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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Astron. Space Sci.</journal-id>
<journal-title>Frontiers in Astronomy and Space Sciences</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Astron. Space Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-987X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">571282</article-id>
<article-id pub-id-type="doi">10.3389/fspas.2021.571282</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Astronomy and Space Sciences</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Prelude to Simulations of Loop Quantum Gravity on Adiabatic Quantum Computers</article-title>
<alt-title alt-title-type="left-running-head">Mielczarek</alt-title>
<alt-title alt-title-type="right-running-head">Quantum Gravity on Quantum Annealer</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Mielczarek</surname>
<given-names>Jakub</given-names>
</name>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/763099/overview"/>
</contrib>
</contrib-group>
<aff>Institute of Theoretical Physics, Jagiellonian University, <addr-line>Krak&#xf3;w</addr-line>, <country>Poland</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/77247/overview">Jan De Boer</ext-link>, University of Amsterdam, Netherlands</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/515463/overview">Francesca Vidotto</ext-link>, Western University, Canada</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/299880/overview">Sayantan Choudhury</ext-link>, National Institute of Science Education and Research (NISER), India</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Jakub Mielczarek, <email>jakub.mielczarek@uj.edu.pl</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to High-Energy and Astroparticle Physics, a section of the journal Frontiers in Astronomy and Space Sciences</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>10</day>
<month>06</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="collection">
<year>2021</year>
</pub-date>
<volume>8</volume>
<elocation-id>571282</elocation-id>
<history>
<date date-type="received">
<day>10</day>
<month>06</month>
<year>2020</year>
</date>
<date date-type="accepted">
<day>25</day>
<month>05</month>
<year>2021</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2021 Mielczarek.</copyright-statement>
<copyright-year>2021</copyright-year>
<copyright-holder>Mielczarek</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&#x20;terms.</p>
</license>
</permissions>
<abstract>
<p>The article addresses the possibility of implementing spin network states, used in the loop quantum gravity approach to Planck scale physics on an adiabatic quantum computer. The discussion focuses on applying currently available technologies and analyzes a concrete example of a D-Wave machine. It is introduced a class of simple spin network states which can be implemented on the Chimera graph architecture of the D-Wave quantum processor. However, extension beyond the currently available quantum processor topologies is required to simulate more sophisticated spin network states. This may inspire new generations of adiabatic quantum computers. A possibility of simulating loop quantum gravity is discussed, and a method of solving a graph non-changing scalar (Hamiltonian) constraint with the use of adiabatic quantum computations is proposed. The presented results establish a basis for the future simulations of Planck scale physics, specifically quantum cosmological configurations, on quantum annealers.</p>
</abstract>
<kwd-group>
<kwd>quantum gravity</kwd>
<kwd>quantum computation</kwd>
<kwd>Planck scale</kwd>
<kwd>quantum annealing</kwd>
<kwd>adiabatic quantum algorithm</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>One can distinguish two main applications of quantum computers. The first is data processing associated with the implementation of quantum algorithms, e.g., quantum machine learning protocols (<xref ref-type="bibr" rid="B5">Biamonte et&#x20;al., 2017</xref>). The second concerns simulations of quantum systems.</p>
<p>Simulating quantum systems using quantum computers is fundamentally different from what simulations performed at classical computers are. While classical simulations rely on either discretization of a given physical system or an adequate algebraic analysis, the simulations performed on quantum computers allow to <italic>imitate</italic> a given quantum system. This kind of <italic>exact simulation</italic> of a quantum system has been a subject of discussion in the seminal Feynman&#x2019;s article (<xref ref-type="bibr" rid="B9">Feynman, 1982</xref>).</p>
<p>In order to understand better what we mean by exact simulations, let us consider the case of Planck scale physics. Here, the relevant degrees of freedom are defined at length scales of the order of the Planck length <inline-formula id="inf1">
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</inline-formula>. Despite significant advances made in theoretical understanding and experimental techniques, the Planck scale physics remains empirically directly inaccessible.</p>
<p>On the other hand, concrete examples of theories describing elementary quantum gravitational degrees of freedom exist. One such approach is loop quantum gravity (LQG) (<xref ref-type="bibr" rid="B20">Rovelli, 1998</xref>; <xref ref-type="bibr" rid="B2">Ashtekar and Lewandowski, 2004</xref>; <xref ref-type="bibr" rid="B22">Rovelli and Vidotto, 2014</xref>). In LQG, background-independent degrees of freedom can be defined, and predictions can be made (<xref ref-type="bibr" rid="B1">Agullo et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B4">Barrau et&#x20;al., 2014</xref>). Even if the degrees of freedom under consideration are experimentally not directly accessible, one can consider their <italic>projection</italic> onto another physical realization, which will imitate its quantum behavior (see <xref ref-type="fig" rid="F1">Figure&#x20;1</xref>). Under the assumption that quantum mechanics is valid at the Planck scale, the projected realization is quantum-mechanically equivalent to the original system. The only difference is appropriately rescaled couplings adjusted to the physical nature of the simulator (built, e.g., with the use of superconducting qubits). Such projection of one quantum system onto its equivalent imitation allows performing what we previously called exact simulations. As it has already been mentioned, the quantum simulations are very different from what we usually consider as physical simulations, where for instance, a given differential equation is discretized and then implemented on a computer with the use of appropriate algorithms. In contrast, in the case of exact simulations, one actually performs experiments on a quantum system which is defined as being equivalent (quantum mechanically) to a part (or a whole) of the original quantum system.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Pictorial presentation of the relation between the original quantum system defined at the Planck scales and its exact simulation. The exact simulation is performed with the use of projection of the original quantum system onto the architecture of a quantum computer. In contrast to the Planck scale system, measurements of the quantum degrees of freedom can be performed at the level of the quantum simulation.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g001.tif"/>
</fig>
<p>The aim of this article is to investigate the possibility of performing exact quantum simulations of the spin network states, which are used to construct the Hilbert space in the LQG approach to quantum gravity. Our interest is focused on applying existing adiabatic quantum computers, a commercial example of which is one provided by the D-Wave Systems company.</p>
<p>We consider conceptual issues related to the possibility of simulating Loop Quantum Gravity based on the considered fixed graph case. Specifically, the implementation of the scalar constraint is analyzed, and a toy model of such a procedure is presented. We conclude with an outlook of the following steps to be done in the research direction initiated in this article.</p>
<p>The idea of employing the spin network states in quantum computations already appeared in the literature [see Refs <xref ref-type="bibr" rid="B17">Marzuoli and Rasetti (2005)</xref>, <xref ref-type="bibr" rid="B14">Kauffman and Lomonaco (2008)</xref>, <xref ref-type="bibr" rid="B12">Jordan (2010)</xref>]. However, the potential of applying spin networks for universal quantum data processing was considered only. Up to the best of our knowledge, the issue of relating spin networks with adiabatic quantum computations was not considered before. While this article was in the final stage of preparing a study in which an LQG spin network is implemented on a molecular quantum simulator appeared. A simulation of quantum fluctuations of a 5-node spin network in the kinematical regime was performed (<xref ref-type="bibr" rid="B15">Li et&#x20;al., 2019</xref>). Here, we will consider the same type of spin network in <xref ref-type="sec" rid="s4">Section 4</xref> in the context of solving a prototype scalar constraint with the use of adiabatic quantum computations.</p>
</sec>
<sec id="s2">
<title>2 Adiabatic Quantum Computing</title>
<p>The last years have brought significant progress in the development of quantum computing technologies (<xref ref-type="bibr" rid="B6">Campbell et&#x20;al., 2017</xref>). First, quantum computers have been commercialized and made available in a cloud or as independent hardware units. In both cases, the currently most advanced commercial technologies were possible to achieve thanks to the development of superconducting quantum circuits (<xref ref-type="bibr" rid="B24">You and Nori, 2005</xref>). In particular, the IBM Q universal quantum computers built using 5 and 20 superconducting qubits have been developed. However, from the point of view of exact simulations discussed in the Introduction, another type of quantum computer seems to be more suitable to use currently&#x2014;namely the <italic>adiabatic quantum computers</italic> (<xref ref-type="bibr" rid="B13">Kadowaki and Nishimori, 1998</xref>).</p>
<p>Adiabatic quantum computers, in contrast to the universal ones, are designed to solve a specific problem of finding the minimum of a Hamiltonian <inline-formula id="inf2">
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</inline-formula> of a coupled system of qubits (spins). In the process of finding the minimum of <inline-formula id="inf3">
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<label>(1)</label>
</disp-formula>where <inline-formula id="inf4">
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</inline-formula> is the so-called base Hamiltonian, which is characterized by a simple and easy to prepare ground state. In practice, the base Hamiltonian is often equal to <inline-formula id="inf5">
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</inline-formula>, so that the ground state corresponds to the alignment of spins in the <italic>x</italic> direction. Then, the value of <italic>&#x3bb;</italic> is changed adiabatically from <inline-formula id="inf6">
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</inline-formula> Hamiltonian is considered. This issue is closely related to the efficiency of the quantum annealing-based algorithms to the classical ones [see Ref <xref ref-type="bibr" rid="B5">Biamonte et&#x20;al. (2017)</xref>] for discussion of this subject).</p>
<p>In practical implementations, the most considered form of <inline-formula id="inf12">
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<p>where <inline-formula id="inf13">
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<p>From the mathematical viewpoint, the class of problems which can be solved in that way is the so-called Quadratic Unconstrained Binary Optimization (QUBO), which typically is of the NP-hard type. This is because, when we look a the problem from the classical perspective by measuring the orientations of spins along the <italic>z</italic>-axis, the two values of <inline-formula id="inf16">
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<p>The physical implementation of the QUBO problem using the quantum annealing procedure is provided by the D-Wave machine. In this realization, the spins (qubits) are created with the use of superconducting circuits in the form of CC JJ RF-SQUIDs (<xref ref-type="bibr" rid="B10">Harris et&#x20;al., 2010</xref>) built with the use of Josephson junctions composed of Niobium in the superconducting state. The qubit basis states are defined employing two different orientations of quantum of magnetic flux across the superconducting circuit. SQUID (superconducting quantum interference device) introduces interactions between the qubits based circuits called <italic>couplers</italic>, which introduce the <inline-formula id="inf18">
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</inline-formula>. The readout of the final quantum states of qubits is performed with the use of sensitive magnetometers built with the use of SQUIDs.</p>
<p>In the D-Wave quantum annealer, the superconducting qubits <inline-formula id="inf23">
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</inline-formula> are arranged into 8-qubit blocks forming the so-called <italic>Chimera</italic> architecture. Each block consists of 16 couplings between 8 spins. As a consequence, not all qubits are coupled. The topology of couplings between qubits in a single block is presented in <xref ref-type="fig" rid="F2">Figure&#x20;2</xref>. In the so far most advanced version of the D-Wave machine (the D-Wave 2000) the 8-qubit blocks form a 16&#x20;&#xd7; 16 matrix (256 blocks in total), leading to 2048 qubits.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Three different representations of the structure of couplings between eight <inline-formula id="inf24">
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</inline-formula> qubits forming an elementary block of the D-Wave processor: <bold>(A)</bold> The physical representation of quibits as closed superconducting loops. The couplers between the qubits are represented by triangles. <bold>(B)</bold> The Chimera graph structure of couplings between the eight qubits. <bold>(C)</bold> Representation of a single block which is useful when interconnections in the array of blocks are considered.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g002.tif"/>
</fig>
</sec>
<sec id="s3">
<title>3 Spin Networks</title>
<p>Let us now proceed to discuss spin networks. We begin with a brief overview of how spin networks appear in the loop quantum gravity approach to quantum gravity. Then we introduce a class of spin networks that is possible to implement on the Chimera architecture of D-Wave quantum processors.</p>
<p>The fundamental elements of the LQG approach to quantum gravity are holonomies of Ashtekar connection <inline-formula id="inf25">
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<p>where <inline-formula id="inf28">
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<p>The key idea behind LQG is to build a Hilbert space of the theory out of Wilson loops. However, such a basis is, in general, over-complete. A solution to the problem comes from the construction of <italic>spin-networks</italic> which are a certain linear combination of products of Wilson loops (<xref ref-type="bibr" rid="B21">Rovelli and Smolin, 1990</xref>). Such an approach guarantees that both the Gauss constraint (ensuring local gauge invariance) is satisfied by the base states, and the Hilbert space is complete. By introducing an equivalence relation between topologically equivalent spin networks, the so-called diffeomorphism constraint can be satisfied. There is eventually a scalar (Hamiltonian) constraint, which has to be satisfied by physical states. In this section, we will focus on spin network states satisfying both Gauss and diffeomorphism constraints. The issue of satisfying the scalar constraint (with the use of adiabatic quantum computing) will be discussed in the next section.</p>
<p>The spin network is formally a graph composed of edges <italic>E</italic> and nodes <italic>N</italic> with spin labels at the edges and the so-called <italic>intertwiners</italic> at the nodes. The spin labels correspond to irreducible representations of the <inline-formula id="inf32">
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</inline-formula> group such that triangle inequalities (reflecting the Gauss constraint) are satisfied at the nodes. The intertwiners correspond to invariant subspaces at the nodes, which we will discuss in more detail&#x20;below.</p>
<p>In <xref ref-type="fig" rid="F3">Figure&#x20;3</xref> we present an exemplary spin network composed of 3-valent and 4-valent nodes. An essential feature of the nodes is that 3-valent nodes do not carry a volume element while 4-valent nodes and higher valent nodes are associated with 3-volume (in the sense that eigenvalues of the volume operator in such a state are non-vanishing).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>
<bold>A)</bold> An exemplary spin network. <bold>(B)</bold> In the geometric picture the 4-valent node is dual to a tetrahedron (3-simplex).</p>
</caption>
<graphic xlink:href="fspas-08-571282-g003.tif"/>
</fig>
<p>The particular case is a 4-valent node that is dual to a tetrahedron (3-simplex). One can imagine that the vertex is located in the center of the tetrahedra, while each of the associated links intersects with one of the surfaces (see block b) in <xref ref-type="fig" rid="F3">Figure&#x20;3</xref>).</p>
<p>In this article, we are considering the case of spin networks composed of 4-valent vertices only and spin labels corresponding to fundamental representations of the <inline-formula id="inf33">
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</inline-formula>. The reason for that is that in such a case, the Hilbert space at each vertex is a tensor product of four 1/2 spins, which can be decomposed into irreducible representations in the following way:<disp-formula id="e4">
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<p>There are, therefore, two possibilities in which the spins can add up to zero. In consequence, the invariant subspace for such a vertex is two dimensional:<disp-formula id="e5">
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<p>We associate the two dimensional invariant space with the qubit space. The nature of the qubit associated with the 4-vertex under consideration is graphically presented in <xref ref-type="fig" rid="F4">Figure&#x20;4</xref>.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>The 4-valent node with spin labels equal to <inline-formula id="inf35">
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</caption>
<graphic xlink:href="fspas-08-571282-g004.tif"/>
</fig>
<p>Worth mentioning here is that there is a freedom of choice of channel in which recoupling of spin labels at the vertex is performed. In particular, in the <italic>s</italic> channel the base states can be expressed in terms of the four <inline-formula id="inf36">
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</disp-formula>
</p>
<p>The above definitions of the basis states for a qubit have recently been considered in the context of universal quantum computations in Refs. <xref ref-type="bibr" rid="B15">Li et&#x20;al. (2019)</xref>, <xref ref-type="bibr" rid="B19">Mielczarek (2019)</xref>, <xref ref-type="bibr" rid="B7">Czelusta and Mielczarek (2021)</xref>. Alternatively, it is convenient to construct our qubit states such that they are eigenvectors of the volume operator [see e.g. Ref <xref ref-type="bibr" rid="B8">Feller and Livine (2016)</xref> for details]:<disp-formula id="e7">
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<label>(8)</label>
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</inline-formula> is&#x20;the minimal eigenvalue of the volume operator (<xref ref-type="bibr" rid="B22">Rovelli and Vidotto, 2014</xref>). The positive and negative signs of the eigenvalues distinguish between the two allowed orientations of a 3-simplex. Consequently, in LQG, the elementary volume can contribute with both signs: positive (for <inline-formula id="inf46">
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</inline-formula>). However, it is expected that in the semiclassical limit, one of the contributions will dominate over the other. The eigenstates <inline-formula id="inf48">
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</inline-formula> are the qubit base states that we refer to in the rest of this article.</p>
<p>Having the definition of a qubit, one can consider different spin network topologies that are possible to implement directly with Chimera architecture. In <xref ref-type="fig" rid="F5">Figure&#x20;5</xref> we present connected spin networks with the number of nodes equal to <inline-formula id="inf50">
<mml:math id="m60">
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</inline-formula> and 4, which can be directly embedded into the Chimera&#x20;graph.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Connected spin networks compatible with the Chimera architecture: <bold>(A)</bold> <inline-formula id="inf51">
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</inline-formula>.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g005.tif"/>
</fig>
<p>A single coupling between the qubits in the quantum processor architecture can be associated with one or more links in the corresponding spin network. The difference between connections can be further encoded in the strength of the couplers. In particular, in the case a) in <xref ref-type="fig" rid="F5">Figure&#x20;5</xref> there are two possible 4-valent spin networks can be associated with two coupled qubits. Relating a single coupler with a single link in the spin network is generically not possible. In the case of 4-valent nodes and a single block of D-Wave processor, the only possibility is given by the configuration represented in blocks b) and c) in <xref ref-type="fig" rid="F2">Figure&#x20;2</xref>. The situation corresponds to a spin network with <inline-formula id="inf55">
<mml:math id="m65">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>8</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> qubits and <inline-formula id="inf56">
<mml:math id="m66">
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>16</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> edges forming the Chimera&#x20;graph.</p>
<p>As one can notice, the structure of Chimera architecture imposes significant restrictions on the possible associated spin network topologies. In particular, it is not possible to implement a &#x201c;triangular&#x201d; <inline-formula id="inf57">
<mml:math id="m67">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>3</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> spin network directly with the use of elementary qubits. In order to go beyond the limitations of the Chimera architecture, one can consider effective qubits (chain qubits) composed of two or more spins. If the coupling between the qubits is sufficiently negative, then the qubits will tend to align in the same direction, which is preferred energetically. In such a case, measurements can be performed on one of the elementary qubits contributing to the chain, while the remaining qubits can be considered ancilla qubits.</p>
<p>With the use of chain qubits (see <xref ref-type="fig" rid="F6">Figure 6</xref>), the dictionary of spin networks can be extended further. In particular, previously inaccessible spin networks for <inline-formula id="inf58">
<mml:math id="m68">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>3</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf59">
<mml:math id="m69">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> can now be constructed (see <xref ref-type="fig" rid="F7">Figure&#x20;7</xref>).</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>A chain qubit. If the <inline-formula id="inf95">
<mml:math id="m116">
<mml:mrow>
<mml:msub>
<mml:mi>b</mml:mi>
<mml:mrow>
<mml:mn>15</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> coupling is sufficiently negative then the spins <inline-formula id="inf96">
<mml:math id="m117">
<mml:mrow>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mn>1</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf97">
<mml:math id="m118">
<mml:mrow>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mn>5</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> will have tendency to align in the same direction.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g006.tif"/>
</fig>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Connected spin networks compatible with Chimera architecture: <bold>(A)</bold> <inline-formula id="inf60">
<mml:math id="m70">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>3</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, <bold>(B)</bold> <inline-formula id="inf61">
<mml:math id="m71">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g007.tif"/>
</fig>
<p>Worth stressing is that different types of effective qubits can be considered and <xref ref-type="fig" rid="F7">Figure&#x20;7</xref> represents only a one of many possible implementations of the spin networks under consideration.</p>
<p>A more extended example is a regular square lattice with the nearest neighbor connections. Implementation of the regular lattice spin network on the Chimera architecture of the quantum processor is shown in <xref ref-type="fig" rid="F8">Figure&#x20;8</xref>.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Regular lattice spin network embedded with the use of chain qubits. Here, four 8 qubit blocks of the D-Wave processor are&#x20;used.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g008.tif"/>
</fig>
<p>The regular lattice configuration enables simulation of a 2D <italic>Ising spin networks</italic> discussed in Ref (<xref ref-type="bibr" rid="B8">Feller and Livine, 2016</xref>). which provide a toy model of extended quantum spacetime. The analysis of such configurations is especially interesting in the context of phase transitions and domain formation, which may reflect the emergence of semi-classical spacetime. We will come back to this issue in the next section. Furthermore, in further studies, it would be interesting to investigate if the 3D hexagonal type <italic>Ising spin network</italic> can also be embedded into the architecture of the D-Wave processor.</p>
</sec>
<sec id="s4">
<title>4 Simulation of Loop Quantum Gravity</title>
<p>The spin network states discussed in the previous sections satisfy the Gauss constraint. Moreover, the diffeomorphism constraint can be imposed by considering equivalence classes under the action of spatial diffeomorphisms, which means that we equate all graphs with the same topology.</p>
<p>It remains the scalar (Hamiltonian) constraint, which is the most difficult one to satisfy. Finding a solution to the Hamiltonian constraint in the 3&#x20;&#x2b; 1&#x20;D can be perceived as the most difficult open problem in LQG (<xref ref-type="bibr" rid="B23">Thiemann, 2006</xref>).</p>
<p>The scalar constraint reflects the fact that the total energy of the gravitational field is equal to zero. The scalar constraint is, in general, a graph-changing operator, which makes implementation of such a constraint a problematic task. However, the situation in which the action of the constraint preserves the graph structure may provide an intermediate step toward the solution of the full problem. The question is whether adiabatic quantum computation may be helpful&#x20;here.</p>
<p>To address this question, let us observe that finding solutions to the classical constraint:<disp-formula id="e10">
<mml:math id="m72">
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(10)</label>
</disp-formula>can be mapped into a problem of minimizing some Hamiltonian. Because the quantum annealing algorithm is just searching for the minimum of the spin Hamiltonian <xref ref-type="disp-formula" rid="e2">(2)</xref>, making use of adiabatic computations requires association of the minimum of the Hamiltonian with a solution of the constraint <xref ref-type="disp-formula" rid="e10">(10)</xref>. The simplest way to do it is to consider the Hamiltonian H in the following form:<disp-formula id="e11">
<mml:math id="m73">
<mml:mrow>
<mml:mi>H</mml:mi>
<mml:mo>&#x221d;</mml:mo>
<mml:msup>
<mml:mi>C</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(11)</label>
</disp-formula>
</p>
<p>In this case, the Hamiltonian is bounded from below, and in the classical ground state, the constrain <xref ref-type="disp-formula" rid="e10">(10)</xref> is naturally satisfied.</p>
<p>Solution of the constraint <xref ref-type="disp-formula" rid="e10">(10)</xref> allows to extract physical states and construct a physical phase space <inline-formula id="inf62">
<mml:math id="m74">
<mml:mrow>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>phys</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> (or physical Hilbert space) being a subset of kinematical phase space <inline-formula id="inf63">
<mml:math id="m75">
<mml:mrow>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>kin</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
<xref ref-type="fn" rid="fn1">
<sup>1</sup>
</xref>. It is important to stress that the minimum energy states of the Hamiltonian <xref ref-type="disp-formula" rid="e11">(11)</xref> are just the physical states of the theory and they form <inline-formula id="inf64">
<mml:math id="m76">
<mml:mrow>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>phys</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>. If there is no additional matter content, the states represent also a vacuum gravitational field configuration, described by the prototype scalar (Hamiltonian) constraint under considerations. The auxiliary Hamiltonian <xref ref-type="disp-formula" rid="e11">(11)</xref> is a simplified version of the <italic>Master Constraint</italic> introduced in LQG, being a square function of constraints [see Ref <xref ref-type="bibr" rid="B23">Thiemann (2006)</xref>].</p>
<p>There are, however, technical limitations in the implementation of the procedure proposed above. This is because, in the D-Wave annealer, only quadratic Hamiltonian functions are allowed. This implies that the scalar constraint cannot be higher than linear order in the spin variables. On the other hand, scalar constraints being of the higher than linear order in the spin variables is expected in the full&#x20;LQG.</p>
<p>The most general type of the constraint that one consider in the context of D-Wave quantum computer is<disp-formula id="e12">
<mml:math id="m77">
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:munderover>
<mml:msub>
<mml:mi>a</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>c</mml:mi>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(12)</label>
</disp-formula>with some parameters <inline-formula id="inf65">
<mml:math id="m78">
<mml:mrow>
<mml:msub>
<mml:mi>a</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>c</mml:mi>
<mml:mo>&#x2208;</mml:mo>
<mml:mi mathvariant="normal">&#x211d;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>
<xref ref-type="fn" rid="fn2">
<sup>2</sup>
</xref> and where <inline-formula id="inf66">
<mml:math id="m79">
<mml:mrow>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x2208;</mml:mo>
<mml:mrow>
<mml:mo>{</mml:mo>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1,1</mml:mn>
</mml:mrow>
<mml:mo>}</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula> are classical spin variables.</p>
<p>Here, for the sake of simplicity we will consider the case with <inline-formula id="inf67">
<mml:math id="m80">
<mml:mrow>
<mml:msub>
<mml:mi>a</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mo>&#x2200;</mml:mo>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, such that the prototype scalar constraint <xref ref-type="disp-formula" rid="e12">(12)</xref> takes the following form:<disp-formula id="e13">
<mml:math id="m81">
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:munderover>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>c</mml:mi>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(13)</label>
</disp-formula>with some parameter <inline-formula id="inf68">
<mml:math id="m82">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>&#x2208;</mml:mo>
<mml:mrow>
<mml:mo>{</mml:mo>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>,</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>,</mml:mo>
<mml:mi>N</mml:mi>
</mml:mrow>
<mml:mo>}</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>. By squaring <xref ref-type="disp-formula" rid="e13">(13)</xref> we obtain:<disp-formula id="e14">
<mml:math id="m83">
<mml:mrow>
<mml:msup>
<mml:mi>C</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:munder>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mrow>
<mml:mo>&#x2329;</mml:mo>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>j</mml:mi>
</mml:mrow>
<mml:mo>&#x232a;</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:munder>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:mover>
</mml:mrow>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:munder>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:munder>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>c</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(14)</label>
</disp-formula>
</p>
<p>From this one can propose that the Hamiltonian to be considered is:<disp-formula id="e15">
<mml:math id="m84">
<mml:mrow>
<mml:mi>H</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>C</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mrow>
<mml:mo>&#x2329;</mml:mo>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>j</mml:mi>
</mml:mrow>
<mml:mo>&#x232a;</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:munderover>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>h</mml:mi>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:munderover>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(15)</label>
</disp-formula>where <inline-formula id="inf69">
<mml:math id="m85">
<mml:mrow>
<mml:mi>h</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>c</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. The obtained Hamiltonian corresponds to the QUBO problem with a complete graph and equal couplers between the qubits <inline-formula id="inf70">
<mml:math id="m86">
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mi>b</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>. In this model, the ground state (which corresponds to <inline-formula id="inf71">
<mml:math id="m87">
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>) energy is:<disp-formula id="e16">
<mml:math id="m88">
<mml:mrow>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:mfrac>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(16)</label>
</disp-formula>
</p>
<p>There is one more important aspect illustrated by the model - a degeneracy of the ground state. Namely, there are, in general, multiple spin configurations which are minimizing the Hamiltonian (15). In the model under consideration, the vacuum degeneracy depends on both <italic>c</italic> and <italic>N</italic>. Given the <italic>c</italic> and <italic>N</italic>, finding the order of degeneracy is a combinatorial problem which can be reduced to determining the number of <inline-formula id="inf72">
<mml:math id="m89">
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>c</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> subset of a set composed of <italic>N</italic> elements, which is given by the binomial coefficient:<disp-formula id="e17">
<mml:math id="m90">
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtable>
<mml:mtr>
<mml:mtd>
<mml:mi>N</mml:mi>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>c</mml:mi>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:mfrac>
</mml:mrow>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(17)</label>
</disp-formula>
</p>
<p>Then, for a fixed N the maximal degeneracy is obtained for the choices<disp-formula id="e18">
<mml:math id="m91">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mrow>
<mml:mo>&#x230a;</mml:mo>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo>&#x230b;</mml:mo>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>&#x2228;</mml:mo>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mi>c</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mrow>
<mml:mo>&#x2308;</mml:mo>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo>&#x2309;</mml:mo>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(18)</label>
</disp-formula>
</p>
<p>where <inline-formula id="inf73">
<mml:math id="m92">
<mml:mrow>
<mml:mo>&#x230a;</mml:mo>
<mml:mi>x</mml:mi>
<mml:mo>&#x230b;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf74">
<mml:math id="m93">
<mml:mrow>
<mml:mo>&#x2308;</mml:mo>
<mml:mi>x</mml:mi>
<mml:mo>&#x2309;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> are floor and ceiling functions respectively. Based on this, the corresponding maximal degeneracy is equal to<disp-formula id="e19">
<mml:math id="m94">
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtable>
<mml:mtr>
<mml:mtd>
<mml:mi>N</mml:mi>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mrow>
<mml:mo>&#x230a;</mml:mo>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo>&#x230b;</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtable>
<mml:mtr>
<mml:mtd>
<mml:mi>N</mml:mi>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mrow>
<mml:mo>&#x2308;</mml:mo>
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo>&#x2309;</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(19)</label>
</disp-formula>
</p>
<p>The degeneracy is an essential quantity because it corresponds to the number of physical states satisfying the constraint&#x20;<xref ref-type="disp-formula" rid="e13">(13)</xref>.</p>
<p>One can now make relation with the spin networks. For this purpose, let us recall that the spin Hamiltonian <xref ref-type="disp-formula" rid="e15">(15)</xref> corresponding to the constraint <xref ref-type="disp-formula" rid="e13">(13)</xref> describes a complete graph. Associating a spin coupler with a single link of the spin network, one can conclude that for the 4-valent nodes under considerations, the only complete spin network must have <italic>pentagram</italic> structure with <inline-formula id="inf75">
<mml:math id="m95">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>5</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> nodes (see block &#x201c;a&#x201d; in <xref ref-type="fig" rid="F9">Figure&#x20;9</xref>)<xref ref-type="fn" rid="fn3">
<sup>3</sup>
</xref>.</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>(<bold>A</bold>) Pentagram spin network with <inline-formula id="inf76">
<mml:math id="m96">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>5</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>. Each link of the graph is labeled with <inline-formula id="inf77">
<mml:math id="m97">
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>. The qubits (here modeled by the classical bits <inline-formula id="inf78">
<mml:math id="m98">
<mml:mrow>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) are defined at the nodes. <bold>(B)</bold> An exemplary embedding of the pentagram spin network on the two neighbor blocks of the D-Wave processor. The shadowed regions represent collective (chain) qubits which correspond to the nodes of the spin network.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g009.tif"/>
</fig>
<p>Such spin network corresponds to the geometry of a three-sphere. Furthermore, it turns out that introducing composite (chain) spins the pentagram spin network can be implemented using two neighbor blocks of the D-Wave processor. There are various ways to do so. One of them is presented in block &#x201c;b&#x201d; in <xref ref-type="fig" rid="F9">Figure&#x20;9</xref>, where the shadowed regions correspond to the effective qubits composed of the elementary&#x20;ones.</p>
<p>Finally, let us take a look at the energy landscape of the model. In <xref ref-type="fig" rid="F10">Figure&#x20;10</xref> we plot energies corresponding to all of the spin configurations for <inline-formula id="inf79">
<mml:math id="m99">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Energy landscape of the pentagram spin network with <inline-formula id="inf80">
<mml:math id="m100">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>5</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf81">
<mml:math id="m101">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>. The ground state configurations satisfy the prototype scalar constraint <xref ref-type="disp-formula" rid="e13">(13)</xref> and span physical phase space <inline-formula id="inf82">
<mml:math id="m102">
<mml:mrow>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>phys</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> of the&#x20;model.</p>
</caption>
<graphic xlink:href="fspas-08-571282-g010.tif"/>
</fig>
<p>The total number of spin configurations corresponds to dimensionality of the kinematical space: <inline-formula id="inf83">
<mml:math id="m103">
<mml:mrow>
<mml:mtext>dim</mml:mtext>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>kin</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mn>5</mml:mn>
</mml:msup>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>32</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>. On the other hand, the degeneracy of the vacuum of <xref ref-type="disp-formula" rid="e15">(15)</xref> gives us dimensionality of the physical space <inline-formula id="inf84">
<mml:math id="m104">
<mml:mrow>
<mml:mtext>dim</mml:mtext>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>phys</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtable>
<mml:mtr>
<mml:mtd>
<mml:mn>5</mml:mn>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mn>5</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:mfrac>
</mml:mrow>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>10</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> (here we used <xref ref-type="disp-formula" rid="e17">Eq. 17</xref>). The physical space is a subset of kinematical space <inline-formula id="inf85">
<mml:math id="m105">
<mml:mrow>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>phys</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2282;</mml:mo>
<mml:msub>
<mml:mtext>&#x393;</mml:mtext>
<mml:mrow>
<mml:mtext>kin</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> as expected.</p>
<p>In order to extract all the physical states with the use of adiabatic quantum simulations, the quantum annealing procedure has to be performed repeatedly. The outcome is a superposition of the ground states, and the procedure of measurement should select the particular ground states in the independent runs. However, as discussed in Refs (<xref ref-type="bibr" rid="B18">Matsuda et&#x20;al., 2009</xref>; <xref ref-type="bibr" rid="B16">Mandr&#xe0; et&#x20;al., 2017</xref>) the type of quantum annealing procedure used in the D-Wave quantum computers may not be suited to identify all degenerate ground states. The studies suggest that an extension beyond the currently employed base Hamiltonians is needed to ensure that the ground state manifold is adequately sampled. Otherwise, the probability of finding some of the possible ground states may be suppressed.</p>
<p>Assuming that the physical states are selected, analysis of fluctuations of various observables is possible to perform. In the case under consideration, one of the interesting possibilities would be to investigate volume fluctuations. As we already mentioned, the base states corresponding to the 4-valent note qubits are eigenstates of the volume operator describing the same absolute volume but with different signs. It is, however, expected that in the classical limit, only one type of contribution would dominate such that averaged nonvanishing space volume will emerge. On the other hand, in a strongly quantum state, the positive and negative contributions can subtract one another, leading to the lack of the notion of classical geometry. Analysis of correlations of the spins in the physical states could, therefore, tell us whether domains of the same sign of volume are formed. If yes, that would be a sign of the emergence of semi-classical spacetime. Furthermore, the presence of long-range correlation would unavoidably allow associating a notion of length scale to the spin network configurations. Such observation would be a significant step toward the reconstruction of classical spacetime directly from the spin network states.</p>
</sec>
<sec id="s5">
<title>5 Summary</title>
<p>The purpose of this article was to investigate the possibility of the implementation of spin networks on the architecture of commercially accessible adiabatic quantum computers (quantum annealers). In the studies, we focused our attention on spin networks with fixed spin labels (<inline-formula id="inf86">
<mml:math id="m106">
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mn>2</mml:mn>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula>) corresponding to the fundamental representation of the <inline-formula id="inf87">
<mml:math id="m107">
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>U</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula> group. In such a case, the 4-valent nodes give rise to two-dimensional intertwiner space associated with the qubit Hilbert space. In the geometric picture, the 4-valent nodes of a spin network are dual to the 3D simplices, and the qubit bases states represent different orientations of a 3-simplex.</p>
<p>We have shown that it is possible to define spin networks on the architecture of the D-Wave quantum processor in the considered case. However, due to topological restrictions of the Chimera graph, not all spin networks are possible to implement with the use of elementary qubits. However, some obstacles can be overcome by introducing effective (chain) qubits composed of two or more elementary qubits. Such effective qubits allow implementing, e.g., regular 2D square lattice topology of the nearest neighbor type of interaction Ising&#x20;model.</p>
<p>Furthermore, we proposed a method of solving scalar (Hamiltonian) constraints using quantum annealing. In the case of D-Wave quantum annealers, we have shown that a prototype constraint being a linear function of qubit variables, is possible to solve. The solutions of the constraint (i.e.,&#x20;physical states) are obtained as ground states of an appropriate Ising-type Hamiltonian. The procedure has been theoretically demonstrated for the pentagram spin network, which (as we have shown) can be embedded onto the architecture of the D-Wave processor. This opens a path to simulate simplified LQG models on available quantum annealers. However, one has to keep in mind that computational complexity of the approach not been addressed yet. Consequently, it is not known whether quantum annealers may provide the <italic>quantum speed-up</italic> for solving the LQG-related scalar constraints.</p>
<p>Various generalizations of the investigated class of spin networks are to be considered. In particular, the situation which is motivated by the semi-classical limit is when all spin labels are equal to some <inline-formula id="inf88">
<mml:math id="m108">
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x226b;</mml:mo>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mn>2</mml:mn>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula>, instead of <inline-formula id="inf89">
<mml:math id="m109">
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mn>2</mml:mn>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula>. In the case of arbitrary <italic>j</italic>, the dimension of the intertwiner space of a single 4-vertex is<disp-formula id="e20">
<mml:math id="m110">
<mml:mrow>
<mml:mtext>dim</mml:mtext>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mtext>Inv</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
<mml:mo>&#x2297;</mml:mo>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
<mml:mo>&#x2297;</mml:mo>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
<mml:mo>&#x2297;</mml:mo>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>j</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1.</mml:mn>
</mml:mrow>
</mml:math>
<label>(20)</label>
</disp-formula>
</p>
<p>Generalization to the case of higher than 4-valence of nodes can also be considered. In both cases, ancillary qubits have to be introduced appropriately, which is a more difficult task or, in some cases, perhaps even not possible to do. These and other issues related to quantum simulations of spin networks, especially in the context of LQG will be the subject of our further studies.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>The author confirms being the sole contributor of this work and has approved it for publication.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>Author was supported from the Sonata Grant DEC-2014/13/D/ST2/01895 and from the Sonata Bis Grant DEC-2017/26/E/ST2/00763 of the National Science Centre Poland, and the Mobilno&#x15b;&#x107; Plus Grant 1641/MON/V/2017/0 of the Polish Ministry of Science and Higher Education. Furthermore, this publication was made possible through the support of the ID&#x23; 61466 grant from the John Templeton Foundation, as part of the &#x201c;The Quantum Information Structure of Spacetime (QISS)&#x201d; Project (qiss.fr).</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of Interest</title>
<p>The author declares 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>
<ack>
<p>The opinions expressed in this publication are those of the authors and do not necessarily reflect the views of the John Templeton Foundation. Author would like to thank to Mario Flory for his careful reading of the manuscript and helpful comments.</p>
</ack>
<fn-group>
<fn id="fn1">
<label>1</label>
<p>Here, for simplicity, we define the kinematical phase space such that is obtained by solving Gauss and diffeomorphism constraints. This corresponds to all possible spin configurations at the nodes of a given 4-valent spin network. In the quantum theory, the kinematical Hilbert space <inline-formula id="inf90">
<mml:math id="m111">
<mml:mrow>
<mml:msub>
<mml:mi>H</mml:mi>
<mml:mrow>
<mml:mtext>kin</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> with respect to the scalar constraint <inline-formula id="inf91">
<mml:math id="m112">
<mml:mrow>
<mml:mrow>
<mml:mover accent="true">
<mml:mi>C</mml:mi>
<mml:mo>&#x5e;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mo>&#x7c;</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
<mml:mo>&#x232a;</mml:mo>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> is a tensor product of qubit Hilbert spaces defined at <italic>N</italic> nodes of the spin network.</p>
</fn>
<fn id="fn2">
<label>2</label>
<p>Alternatively, one can consider a complex constraint <inline-formula id="inf92">
<mml:math id="m113">
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>N</mml:mi>
</mml:munderover>
<mml:mrow>
<mml:msub>
<mml:mi>z</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:msub>
<mml:mi>s</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>c</mml:mi>
</mml:mrow>
</mml:mstyle>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> with <inline-formula id="inf93">
<mml:math id="m114">
<mml:mrow>
<mml:msub>
<mml:mi>z</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>c</mml:mi>
<mml:mo>&#x2208;</mml:mo>
<mml:mi mathvariant="normal">&#x2102;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. Then, in order to obtain a real Hamiltonian on has to consider <inline-formula id="inf94">
<mml:math id="m115">
<mml:mrow>
<mml:mi>H</mml:mi>
<mml:mo>&#x221d;</mml:mo>
<mml:mo>&#x7c;</mml:mo>
<mml:mi>C</mml:mi>
<mml:msup>
<mml:mo>&#x7c;</mml:mo>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>. This can be extended further to the case of multi-constraint model, which is not discuss&#x20;here.</p>
</fn>
<fn id="fn3">
<label>3</label>
<p>The restriction is because, in the considered case, all couplers have equal value. Therefore, the couplers have to be associated with the same number of links in the spin network. The simplest example is when a single coupler is associated with a single link. However, extensions to the other cases are possible if the general form of the constraint <xref ref-type="disp-formula" rid="e12">(12)</xref> is considered.</p>
</fn>
</fn-group>
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