref ref-type="table-fn" rid="Tfn19">
<sup>f</sup>
</xref>
</td>
<td align="center">859.4</td>
<td align="center">877.5</td>
<td align="center">759.5</td>
<td align="center">853.6</td>
<td align="center">1,452</td>
<td align="center">1,771</td>
<td align="center">241</td>
</tr>
<tr>
<td align="left">m-LH2<xref ref-type="table-fn" rid="Tfn20">
<sup>g</sup>
</xref>
</td>
<td align="center">838.3</td>
<td align="center">855.8</td>
<td align="center">758.3</td>
<td align="center">836.6</td>
<td align="center">1,234</td>
<td align="center">1,502</td>
<td align="center">210</td>
</tr>
<tr>
<td align="left">m-LH2<xref ref-type="table-fn" rid="Tfn21">
<sup>h</sup>
</xref>
</td>
<td align="center">827.2</td>
<td align="center">845.7</td>
<td align="center">759.2</td>
<td align="center">826.2</td>
<td align="center">1,068</td>
<td align="center">1,347</td>
<td align="center">232</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn14">
<label>
<sup>a</sup>
</label>
<p>Experimental uncertainty of the measurements: &#xb1;(0.5&#x2013;0.8) nm.</p>
</fn>
<fn id="Tfn15">
<label>
<sup>b</sup>
</label>
<p>Uncertainty of the &#x2206;E and &#x2206;E<sub>0</sub> values: &#xb1;20&#xa0;cm<sup>&#x2212;1</sup>.</p>
</fn>
<fn id="Tfn16">
<label>
<sup>c</sup>
</label>
<p>Experimental uncertainty of the measurements: &#xb1;(10&#x2013;38) cm<sup>&#x2212;1</sup>.</p>
</fn>
<fn id="Tfn17">
<label>
<sup>d</sup>
</label>
<p>References: 1- (<xref ref-type="bibr" rid="B22">Freiberg et al., 2013</xref>), 2- (<xref ref-type="bibr" rid="B26">Freiberg et al., 2010</xref>), 3- (<xref ref-type="bibr" rid="B58">Pajusalu et al., 2011</xref>), 4- (<xref ref-type="bibr" rid="B47">Kunz et al., 2013</xref>), 5- (<xref ref-type="bibr" rid="B84">Timpmann et al., 2004</xref>). For comparability sake, the data obtained in earlier publications have been re-scaled according to the experimental and calculation procedures taken in the present work.</p>
</fn>
<fn id="Tfn18">
<label>
<sup>e</sup>
</label>
<p>Dominant carotenoid spheroidenone.</p>
</fn>
<fn id="Tfn19">
<label>
<sup>f</sup>
</label>
<p>Neurosporene mutant.</p>
</fn>
<fn id="Tfn20">
<label>
<sup>g</sup>
</label>
<p>&#x3b1;&#x2013;H-bond mutant.</p>
</fn>
<fn id="Tfn21">
<label>
<sup>h</sup>
</label>
<p>&#x3b1;&#x3b2;&#x2013;H-bond mutant.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>The concentrated samples were stored at &#x2212;78&#xb0;C in deep freezer. Prior the use the samples were diluted with buffer (20&#xa0;mM Tris-HCl or 20&#xa0;mM HEPES, depending on samples) to meet the required for specific measurements optical density. The buffers for purified complexes additionally contained proper detergent (n-dodecyl &#x3b2;-D-maltopyranoside (DDM), dihexanoylphosphatidylcholine (DHPC), octyl &#x3b2;-glucoside (&#x3b2;OG) or lauryldimethylamine oxide (LDAO)) to prevent aggregation of the proteins. The <italic>Trv</italic>. 970 and <italic>Tch. tepidum</italic> solutions also contained 60&#xa0;mM CaCl<sub>2</sub> to keep samples saturated with Ca<sup>2&#x2b;</sup>. To produce the Ca<sup>2&#x2b;</sup>-depleted samples, EDTA was added and the sample solution was incubated for several hours before the measurements. Glycerol with a 2:1 volume ratio was used to obtain transparent glassy samples at cryogenic temperatures.</p>
</sec>
<sec id="s2-2">
<title>2.2 Spectroscopy</title>
<p>xThe multipurpose spectroscopic setup applied in this work has been recently described (<xref ref-type="bibr" rid="B66">R&#xe4;tsep et al., 2017</xref>; <xref ref-type="bibr" rid="B83">Timpmann et al., 2021</xref>). It comprises a model 3900S Ti: sapphire laser of 0.5 cm<sup>&#x2013;1</sup> linewidth pumped by a Millennia Prime solid-state laser (both Spectra Physics), a 0.3-m focal length spectrograph Shamrock SR-303i, equipped with a thermo-electrically cooled CCD camera DV420A-OE (both Andor Technology) for the measurements of fluorescence excitation anisotropy and hole-burning spectra, and a high-stability broad-band tungsten light source BPS100 (BWTek) for absorption measurements. In the measurements of anisotropy spectra, the vertically polarized laser beam was scanned over a proper wavelength range. The fluorescence spectra were detected through high-contrast analyzing polarizer set parallel or perpendicular to the excitation laser beam. Another correcting polarizer was fixed at 45&#xb0; to the polarization direction of the analyzing polarizer. The estimated experimental uncertainty of the baseline anisotropy value is &#xb1; 0.03. Photobleaching and scattering are potentially detrimental to the quality of anisotropy measurements. To minimize photobleaching, the excitation light flux density was kept as low as feasible for achieving reasonable signal-to-noise ratio. At the experimental power density of 1&#x2013;10&#xa0;mW/cm<sup>2</sup> some amount of photobleaching was only observed when excited in resonance with the main absorption band of the samples, which, however, didn&#x2019;t concern determination of the anisotropy dip positions. Optimization of the sample concentration and blackening of the cuvettes&#x2019; holder were used to curtail the excitation laser-light scattering. The wavelength scale of the spectrometer was determined with a precision of &#xb1; 0.1&#xa0;nm using a Ne&#x2212;Ar calibration lamp. In low-temperature measurements the PMMA plastic cuvettes (Brand) filled with the sample solution were placed into a liquid helium bath cryostat (Utreks). The cryostat was equipped with a temperature controller (model 211 Lakeshore Cryotronics), stabilizing the temperature within &#xb1; 0.5&#xa0;K.</p>
</sec>
<sec id="s2-3">
<title>2.3 Data analysis</title>
<p>The data were analyzed and fitted using the graphing and data analysis software Origin 9.0 SR1 (OriginLab).</p>
</sec>
</sec>
<sec sec-type="results|discussion" id="s3">
<title>3 Results and discussion</title>
<p>For an overview and reading convenience, we will start this Section by presenting the absorption and fluorescence excitation anisotropy spectra of the core (LH1 or LH1-RC) and peripheral (LH2) light-harvesting complexes from WT purple bacteria. We then continue with describing the modifications of these basic spectra caused by the changes of the chromoprotein structure such as due to H-bonding engineering or of environment resulting a detergent purification process. Other spectra/methods will be introduced in proper places. Most of the spectra presented are recorded at low temperature of 4.5&#xa0;K for the sake of improved spectral resolution. Numerical data characterizing excitons in LH1/LH1-RC and LH2 are, respectively, collected into <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>.</p>
<sec id="s3-1">
<title>3.1 Absorption spectra of wild type complexes</title>
<p>Demonstrated in <xref ref-type="fig" rid="F1">Figure 1</xref> are the Q<sub>y</sub> absorption spectra of LH1-RC (<xref ref-type="fig" rid="F1">Figure 1A</xref>) and LH2 (<xref ref-type="fig" rid="F1">Figure 1B</xref>) complexes from selected WT bacteria in the proper light-harvesting exciton spectral range, see below. Broadband version of the absorption spectra spanning from 250&#xa0;nm to 1,100&#xa0;nm can be found in, <xref ref-type="sec" rid="s10">Supplementary Figure 1</xref>. For better comparison, reciprocal (linear in energy) wavelength scale is applied whenever feasible. Also, for the convenience sake, a reference terrestrial solar irradiation spectrum is provided on top of the experimental absorption spectra. It is well-known that the absorption spectra of LH1-RC complexes are in the near-infrared part of the solar spectrum dominated by a sole Q<sub>y</sub> exciton band of LH1, also known as B875. The RC cofactors contribute visibly into this spectrum only around 750 and 850&#xa0;nm, in the high-energy tail of the absorbance of LH1 excitons. Absorption spectra of LH2 complexes encompass two peaks, due to weakly-coupled and strongly-coupled pigments in the B800 and B850 circular arrangements of BChls, respectively.</p>
<p>The peak-normalized spectra in <xref ref-type="fig" rid="F1">Figure 1</xref> demonstrate an exciting spectral tunability of LH1 excitons in different native complexes that almost reaches 100&#xa0;nm. This is much more than the extent observed in the case of B850 (12&#xa0;nm) or B800 (5&#xa0;nm). For the sake of comparison, it is interesting to note that the variations of the Q<sub>y</sub> energy of BChl in polar and nonpolar solvents are about 17&#xa0;nm and 22&#xa0;nm, respectively (<xref ref-type="bibr" rid="B50">Limantara et al., 1997</xref>). As follows, we will concentrate on the properties of the most responsive strongly coupled B875 and B850 excitons.</p>
</sec>
<sec id="s3-2">
<title>3.2 Fluorescence excitation anisotropy spectra of wild type complexes</title>
<p>Presented in <xref ref-type="fig" rid="F2">Figure 2</xref> are the fluorescence excitation anisotropy spectra of the Q<sub>y</sub> excitons in, respectively, LH1/LH1-RC (<xref ref-type="fig" rid="F2">Figure 2A</xref>) and LH2 (<xref ref-type="fig" rid="F2">Figure 2B</xref>) complexes from the same WT bacterial strains as exposed in <xref ref-type="fig" rid="F1">Figure 1</xref>. Shown also with continuous line is absorption spectra of the samples.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Fluorescence excitation anisotropy (colored data points, same color coding as in <xref ref-type="fig" rid="F1">Figure 1</xref>) and absorption (black line) spectra recorded at 4.5&#xa0;K of <italic>Q</italic>
<sub>y</sub> excitons in LH1/LH1-RC <bold>(A)</bold> and LH2 <bold>(B)</bold> complexes of wild type bacterial strains as indicated. Shown in the background are absorption spectra of the samples. The spectra corresponding to different complexes are vertically shifted relative to each other by 0.3 anisotropy units for better visibility. Lines connecting discreet anisotropy data points are here and subsequently drawn for leading the eye. The numbers on top of anisotropy curves indicate &#x2206;E exciton bandwidths.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g002.tif"/>
</fig>
<p>The shape of the anisotropy spectrum generally depends on the recording wavelength, see <xref ref-type="fig" rid="F3">Figure 3</xref>. Being an evidence of a spectrally disordered ensemble of light-harvesting complexes, this effect is the strongest at selective recording in the blue side of the emission spectrum, but almost vanishes when recording at red part, past the maximum of the spectrum, as demonstrated in the inset of <xref ref-type="fig" rid="F3">Figure 3</xref>. Therefore, in order to handle comparable results, selective recording of fluorescence at red side of the spectra with 10-nm bandwidth was commonly applied in the anisotropy measurements.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Variations of the fluorescence excitation anisotropy spectra in dependence of the fluorescence recording wavelength represented in case of the m-&#x394;CrtB carotenoid-less LH1-RC mutant membrane complex of <italic>Rba. sphaeroides</italic>. The anisotropy data designated by blue and red balls are collected selectively, using parts of the emission spectrum indicated by correspondingly colored bars. Exposed in the background are the absorption (blue line) and fluorescence (red line) spectra of the sample. Shown in the inset is the dependence of the blue (left axis) and red (right axis) anisotropy dip positions on the fluorescence recording wavelength.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g003.tif"/>
</fig>
<p>In agreement with the previous work (<xref ref-type="bibr" rid="B84">Timpmann et al., 2004</xref>; <xref ref-type="bibr" rid="B85">Timpmann et al., 2005</xref>), the anisotropy spectra of different cyclic light-harvesting complexes look rather similar. They feature high anisotropy values at the long wavelength edge of the respective absorption spectra that strive towards a theoretical maximum value of 0.4 and two dips towards shorter wavelengths, where anisotropy values close to 0 are generally observed. According to numerical modeling (<xref ref-type="bibr" rid="B86">Trinkunas and Freiberg, 2006</xref>; <xref ref-type="bibr" rid="B58">Pajusalu et al., 2011</xref>) the higher-energy (or blue) anisotropy dip consistently showing up in a relatively narrow spectral range of 760 &#xb1; 10&#xa0;nm rather precisely reproduces the high-energy edge of the Q<sub>y</sub> exciton band, whereas the red dip appears around the strong (k &#x3d; &#xb1;1, &#xb1;2) Q<sub>y</sub> exciton transitions.</p>
<p>Hence, the energy difference &#x2206;E between the blue and red dips, although underestimating the actual exciton bandwidth, can be considered as an effective measure of the exciton bandwidth in cyclic light-harvesting complexes (<xref ref-type="bibr" rid="B84">Timpmann et al., 2004</xref>). As shown in (<xref ref-type="bibr" rid="B85">Timpmann et al., 2005</xref>), a more precise estimation of the exciton bandwidth is obtained as the energy difference &#x2206;E<sub>0</sub> between the blue dip of the anisotropy spectrum and &#x3bb;<sub>0</sub>. The &#x3bb;<sub>0</sub> represents the peak wavelength of the maximum of the inhomogeneous distribution function (IDF) of the lowest-energy k &#x3d; 0 exciton states, which is measured as the peak position of the hole burning action spectrum (<xref ref-type="bibr" rid="B69">Reddy and Small, 1991</xref>). From the &#x2206;E and &#x2206;E<sub>0</sub> data collected in <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>, one can immediately grasp that exciton bandwidths in peripheral complexes are systematically narrower compared with those in core complexes, the ratio changing from about 2/3 in <italic>Rba. sphaeroides</italic> to almost 3/4 in <italic>Rbl. acidophilus</italic>.</p>
</sec>
<sec id="s3-3">
<title>3.3 Impact of the chromoprotein environment and structure</title>
<p>Generally speaking, molecular excitons are sensitive to all physical factors that disturb transition energies of the sites and couplings between them. As follows, we will demonstrate using parallel measurements of fluorescence anisotropy and absorption spectra the responses of the light-harvesting exciton band structure upon altering the environment and internal structure of the chromoproteins. The problem is that in intricate systems such as the chromoproteins studied here, these effects can but rarely be uniquely unraveled. The answer to the question whether one is dealing with environmental or structural property depends on the degree of the effects observed as well as on subjective viewpoint of the investigators. Nevertheless, most researches agree that purification of membrane proteins out of its native membrane by mild detergents, a standard biochemical procedure for studying membrane proteins in isolation, provides a more-or-less pure case of an environmental change, see <xref ref-type="fig" rid="F4">Figure 4</xref>.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Comparison of the fluorescence excitation anisotropy spectra (scattered data points) of Q<sub>y</sub> excitons in detergent-isolated and membrane-embedded LH2 <bold>(A)</bold> and LH1/LH1-RC complexes <bold>(B)</bold> of <italic>Rba. sphaeroides</italic>, as indicated. The multiple anisotropy spectra in panel <bold>(B)</bold> are for better visibility up-shifted with respect to the bottom LH1 spectrum by 0.06 anisotropy units in case of m-LH1, by 0.085 units in case of m-LH1-RC, and by 0.10 units in case of LH1-RC. Shown also with continuous lines are the correspondingly colored and peak-normalized absorption spectra of the samples.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g004.tif"/>
</fig>
<p>Examples of the internal structure variations presented in this work include changes in spatial organization of pigment chromophores illustrated by <xref ref-type="fig" rid="F4">Figure 4B</xref> and <xref ref-type="fig" rid="F5">Figure 5</xref>, in the content of metal ions (<xref ref-type="fig" rid="F6">Figure 6</xref>), in the tertiary structure H-bonding network (<xref ref-type="fig" rid="F7">Figure 7</xref>), and in the type and presence of carotenoids (<xref ref-type="sec" rid="s10">Supplementary Figure 2</xref>).</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Comparison of the fluorescence excitation anisotropy spectra (scattered data points) of Q<sub>y</sub> excitons in wild type (black) and B800-less (red) mutant LH2 complexes from <italic>Rba. sphaeroides</italic>. Shown in the background are correspondingly colored absorption spectra of the samples.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g005.tif"/>
</fig>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Comparison of the fluorescence excitation anisotropy spectra (scattered data points) of <italic>Q</italic>
<sub>y</sub> excitons in WT Ca-containing (black) and Ca-depleted (Ca&#x2013;, red) LH1-RC complexes of <italic>Trv.</italic> 970 <bold>(A)</bold>, and in the complexes of <italic>Tch. tepidum</italic> containing either Ca<sup>2&#x2b;</sup> (Ca&#x2b;, black) or Ba<sup>2&#x2b;</sup> ions (Ba&#x2b;, red) <bold>(B)</bold>. Shown in the background are correspondingly colored absorption spectra of the samples.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g006.tif"/>
</fig>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Assessment of the fluorescence excitation anisotropy spectra (scattered data points) of the <italic>Q</italic>
<sub>y</sub> excitons in native (black) and specific H-bond mutant LH1-RC-pufX <bold>(A)</bold> and LH2 <bold>(B)</bold> complexes (blue and red) from <italic>Rba. sphaeroides</italic> as indicated. Drawn by black line in the background are absorption spectra of the samples, all recorded at 4.5&#xa0;K. See text for further explanations.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g007.tif"/>
</fig>
<p>
<bold>Native membrane-embedded <italic>versus</italic> detergent-isolated chromoproteins</bold>. Shown in <xref ref-type="fig" rid="F4">Figure 4A</xref> are effects of detergent-purification on the absorption and fluorescence anisotropy spectra of LH2 complexes of <italic>Rba. sphaeroides</italic>. As seen, the purification result in subtle but characteristic spectral modifications, which foremost include a couple of nanometers blue-shift and broadening of the Q<sub>y</sub> absorption band. The Q<sub>y</sub> band broadening observed may be caused by 1) the less ordered detergent environment or by 2) the enhanced exciton coupling. The concurrently measured anisotropy spectra that demonstrate narrowing of the exciton band exclude option 2). The weakening of exciton couplings upon the membrane protein purification is also consistent with the common-sense loosening of the protein structure in the surroundings of detergent micelle rather than with tightening. At the same time, as seen in <xref ref-type="table" rid="T3">Table 3</xref>, choice 1) appears to contradict with the much narrower IDF observed in the case of detergent-isolated sample. An obvious solution to this conundrum is that &#x393;<sub>IDF</sub> in native membrane-embedded LH2s is dominated by external disorder, while that in detergent isolated LH2s, by internal disorder. See continuation of this discussion in <xref ref-type="sec" rid="s3-5">Section 3.5</xref>.</p>
<p>The Q<sub>y</sub> band of LH1 complexes similarly broadens in response to detergent-purification, while the exciton band is narrowing (<xref ref-type="fig" rid="F4">Figure 4B</xref>). Yet in this case, internal disorder appears to play leading role because of greater &#x393;<sub>IDF</sub> recorded for purified LH1 complexes, see <xref ref-type="table" rid="T2">Table 2</xref>. Notable also is the much-shifted position of the blue anisotropy dip and somewhat distorted structure of the anisotropy spectrum of purified LH1 complexes compared with those of membrane complexes. Especially the deviating blue anisotropy dip, which we will repeatedly meet below (see <xref ref-type="fig" rid="F5">Figures 5</xref>&#x2013;<xref ref-type="fig" rid="F7">7</xref>), is a sure indicator of structural rearrangements accompanying the various sample handling processes (<xref ref-type="bibr" rid="B26">Freiberg et al., 2010</xref>; <xref ref-type="bibr" rid="B47">Kunz et al., 2013</xref>). Spectral responses following the assembly of LH1 with RC to mimic core LH1-RC complexes in the native membrane environment appear rather small and uncharacteristic, as are the differences between the spectra of native dimeric (LH1-RC-pufX) and monomeric mutant (LH1-RC) core complexes, see <xref ref-type="fig" rid="F4">Figure 4B</xref> and <xref ref-type="table" rid="T2">Table 2</xref>.</p>
<p>Although subtle, important effects of embodiment of bacterial light-harvesting complexes into lipid bilayer have been thus established combining absorption, fluorescence anisotropy and hole-burning techniques. These data add to the mounting previous evidence that some photosynthetic processes may proceed differently in the native membrane, as compared to artificial detergent environment (<xref ref-type="bibr" rid="B6">Bowyer et al., 1985</xref>; <xref ref-type="bibr" rid="B37">Hunter et al., 1985</xref>; <xref ref-type="bibr" rid="B3">Beekman et al., 1997</xref>; <xref ref-type="bibr" rid="B61">Pugh et al., 1998</xref>; <xref ref-type="bibr" rid="B88">Urboniene et al., 2007</xref>; <xref ref-type="bibr" rid="B60">Pflock et al., 2008</xref>; <xref ref-type="bibr" rid="B23">Freiberg et al., 2012b</xref>; <xref ref-type="bibr" rid="B19">Freiberg et al., 2016</xref>). According to data in <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>, the relative exciton band narrowing observed in LH2 and LH1 complexes of different organisms is rather small: 2%&#x2013;3% and 3%&#x2013;9%, respectively. In water-soluble chlorophyll proteins, for example, much stronger environmental effects have been detected (<xref ref-type="bibr" rid="B27">Fresch et al., 2020</xref>).</p>
<p>
<bold>LH2 complex with depleted B800 pigment ring</bold>. <xref ref-type="fig" rid="F5">Figure 5</xref> offers a comparison of the fluorescence excitation anisotropy spectra of Q<sub>y</sub> excitons for the WT and mutant B800-less complexes of LH2 from <italic>Rba. sphaeroides</italic>. Removal of the BChls from the B800 binding sites implicates large perturbation on both the protein spatial structure and the B850 exciton structure, as compared the same characteristics in WT complex. In conformity with this, a 5&#x2013;6&#xa0;nm red-shift of the B850 absorption band was observed, associated with almost 200&#xa0;cm<sup>&#x2013;1</sup> broadening of &#x2206;E (see <xref ref-type="table" rid="T3">Table 3</xref>).</p>
<p>Unfortunately, because of high affinity of B800 binding sites to native as well as to non-native pigments (<xref ref-type="bibr" rid="B79">Swainsbury et al., 2019</xref>), the ambition to prepare the complexes completely free from the B800 site inclusions is untenable. As an example, all the multiple samples in our disposal show different degree of contamination of the B800 sites with the BChl pigments, as shown in <xref ref-type="sec" rid="s10">Supplementary Figure 3</xref>. To our mind, this provides a reasonable explanation for the long-lasting confusion about the variability of the relevant literature data (<xref ref-type="bibr" rid="B49">Leupold et al., 1999</xref>; <xref ref-type="bibr" rid="B84">Timpmann et al., 2004</xref>; <xref ref-type="bibr" rid="B28">Gall et al., 2010</xref>). In particularly, this removes any credibility behind the identification of an upper exciton component in the LH2 complex with depleted B800 of <italic>Rba. sphaeroides</italic> using CD (<xref ref-type="bibr" rid="B46">Koolhaas et al., 1998</xref>).</p>
<p>
<bold>Effects of structurally relevant metal ion inclusions</bold>. Metal ions are frequent embellishments of photosynthetic proteins. However, to the best of our knowledge, only sulfur purple bacteria utilize Ca<sup>2&#x2b;</sup> ions to gain supremacy by extending LH1 spectra maximally towards red. Hence, the Q<sub>y</sub> absorption of LH1 in WT Ca<sup>2&#x2b;</sup> containing <italic>Tch. tepidum</italic> exhibits at ambient temperature a peak at 914&#xa0;nm (<xref ref-type="bibr" rid="B17">Fathir et al., 1998</xref>), while that in <italic>Trv</italic>. 970&#xa0;at record long wavelength of 960&#xa0;nm (<xref ref-type="bibr" rid="B59">Permentier et al., 2001</xref>). The depletion of 16 Ca<sup>2&#x2b;</sup> ions in the C-terminal domain of LH1 complexes results in significant blue-shifting of their absorbance, see <xref ref-type="fig" rid="F6">Figure 6A</xref> and <xref ref-type="table" rid="T2">Table 2</xref>. The new structure is less ordered, confirmed by substantial broadening of both the Q<sub>y</sub> absorption band and IDF. The shift toward higher energies is reversible, so that the original spectra almost precisely recover upon the reconstitution of Ca<sup>2&#x2b;</sup> back into the respective protein structures (<xref ref-type="bibr" rid="B38">Imanishi et al., 2019</xref>). In contrast, the effect of metal ions (Ca<sup>2&#x2b;</sup> or Ba<sup>2&#x2b;</sup>) on the spectra of LH2 complexes is fairly weak, see <xref ref-type="table" rid="T3">Table 3</xref>.</p>
<p>We have previously established an enhancement of exciton couplings as the main mechanism of the Ca-facilitated spectral red-shift (<xref ref-type="bibr" rid="B83">Timpmann et al., 2021</xref>). These data are reproduced in <xref ref-type="fig" rid="F6">Figure 6A</xref>. Shown in <xref ref-type="fig" rid="F6">Figure 6B</xref> is a fresh result of exchange of Ca<sup>2&#x2b;</sup> to Ba<sup>2&#x2b;</sup>, another group IIA alkaline earth metal with slightly greater ion radius. As seen from spectral responses, the effect of ions exchange is much less dramatic than depletion of the ions. This is reasonable, because the ion replacement is expected only slightly distort the native Ca<sup>2&#x2b;</sup> binding sites, while the removal of ions is prone to collapse the sites that may initiate a large-scale restructuring of the protein (<xref ref-type="bibr" rid="B81">Timpmann et al., 2023</xref>). The widely separate positions of the blue anisotropy dips observed in case of <italic>Trv.</italic> 970 complexes and the nearly overlapping dips in case of <italic>Tch. tepidum</italic> complexes support these initial conclusions.</p>
<p>
<bold>Tertiary-structure hydrogen-bonding effects</bold>. Hydrogen bonding applied at different stages of protein folding is vital for stabilization of the protein. A few well-defined tertiary structure H-bonds have been identified, which are instrumental in color tuning of Q<sub>y</sub> bands in LH1 and LH2 complexes (<xref ref-type="bibr" rid="B18">Fowler et al., 1994</xref>; <xref ref-type="bibr" rid="B76">Sturgis et al., 1997</xref>; <xref ref-type="bibr" rid="B77">Sturgis and Robert, 1997</xref>; <xref ref-type="bibr" rid="B41">Kangur et al., 2008</xref>; <xref ref-type="bibr" rid="B89">Uyeda et al., 2010</xref>; <xref ref-type="bibr" rid="B21">Freiberg et al., 2012a</xref>). These first and foremost concern the bonds formed between the conserved tryptophan (Trp) and/or tyrosine (Tyr) protein residues and the C3 acetyl carbonyl group of BChls. According to recent theoretical evaluations, the band shifts created are due to joint effect of the dihedral angle of the acetyl moiety and the shuttling of the proton in the H-bond (<xref ref-type="bibr" rid="B15">De Vico et al., 2018</xref>).</p>
<p>Any adjustment of the H-bonding pattern necessarily involves transformation of the ground and excited electronic state structures of the excitonically coupled aggregates, hence their exciton properties. A straightforward way to demonstrate this is by direct comparison of the exciton state bandwidths, as revealed by fluorescence excitation anisotropy (data in <xref ref-type="table" rid="T2">Tables 2</xref>, <xref ref-type="table" rid="T3">3</xref>).</p>
<p>
<xref ref-type="fig" rid="F7">Figure 7</xref> provides examples of anisotropy spectra in case of WT and various H-bond mutant LH1-RC and LH2 complexes from <italic>Rba. sphaeroides</italic>. In the LH1-RC complex, one of these mutations (&#x3b1;Trp<sub>&#x2b;11</sub>Phe, termed &#x3b1;-mutant in <xref ref-type="fig" rid="F7">Figure 7A</xref>), replaces the tryptophan that H-bonds to the C3 acetyl carbonyl group of one of the BChls in a &#x3b1;&#x3b2;-BChl<sub>2</sub> apoprotein unit, disrupting the H-bond, while another (&#x3b2;Trp<sub>&#x2b;9</sub>Phe, &#x3b2;-mutant), disrupts the H-bond to the C3 acetyl carbonyl of the pairing BChl. Double mutant core complexes with replacements in both sites are structurally compromised and are unstable in detergent. For LH2 only membrane-embedded complexes are available carrying the H-bond breaking single (&#x3b1;Tyr44Phe, &#x3b1;-mutant) or double (&#x3b1;Tyr44Phe-&#x3b1;Tyr45Leu, &#x3b1;&#x3b2;-mutant) residue replacements.</p>
<p>In agreement with the previous knowledge (<xref ref-type="bibr" rid="B18">Fowler et al., 1994</xref>), the disruption of particular H-bonds results in blue-shifting of the absorption spectra in comparison with the spectrum of the WT complex. With one notable exception, these spectral shifts are according to expectation accompanied by exciton band narrowing. Except the &#x3b2;-mutant of LH1-RC-pufX, which shows broadening, not narrowing of the exciton bandwidth. Although quantitative evaluation of this effect awaits to be done, the shift of the blue side anisotropy dip allows to conclude that the replacement of the residue at the &#x3b2;<sub>&#x2b;9</sub> position causes greater amount of structural rearrangements in LH1 than the replacement at the &#x3b1;<sub>&#x2b;11</sub> position, confirming a prior notion obtained from analyses of Raman spectra (<xref ref-type="bibr" rid="B76">Sturgis et al., 1997</xref>).</p>
<p>
<bold>Carotenoid depletion or exchange</bold>. The significance of carotenoids in the assembly and reinforcement of light-harvesting protein structures is widely recognized (<xref ref-type="bibr" rid="B51">Loach and Parkes-Loach, 2008</xref>). Yet the role carotenoids play in modulation of the light-harvesting exciton properties is less well documented. Here, we have been assessing the consequences of carotenoid exchange or depletion in a number of bacterial light-harvesting complexes. The results obtained are collected in <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>, being also partially illustrated by <xref ref-type="sec" rid="s10">Supplementary Figure 2</xref>.</p>
<p>
<xref ref-type="sec" rid="s10">Supplementary Figure 2</xref> shows that the depletion of carotenoids from either LH1 or LH2 complexes has by far greater impact on light-harvesting excitons than their exchange. The exchange such as demonstrated in <xref ref-type="sec" rid="s10">Supplementary Figure 2A</xref> generally well keeps the structure of the exciton band. However, collapse of the voids subsequent to removal of carotenoid and the accompanying relaxation of the B850/B875 pigment assembles may (as shown in <xref ref-type="sec" rid="s10">Supplementary Figure 2B</xref>) or may not (<xref ref-type="sec" rid="s10">Supplementary Figure 2C</xref>) save the intact exciton structure.</p>
</sec>
<sec id="s3-4">
<title>3.4 Validation of the top exciton band edge by CD and fluorescence excitation spectroscopy</title>
<p>As it was presented in Introduction, attempts have been made to reveal the electronic structure of BChl excitons in LH2 and LH1 complexes by other experimental techniques, apart from polarized fluorescence spectroscopy. Especially CD method has been popular, because the structure-based model calculations promise clear CD signatures related to both red and blue exciton band edges of light-harvesting complexes that contain cyclic B850/B875 aggregates of BChls. These attempts, however, have all failed in intact peripheral and core light-harvesting units. Not so much because the expected weakness of the CD signal corresponding to the top of the exciton band, but more typically because of unfortunate spectral overlaps with other complements of these units such as RC in LH1-RC or B800 in LH2, which both overwhelmingly contribute into the CD spectra in the spectral range of interest.</p>
<p>Since the efforts to fix the LH2 complexes sufficiently free of B800 pigments proved unsuccessful, we were paying attention to purified LH1 complexes free of RC. In these complexes, a weak negative CD band was previously observed around 754&#xa0;nm at 77&#xa0;K and around 763&#xa0;nm at room temperature (<xref ref-type="bibr" rid="B32">Georgakopoulou et al., 2006b</xref>). According to exciton modeling, these features were ascribed to the high-energy exciton component of the Q<sub>y</sub> band.</p>
<p>
<xref ref-type="fig" rid="F8">Figure 8A</xref> confronts the CD spectrum of the LH1 complex from <italic>Rba. sphaeroides</italic> measured in this work at 77&#xa0;K with its fluorescence anisotropy spectrum recorded at 4.5&#xa0;K. Let us note that the CD spectrum of our sample precisely reproduces the already published spectra (<xref ref-type="bibr" rid="B31">Georgakopoulou et al., 2006a</xref>; <xref ref-type="bibr" rid="B32">Georgakopoulou et al., 2006b</xref>). The close match observed between the location of the CD and anisotropy dips reconfirms that the latter can be considered as an adequate measure of the top exciton band position.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>
<bold>(A)</bold> Comparison of the CD spectrum (continuous line, recorded at 77&#xa0;K) and the fluorescence excitation anisotropy spectrum (scattered data points, recorded at 4.5&#xa0;K (same data as in <xref ref-type="fig" rid="F4">Figure 4B</xref>)) of Q<sub>y</sub> excitons in detergent-isolated LH1 complexes from <italic>Rba. sphaeroides</italic>. <bold>(B)</bold> Comparison of the absorptance (1&#x2013;T, black line) and fluorescence excitation (red dots, recorded at 995&#x2013;1,040&#xa0;nm) spectra of the LH1-RC complex from Trv. 970&#xa0;at 4.5&#xa0;K. The inset shows detailed view of the congested spectral region around the top of the LH1 exciton band with dominating absorption by RC pigments. Shown with scattered blue rings is the fluorescence anisotropy data.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g008.tif"/>
</fig>
<p>The measurements of fluorescence excitation spectra provide yet another independent validation of the fluorescence anisotropy technique. Demonstrated in <xref ref-type="fig" rid="F8">Figure 8B</xref> is the experimental determination of the top exciton band edge in the intact LH1-RC core complex from <italic>Trv</italic>. 970, in which case the CD method fails totally. The inset represents the blow-up version of the figure in the spectral region of the LH1 exciton band top, where the 1&#x2013;T spectrum is dominated by the RC absorbance.</p>
<p>As seen, the photons absorbed at cryogenic temperatures by the RC get trapped and do not practically contribute into the LH1 exciton fluorescence. This exposes a rather weak (&#x223C;235-fold smaller than the main Q<sub>y</sub> exciton absorption band at 987&#xa0;nm) absorption band peaking at 772&#xa0;nm. Exact overlap with the high-energy anisotropy dip allows this band to be assigned to the exiton states at the very top of the exciton band.</p>
</sec>
<sec id="s3-5">
<title>3.5 Correlation between the Q<sub>y</sub> exciton bands and absorption spectra</title>
<p>Having determined the boundaries of the Q<sub>y</sub> exciton state manifolds for all the 33 light-harvesting complexes studied, as represented in <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>, it would be instrumental to plot the exciton bandwidths as a function of the Q<sub>y</sub> absorption peak energy, E (<xref ref-type="fig" rid="F9">Figure 9</xref>). The graphs are presented separately for the &#x2206;E (<xref ref-type="fig" rid="F9">Figure 9B</xref>) and &#x2206;E<sub>0</sub> (<xref ref-type="fig" rid="F9">Figure 9C</xref>) bandwidth definitions. They draw (almost) parallel lines, establishing linear negative correlations between the exciton bandwidths and the E. This means that the complexes with broader bandwidths (with stronger coupled excitons) are adapted to absorb lower-energy (redder) light and <italic>vice versa</italic>. A spectral division of the complexes into two major groups (LH1/LH1-RC core complexes and LH2 peripheral complexes) can also be clearly seen in <xref ref-type="fig" rid="F9">Figures 9B, C</xref>. In energy terms, the color-tuning range of core complexes (1,481&#xa0;cm<sup>&#x2013;1</sup>) is almost twice greater than that of LH2 complexes (752&#xa0;cm<sup>&#x2013;1</sup>).</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>
<bold>(A)</bold> The &#x2206;E and &#x2206;E<sub>0</sub> measures of exciton bandwidth (designated by horizontal lines), illustrated in case of LH1-RC (Ca&#x2013;) complexes of <italic>Trv</italic>. 970. The approximately Gaussian-shape IDF band (cyan) is arbitrarily scaled with respect to normalized absorption (blue) and fluorescence (red, excited non-resonantly at 407&#xa0;nm) spectra in the background. <bold>(B, C)</bold> Correlation observed between the exciton bandwidths &#x2206;E <bold>(B)</bold> and &#x2206;E<sub>0</sub> <bold>(C)</bold>, and the position of the Q<sub>y</sub> exciton absorption band maximum E<sub>Q</sub> for the LH1/LH1-RC (red-colored data points) and LH2 (blue-colored data points) complexes. Shown with lines are linear regressions of the data. The data for the LH3 complex from <italic>Rbl. acidophilus</italic> is marked by arrow.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g009.tif"/>
</fig>
<p>The &#x2206;E<sub>0</sub> exciton bandwidths as a function of E well follow a linear function: &#x2206;E<sub>0</sub> &#x3d; 11,700&#x2013;0.850 &#xd7; E. A great practical value of this insight is that exciton bandwidths (thus the exciton couplings) and their changes can be readily evaluated with reasonable accuracy using simple measurements of absorption spectra. We have verified that the data that appear deviating from the above linear law correspond to structurally modified complexes, the LH3 complex from <italic>Rbl. acidophilus</italic> being an extreme case. Note, however, that this deceivingly simple relationship determined at 4.5&#xa0;K is not expected to hold at elevated temperatures, because of thermally-induced variations of site energies, exciton coupling energies as well as the structure of the chromoprotein complexes in certain cases (<xref ref-type="bibr" rid="B65">R&#xe4;tsep et al., 2018</xref>). Additional investigations are, therefore, required to find the bandwidth dependences on temperature (<xref ref-type="bibr" rid="B58">Pajusalu et al., 2011</xref>; <xref ref-type="bibr" rid="B22">Freiberg et al., 2013</xref>).</p>
<p>The exciton bandwidths recoded in the LH1/LH1-RC core complexes vary between 3,005 and 1,857&#xa0;cm<sup>&#x2013;1</sup>, while those in LH2 peripheral complexes, between 2,013 and 1,347&#xa0;cm<sup>&#x2013;1</sup>. The exciton couplings energies can be deduced from a &#x201c;rule of thumb&#x201d; equation, &#x2206;E<sub>0</sub> &#x2248; 2 (V<sub>1</sub>&#x2b;V<sub>2</sub>), of a model dimerized BChl chain in nearest-neighbor approximation, where V<sub>1</sub> and V<sub>2</sub> are the intra- and inter-dimer coupling energies. Assuming V<sub>1</sub> &#x2248; V<sub>2</sub>, the low-temperature coupling energies may thus reach about 750&#xa0;cm<sup>&#x2013;1</sup> in LH1/LH1-RC and about 500&#xa0;cm<sup>&#x2013;1</sup> in LH2.</p>
<p>The formation of excitons is usually accompanied by sharpening of monomer spectra, a celebrated example being J-aggregates (<xref ref-type="bibr" rid="B34">Hestand and Spano, 2018</xref>). The degree of exciton line narrowing is a function of the ratio &#x393;<sub>m</sub>/V, where &#x393;<sub>m</sub> is the width of the inhomogeneously broadened monomer spectrum and V &#x3d; (V<sub>1</sub>&#x2b;V<sub>2</sub>)/2. Therefore, it is expected that the complexes with stronger coupling expose narrower IDF, a results of the so-called exciton motional narrowing effect (<xref ref-type="bibr" rid="B45">Knapp, 1984</xref>). This qualitative expectation is indeed roughly followed by our data, see <xref ref-type="sec" rid="s10">Supplementary Figure 4</xref>. It also appears reasonable that the relatively weaker-coupled LH2 complexes are more widely spread with respect to the average value of &#x393;<sub>IDF</sub>. Yet in several cases such as LH1-RC (Ca&#x2212;) of <italic>Trv</italic>. 970, LH1-RC (Ba&#x2b;) of <italic>Tch. tepidum</italic>, LH2 of <italic>E. haloalkaliphila</italic>, and all membrane-embedded LH2 complexes of <italic>Rba. sphaeroides</italic>, anomalously broad IDFs (&#x393;<sub>IDF</sub> &#x2265; 200&#xa0;cm<sup>&#x2013;1</sup>) are observed, see <xref ref-type="table" rid="T2">Table 2</xref> and <xref ref-type="table" rid="T3">Table 3</xref>.</p>
<p>In the literature, the width &#x393;<sub>IDF</sub> has been widely considered as a proper measure of the exciton disorder (<xref ref-type="bibr" rid="B68">Reddy et al., 1992</xref>; <xref ref-type="bibr" rid="B62">Purchase and V&#xf6;lker, 2009</xref>). This is not quite correct, because in the chromoprotein systems two qualitatively different types of spectral disorders have been identified, one caused by intra-protein (or internal) and second, due to inter-protein (external) variations (<xref ref-type="bibr" rid="B25">Freiberg et al., 1999</xref>), whereas only the former component is subject to motional narrowing. The systems with anomalously broad IDFs listed above thus apparently belong into the realm governed by external disorder.</p>
<p>The phototropic bacteria that in addition to core complexes contain peripheral light-harvesting complexes have to carefully tune their respective spectra to achieve optimal transport of excitons towards RCs. As can be seen from <xref ref-type="fig" rid="F10">Figure 10</xref> and <xref ref-type="sec" rid="s10">Supplementary Figure 5</xref>, the exciton state manifolds in core and peripheral complexes perfectly match each other, whereby the high-energy edges of the exciton state manifolds in LH1 and LH2 nearly coincide. These facts were noticed years ago (<xref ref-type="bibr" rid="B22">Freiberg et al., 2013</xref>), but their comprehensiveness wasn&#x2019;t immediately evident.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Overlap of exciton bands at 4.5&#xa0;K of LH1-RC and LH2 complexes in the whole photosynthetic membranes of <italic>Rbl. acidophilus</italic> <bold>(A)</bold> and in a mixture of <italic>Tch. tepidum</italic> complexes containing Ba<sup>2&#x2b;</sup> <bold>(B)</bold>. Shown in the background are peak-normalized absorption (blue) and fluorescence (red) spectra of the samples. The colored anisotropy data points are obtained by integrating fluorescence over the corresponding colored bar areas. The lines connecting data points are to lead the eye. See text for further details.</p>
</caption>
<graphic xlink:href="fchem-11-1231431-g010.tif"/>
</fig>
</sec>
</sec>
<sec id="s4">
<title>4 Summary and concluding remarks</title>
<p>Exciton phenomena play a fundamental role in photosynthesis, yet surprisingly, there is a lack of quantitative information obtained directly from experimental studies regarding exciton parameters. The current research addresses this gap by developing an experimental methodology to characterize excitons in cyclic light-harvesting chromoprotein complexes found in photosynthetic purple bacteria. By conducting measurements on 17 core complexes and 16 peripheral complexes, we establish a robust linear correlation between the exciton bandwidth and the positions of the lowest-energy exciton absorption band. This absorption band, associated with Q<sub>y</sub> electronic transitions in BChl pigments, holds significant importance for photosynthetic exciton transport and trapping. Our findings thus importantly confirm the crucial role of excitons in expanding the spectral range of bacterial light-harvesting. Furthermore, the simple relationship (an &#x201c;exciton ruler&#x201d;) identified across the entire class of photosynthetic purple bacterial species enables valuable benchmarking of calculated exciton parameters through straightforward absorption spectrum measurements.</p>
<p>The fluorescence excitation anisotropy method reveals the sensitivity of the blue anisotropy dip to structural changes in the light-harvesting complexes, providing an added advantage. The observation that most modifications to the chromoproteins result in a reduction of exciton bandwidth suggests that the inherent structures of purple bacterial light-harvesting complexes are optimally designed for their function.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="sec" rid="s10">Supplementary Material</xref>, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s6">
<title>Author contributions</title>
<p>KT and MR performed the experimental measurements and data analyses, AF designed the research and wrote the manuscript. All authors contributed to the article and approved the submitted version.</p>
</sec>
<sec id="s7">
<title>Funding</title>
<p>This research was supported by the Estonian Research Council, Grant Number PRG664.</p>
</sec>
<ack>
<p>The samples studied were generously donated by Profs. R. Cogdell (Glasgow University), C. N. Hunter (Sheffield University), A. A. Moskalenko (IBBP, Pushchino), Z-Y. Wang-Otomo (Ibaraki University), and N. Woodbury (Arizona State University). L. Kangur, A. Lehtmets, K. Leiger, and M. Pajusalu contributed to this work at different phases of the research. The authors also acknowledge useful discussions with E. Jalviste and J. M. Linnanto concerning the aspects of modeling the light-harvesting exciton spectra.</p>
</ack>
<sec sec-type="COI-statement" id="s8">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s9">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<sec id="s10">
<title>Supplementary material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/fchem.2023.1231431/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/fchem.2023.1231431/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet1.PDF" id="SM1" mimetype="application/PDF" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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