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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Blockchain</journal-id>
<journal-title>Frontiers in Blockchain</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Blockchain</abbrev-journal-title>
<issn pub-type="epub">2624-7852</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1410191</article-id>
<article-id pub-id-type="doi">10.3389/fbloc.2024.1410191</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Blockchain</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Exploring bitcoin cross-blockchain interoperability: estimation through Hurst exponent</article-title>
<alt-title alt-title-type="left-running-head">Nan</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fbloc.2024.1410191">10.3389/fbloc.2024.1410191</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Nan</surname>
<given-names>Zheng</given-names>
</name>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2703808/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/conceptualization/"/>
<role content-type="https://credit.niso.org/contributor-roles/data-curation/"/>
<role content-type="https://credit.niso.org/contributor-roles/formal-analysis/"/>
<role content-type="https://credit.niso.org/contributor-roles/funding-acquisition/"/>
<role content-type="https://credit.niso.org/contributor-roles/investigation/"/>
<role content-type="https://credit.niso.org/contributor-roles/methodology/"/>
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<role content-type="https://credit.niso.org/contributor-roles/supervision/"/>
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<role content-type="https://credit.niso.org/contributor-roles/writing-original-draft/"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
</contrib-group>
<aff>
<institution>International College of Liberal Arts</institution>, <institution>Yamanashi Gakuin University</institution>, <addr-line>Kofu</addr-line>, <country>Japan</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/1710300/overview">Akihiro Fujihara</ext-link>, Chiba Institute of Technology, Japan</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/721608/overview">Sinclair Davidson</ext-link>, RMIT University, Australia</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2209470/overview">Sergio Adriani David</ext-link>, University of S&#xe3;o Paulo, Brazil</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Zheng Nan, <email>nijelnan@gmail.com</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>30</day>
<month>08</month>
<year>2024</year>
</pub-date>
<pub-date pub-type="collection">
<year>2024</year>
</pub-date>
<volume>7</volume>
<elocation-id>1410191</elocation-id>
<history>
<date date-type="received">
<day>31</day>
<month>03</month>
<year>2024</year>
</date>
<date date-type="accepted">
<day>20</day>
<month>08</month>
<year>2024</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2024 Nan.</copyright-statement>
<copyright-year>2024</copyright-year>
<copyright-holder>Nan</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>This study aims to investigate the interoperability of the Bitcoin blockchain by comparing the US dollar prices of five cryptocurrencies derived from the Bitcoin price with their corresponding market prices. The deviation rate between the derived price and the market price, referred to as the arbitrage return rate, is examined with respect to its adherence to the efficient market hypothesis and martingale theory principles, specifically regarding mean-reversion and serial independence. Hurst exponents are estimated using R/S and DFA methods, and their dynamics are analyzed using a sliding window technique. Our findings demonstrate that the Bitcoin blockchain effectively facilitates transactions among the five cryptocurrencies, though evidence suggests a potential structural change in Bitcoin blockchain interoperability following April 2023.</p>
</abstract>
<kwd-group>
<kwd>cryptocurrency</kwd>
<kwd>bitcoin</kwd>
<kwd>blockchain</kwd>
<kwd>cross-chain interoperability</kwd>
<kwd>Hurst exponent</kwd>
<kwd>DFA</kwd>
</kwd-group>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Blockchain Technologies</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>The notion of blockchain interoperability is gaining significant traction both in academic research and industrial applications. <xref ref-type="bibr" rid="B9">Belchior et al. (2022a)</xref> illustrate this trend by noting a substantial increase in Google Scholar search results, from two in 2015 to 207 in 2020. This surge in research interest underscores the growing industry demand for interoperability among many existing blockchains. Historically, individual blockchains were developed to address specific use cases and challenges in isolation, neglecting cross-chain interoperability (<xref ref-type="bibr" rid="B1">Abebe et al., 2019</xref>; <xref ref-type="bibr" rid="B25">Jin et al., 2018</xref>). The adaptability of a blockchain to the requirements of its stakeholders has emerged as a critical driver behind the proliferation of new and diverse blockchains, resulting in a heterogeneous blockchain ecosystem and consequent fragmentation of the blockchain landscape (<xref ref-type="bibr" rid="B10">Belchior et al., 2022b</xref>; <xref ref-type="bibr" rid="B40">Pillai et al., 2020</xref>; <xref ref-type="bibr" rid="B45">Xu et al., 2017</xref>). Presently, practitioners and researchers are confronted with the challenge of balancing novelty and stability as they consider blockchain interoperability to enhance the scalability of existing systems and unlock new use cases (<xref ref-type="bibr" rid="B9">Belchior et al., 2022a</xref>).</p>
<p>In financial markets, blockchain technology finds significant application in cryptocurrencies, where digital tokens are viewed as financial assets with potential monetary use. Among the vast array of cryptocurrencies tracked across numerous exchanges, including Bitcoin (BTC), Ethereum (ETH), Tether (USDT), Binance (BNB), Solana (SOL), and Ripple (XRP), the top six cryptocurrencies dominate the market shares. As of 18 March 2024, these cryptocurrencies collectively hold 77.1% of the market capitalization, with Bitcoin alone accounting for 49.4%. Given its substantial market share, the Bitcoin blockchain is a prime candidate for hosting other blockchains. In this context, bitcoin cross-chain interoperability refers to the capability of cryptocurrencies to be exchanged with one another over the Bitcoin blockchain.</p>
<p>
<xref ref-type="bibr" rid="B47">Wegner (1996)</xref> defines interoperability as the ability of multiple software components to collaborate effectively despite differences in language, interface, and execution platform. The National Interoperability Framework Observatory (NIFO) (<xref ref-type="bibr" rid="B36">European Commission, 2020</xref>) identifies seven layers of interoperability: technical, semantic, organizational, legal, integrated public service governance, and interoperability governance. Various factors influencing interoperability are categorized within each layer (<xref ref-type="bibr" rid="B48">Campmas et al., 2022</xref>). While current efforts primarily focus on the technical layer, we concentrate on semantic-level interoperability. For example, facilitating a transaction from Ethereum to a Ripple user involves at least two blockchains: the source blockchain, Ethereum, and the target blockchain, Ripple.</p>
<p>The process of transferring assets across different blockchains involves three fundamental steps: (i) locking an asset on the source blockchain, (ii) committing to the blockchain transfer, and (iii) creating a representation of the asset (known as a token) on the target blockchain (<xref ref-type="bibr" rid="B10">Belchior et al., 2022b</xref>; <xref ref-type="bibr" rid="B21">Hargreaves et al., 2021</xref>). Belchior et al. (2022a) distinguish transfers between heterogeneous blockchains as cross-blockchain communication (CBC), contrasting with cross-chain communication (CCC) between homogeneous blockchains. <xref ref-type="bibr" rid="B46">Zamyatin et al. (2021)</xref> demonstrate that no CCC protocol can tolerate misbehaving nodes without a trusted third party. The choice of a trusted third party presents two options: centralized or decentralized (<xref ref-type="bibr" rid="B32">Montgomery et al., 2020</xref>). A centralized trusted party could be an exchange or institution. <xref ref-type="bibr" rid="B46">Zamyatin et al. (2021)</xref> suggest that consensus among all distributed ledgers could be an abstraction for a trusted third party. Conversely, a decentralized trusted party could be another blockchain. <xref ref-type="bibr" rid="B12">Borkowski et al. (2018)</xref> propose that the source blockchain should replicate the consensus mechanism of the target blockchain. <xref ref-type="bibr" rid="B26">Lafourcade and Lombard-Platet (2020)</xref> argue that achieving fully decentralized blockchain interoperability is impractical. These findings underscore a crucial realization: Cross-blockchain transactions necessitate a trusted third party, which may involve institutions or consensus mechanisms from the blockchains involved.</p>
<p>We discuss two scenarios for establishing third-party consensus: Cryptocurrency exchanges could use either dollars or bitcoins to facilitate cross-blockchain transactions. For example, Ethereum and Ripple transactions can follow two distinct paths (see <xref ref-type="fig" rid="F1">Figure 1</xref>). The first path involves utilizing a fiat currency, such as the U.S. dollar, as an intermediary to facilitate the consensus processes in both the Ethereum and Ripple blockchains. For instance, one Ether may be valued at $3,480, and with the assistance of an exchange, $3,480 could be exchanged for 5,800 Ripples. This process establishes an exchange rate between Ethers and Ripples, referred to as the cross-blockchain (CBC) exchange rate for Ripple in terms of Ether, denoted ETHXRP. The second path involves employing another blockchain, such as the Bitcoin blockchain, as the intermediary to complete the consensus between Ethereum and Ripple. This approach results in two distinct CBC exchange rates, ETHBTC and XRPBTC, along with the Bitcoin-derived CBC exchange rate, BETHXRP. Therefore, for cross-blockchain transactions between Ethereum and Ripple, there are at least two types of CBC exchange rates, contingent upon the choice of fiat currency or blockchain used. The fiat-currency-derived CBC exchange rate, specifically ETHXRP, serves as a reference point for investigating Bitcoin cross-blockchain interoperability, as BETHXRP represents.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>The cross-blockchain transactions between Ethereum and Ripple, showcasing two distinct paths.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g001.tif"/>
</fig>
<p>It is observed that the proposed CBC transaction model can be simplified into a halfway model. This means that using ETHUSD represents the direct path of a CBC transaction while utilizing the bitcoin-derived ETHUSD, denoted as BETHUSD &#x3d; ETHBTC &#xd7; BTCUSD, signifies the indirect path of a CBC transaction. The advantage of this approach is that it allows focusing on one cryptocurrency against bitcoin at a time.</p>
<p>This study aims to explore the interoperability of the Bitcoin blockchain with the top five cryptocurrencies in terms of market capitalization: ETH, USDT, BNB, SOL, and XRP. The methodology involves comparing the prices of these five cryptocurrencies, namely, ETHUSD, USDTUSD, BNBUSD, SOLUSD, and XRPUSD, with their bitcoin-derived counterparts: BETHUSD, BUSDTUSD, BBNBUSD, BSOLUSD, and BXRPUSD. Tether is the most widely used dollar-pegged stablecoin. Incorporating Tether in the analysis is worthwhile because of its profitable correlation with Bitcoin (<xref ref-type="bibr" rid="B11">Bianchi et al., 2020</xref>) and its noted instability in terms of price, returns, volatility, and trading volume (<xref ref-type="bibr" rid="B20">Grobys and Huynh, 2022</xref>; <xref ref-type="bibr" rid="B22">Hoang and Baur, 2021</xref>).</p>
<p>In the context of cross-blockchain interoperability, Ether&#x2019;s price in dollars, facilitated by the Bitcoin blockchain, should not consistently deviate from Ether&#x2019;s dollar price. Alternatively, the arbitrage return rate, defined as the difference between these two prices, should not consistently present predictable patterns. The absence of long-term memory in the arbitrage returns not only aligns with efficient market theories but also suggests that the Bitcoin blockchain can effectively facilitate transactions across other blockchains.</p>
<p>
<xref ref-type="bibr" rid="B15">Fama&#x2019;s (1970)</xref> efficient market hypothesis (EMH) states that abnormal returns only exist by chance and that no individual can consistently predict future prices using current information. <xref ref-type="bibr" rid="B42">Samuelson&#x2019;s (1973)</xref> martingale model suggests that successive returns should not exhibit serial dependence. However, anomalies cannot simply be dismissed as random errors (<xref ref-type="bibr" rid="B44">Tversky and Kahneman, 1988</xref>). <xref ref-type="bibr" rid="B19">Frankfurter and McGoun (2001)</xref> argue that anomalies are generic in nature and suggest a certain type of market efficiency. <xref ref-type="bibr" rid="B27">Latif et al. (2011)</xref> find that calendar, fundamental, and technical anomalies can lead to abnormal profit. <xref ref-type="bibr" rid="B16">Fama (1990)</xref> contends that &#x201c;such anomalies can be explained only in the context of some particular situations.&#x201d;</p>
<p>One example of an anomaly is the slow response of investors to new information. <xref ref-type="bibr" rid="B24">Jegadeesh and Titman (1993)</xref> observe that adjustments to announcements usually take 12 months, with variations ranging from 6 months to 2 years <xref ref-type="bibr" rid="B5">Barberis and Shleifer (2012)</xref> attribute this slow adjustment to under-reaction and overreaction. As <xref ref-type="bibr" rid="B17">Fama (1998)</xref> concludes in his work, &#x201c;Market efficiency survives the challenge from the literature on long-term return anomalies.&#x201d;</p>
<p>
<xref ref-type="bibr" rid="B7">Bariviera et al. (2017)</xref> use the detrended fluctuation analysis (DFA) method to analyze Bitcoin&#x2019;s intraday returns over 5&#x2013;12&#xa0;h with 500 data points. They argue that DFA is better suited for nonstationary data than the R/S method, which tends to confuse short-term and long-term memory. Their study finds that long-term memory is not linked to market liquidity and decreases over time. <xref ref-type="bibr" rid="B18">Fousekis and Tzaferi (2021)</xref> utilize frequency connectedness analysis, a method introduced by <xref ref-type="bibr" rid="B8">Barun&#xed;k and K&#x159;ehl&#xed;k (2018)</xref>, to examine how shocks in one stochastic process affect another at various frequencies, exploring the relationship between returns and trading activities. They suggest that asymmetry, characterized as a temporal link between returns and trading volume, can be influenced by the strength of spillovers. <xref ref-type="bibr" rid="B3">Assaf et al. (2022)</xref> explore long-term memory by employing a matrix derived from the wavelet-based multivariate long-memory estimator developed by (<xref ref-type="bibr" rid="B2">Achard and Gannaz, 2016</xref>). They discover significant long-term correlations between Bitcoin and five other cryptocurrencies. <xref ref-type="bibr" rid="B14">El Alaoui et al. (2019)</xref> observe a nonlinear interaction between Bitcoin returns and the growth rate of trading volume using multifractal detrended cross-correlation analysis (MF-DCCA). <xref ref-type="bibr" rid="B43">Stosic et al. (2019)</xref> apply the multifractal detrended fluctuation analysis (MF-DFA) to Bitcoin, concluding that Bitcoin returns do not exhibit long-term memory but show anti-persistent long-term correlations in volume changes.</p>
<p>This study proposes employing the rescaled range analysis (R/S) method and detrended fluctuation analysis (DFA) to estimate Hurst exponents using sliding windows. The Hurst exponent is a statistical metric for predictability and is commonly utilized to assess whether a time series exhibits long-term memory, which manifests as volatility clustering in return time series (<xref ref-type="bibr" rid="B7">Bariviera, 2017</xref>). A higher Hurst exponent also enhances the accuracy of backpropagation Neural Networks (<xref ref-type="bibr" rid="B41">Qian and Rasheed, 2004</xref>). Additionally, Bai-Perron tests for breakpoints complement the Hurst exponent methodology. This study contributes to the literature by investigating long-term memory in Bitcoin-related arbitrage returns. The analysis is conducted using the R programming language.</p>
<p>The remainder of the paper is structured as follows: <xref ref-type="sec" rid="s2">Section 2</xref> outlines the dataset and methodology, <xref ref-type="sec" rid="s3">Section 3</xref> presents the results and discussion, and <xref ref-type="sec" rid="s4">Section 4</xref> concludes the paper.</p>
</sec>
<sec id="s2">
<title>2 Data and methodology</title>
<p>The data is collected daily from Yahoo Finance. This dataset includes six cryptocurrencies: Bitcoin (BTC), Ethereum (ETH), Tether (USDT), Binance (BNB), Solana (SOL), and Ripple (XRP). Each cryptocurrency has its price time series: BTCUSD, ETHUSD, USDTUSD, BNBUSD, SOLUSD, and XRPUSD. Since we use the Bitcoin blockchain as the trusted third-party abstraction, there are five cross-blockchain (CBC) exchange rates: ETHBTC, USDTBTC, BNBBTC, SOLBTC, and XRPBTC. For simplicity, we exclude &#x201c;CBC&#x201d; from the notation. The investigation period spans from 11 November 2017, to 18 March 2024, totaling 2319 observations after discarding two missing values. However, Solana, launched in 2020, extends from 10 April 2020, to 18 March 2024, comprising 1438 observations. Using Yahoo Finance as the primary data source for cryptocurrency prices carries the risk of data inaccuracies. However, it provides consistency and minimizes timestamp issues.</p>
<p>In order to assess the interoperability of the Bitcoin blockchain, it is necessary to generate a Bitcoin-derived dollar price for each cryptocurrency, denoted as BCRYPTOUSD. This process involves evaluating how closely the consensus mechanism of the bitcoin blockchain mirrors that of other cryptocurrency blockchains and, subsequently, how it translates this consensus into a dollar value within its own mechanism. The computation for the bitcoin-derived cryptocurrency price is outlined by <xref ref-type="bibr" rid="B33">Nan and Kaizoji (2017</xref>, <xref ref-type="bibr" rid="B34">2019)</xref>.<disp-formula id="e1">
<mml:math id="m1">
<mml:mrow>
<mml:mi>B</mml:mi>
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<mml:mo>&#xd7;</mml:mo>
<mml:mrow>
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</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>where &#x201c;CRYPTO&#x201d; represents any given cryptocurrency.</p>
<p>For instance, the calculation of BETHUSD on 18 March 2024, can be derived from ETHUSD and ETHBTC using <xref ref-type="disp-formula" rid="e1">Equation 1</xref>: <inline-formula id="inf1">
<mml:math id="m2">
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</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#xd7;</mml:mo>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
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</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>0.0525</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>67832.22</mml:mn>
<mml:mo>&#x2248;</mml:mo>
<mml:mn>3561</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<p>This indicates that one ether is valued at $3561 when bridged by the bitcoin blockchain. Notably, ETHBTC was quoted at $3561.764 on the same day.</p>
<p>Similarly, there are 2319 observations for four bitcoin-derived cryptocurrency prices: BETHUSD, BUSDTUSD, BBNBUSD, and BXRPUSD, while BSOLUSD has 1438 observations.</p>
<p>For each cryptocurrency and US dollar pair, two prices are quoted: one direct price and one indirect price bridged by the bitcoin blockchain. The arbitrage return rate between these two prices can be constructed using the equation provided by <xref ref-type="bibr" rid="B35">Nan and Kaizoji (2020)</xref> and <xref ref-type="bibr" rid="B39">Pichl and Kaizoji (2017)</xref>.<disp-formula id="e2">
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<mml:mn>1</mml:mn>
</mml:mrow>
</mml:math>
<label>(2)</label>
</disp-formula>where <inline-formula id="inf2">
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</mml:math>
</inline-formula> represents the arbitrage return rate between BETHUSD and ETHUSD. Similarly, we can calculate the other four arbitrage return rates using <xref ref-type="disp-formula" rid="e2">Equation 2</xref>: <inline-formula id="inf3">
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</mml:math>
</inline-formula>, <inline-formula id="inf4">
<mml:math id="m6">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>B</mml:mi>
<mml:mi>N</mml:mi>
<mml:mi>B</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf5">
<mml:math id="m7">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>X</mml:mi>
<mml:mi>R</mml:mi>
<mml:mi>P</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, and <inline-formula id="inf6">
<mml:math id="m8">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>O</mml:mi>
<mml:mi>L</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<p>The Hurst exponent, denoted as H, quantifies the degree of serial dependence in a time series. Initially developed to measure long-term memory in hydrological time series by <xref ref-type="bibr" rid="B23">Hurst (1951)</xref>, it was later introduced by <xref ref-type="bibr" rid="B30">Mandelbrot and Wallis (1968)</xref> for analyzing financial time series. Theoretically, the value of the Hurst exponent categorizes a time series into three groups, as outlined by Qian and Rasheed (<xref ref-type="bibr" rid="B41">Qian and Rasheed, 2004</xref>): (i) a white noise when 0 &#x3c; H &#x3c; 0.5, (ii) a random walk when H &#x3d; 0.5, and (iii) a persistent series when H &#x3e; 0.5. As H approaches 0, the strength of serial dependence weakens, while it strengthens as H approaches 1.</p>
<p>Various estimators of the Hurst exponent based on scaling properties exist, with two commonly used ones being the R/S estimator, which relies on the rescaled range statistic, and the detrended fluctuation analysis (DFA) estimator. Additionally, we employ a sliding window method to assess the dynamics of the estimated Hurst exponents.</p>
<sec id="s2-1">
<title>2.1 R/S estimator</title>
<p>The rescaled range analysis (R/S) method scales the range of the cumulative sum of deviation of a time series from its mean (<xref ref-type="bibr" rid="B6">Bariviera, 2017</xref>). Let <inline-formula id="inf7">
<mml:math id="m9">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, be a time series, and the R/S estimator can be found through the following procedure (<xref ref-type="bibr" rid="B28">Lee, 2022</xref>):<list list-type="simple">
<list-item>
<p>(i) Split <inline-formula id="inf8">
<mml:math id="m10">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> into <inline-formula id="inf9">
<mml:math id="m11">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> subseries.</p>
</list-item>
</list>
</p>
<p>Each subperiod has an equal length of <inline-formula id="inf10">
<mml:math id="m12">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>. The number of subperiods is <inline-formula id="inf11">
<mml:math id="m13">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>. So <inline-formula id="inf12">
<mml:math id="m14">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#xd7;</mml:mo>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x2265;</mml:mo>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, and the last subseries may contain NAs.</p>
<p>Note that the subscripts have different meanings:<disp-formula id="equ1">
<mml:math id="m15">
<mml:mrow>
<mml:mi>t</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>w</mml:mi>
<mml:mi>h</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>l</mml:mi>
<mml:mi>e</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>t</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>m</mml:mi>
<mml:mi>e</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>i</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>x</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
</disp-formula>
<disp-formula id="equ2">
<mml:math id="m16">
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>s</mml:mi>
<mml:mi>u</mml:mi>
<mml:mi>b</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>s</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>r</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>s</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>i</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>x</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</disp-formula>
<disp-formula id="equ3">
<mml:math id="m17">
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>s</mml:mi>
<mml:mi>u</mml:mi>
<mml:mi>b</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>t</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>m</mml:mi>
<mml:mi>e</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>i</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>x</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</disp-formula>
<list list-type="simple">
<list-item>
<p>(ii) Calculate the mean <inline-formula id="inf13">
<mml:math id="m18">
<mml:mrow>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> and standard deviation <inline-formula id="inf14">
<mml:math id="m19">
<mml:mrow>
<mml:msub>
<mml:mi>S</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> for each subperiod:</p>
</list-item>
</list>
<disp-formula id="equ4">
<mml:math id="m20">
<mml:mrow>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<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:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:munderover>
</mml:mstyle>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>a</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>d</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msub>
<mml:mi>S</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<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:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:munderover>
</mml:mstyle>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</disp-formula>
</p>
<p>Note that the last subperiod <inline-formula id="inf15">
<mml:math id="m21">
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:math>
</inline-formula> has NAs, so <inline-formula id="inf16">
<mml:math id="m22">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> should be adjusted accordingly.<list list-type="simple">
<list-item>
<p>(iii) Calculate the demeaned <inline-formula id="inf17">
<mml:math id="m23">
<mml:mrow>
<mml:msub>
<mml:mi>d</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> from the original time series <inline-formula id="inf18">
<mml:math id="m24">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> for each subperiod:</p>
</list-item>
</list>
<disp-formula id="equ5">
<mml:math id="m25">
<mml:mrow>
<mml:msub>
<mml:mi>d</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>M</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</disp-formula>where <inline-formula id="inf19">
<mml:math id="m26">
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>.<list list-type="simple">
<list-item>
<p>(iv) Calculate the cumulative series of <inline-formula id="inf20">
<mml:math id="m27">
<mml:mrow>
<mml:msub>
<mml:mi>d</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf21">
<mml:math id="m28">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, for each subperiod:</p>
</list-item>
</list>
<disp-formula id="equ6">
<mml:math id="m29">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>i</mml:mi>
</mml:munderover>
</mml:mstyle>
<mml:msub>
<mml:mi>d</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</disp-formula>
<list list-type="simple">
<list-item>
<p>(v) Find the range <inline-formula id="inf22">
<mml:math id="m30">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> for each subperiod:</p>
</list-item>
</list>
<disp-formula id="equ7">
<mml:math id="m31">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>max</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>min</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</disp-formula>
<list list-type="simple">
<list-item>
<p>(vi) Rescale the range <inline-formula id="inf23">
<mml:math id="m32">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> by its standard deviation <inline-formula id="inf24">
<mml:math id="m33">
<mml:mrow>
<mml:msub>
<mml:mi>S</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> to get <inline-formula id="inf25">
<mml:math id="m34">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>/</mml:mo>
<mml:msub>
<mml:mi>S</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, and then calculate the mean of the rescaled range using <xref ref-type="disp-formula" rid="e3">Equation 3</xref>:</p>
</list-item>
</list>
<disp-formula id="e3">
<mml:math id="m35">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>R</mml:mi>
<mml:mo>/</mml:mo>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:msub>
<mml:mo>&#x2261;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:munderover>
</mml:mstyle>
<mml:mfrac>
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>S</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
<label>(3)</label>
</disp-formula>
<list list-type="simple">
<list-item>
<p>(vii) Repeat steps (i) through (vi) by varying <inline-formula id="inf26">
<mml:math id="m36">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
</list-item>
</list>
</p>
<p>The length of the subseries, <inline-formula id="inf27">
<mml:math id="m37">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, is a variable. Typically, we can select <inline-formula id="inf28">
<mml:math id="m38">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> using the following method:<disp-formula id="equ8">
<mml:math id="m39">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mn>0</mml:mn>
</mml:msup>
</mml:mrow>
</mml:mfrac>
<mml:mo>,</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mn>1</mml:mn>
</mml:msup>
</mml:mrow>
</mml:mfrac>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mi>k</mml:mi>
</mml:msup>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</disp-formula>where we aim for <inline-formula id="inf29">
<mml:math id="m40">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mo>/</mml:mo>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mi>k</mml:mi>
</mml:msup>
<mml:mo>&#x2248;</mml:mo>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mn>3</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>, hence <inline-formula id="inf30">
<mml:math id="m41">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>r</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>u</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>d</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>log</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mo>/</mml:mo>
<mml:msup>
<mml:mn>2</mml:mn>
<mml:mn>3</mml:mn>
</mml:msup>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mo>&#x2061;</mml:mo>
<mml:mi mathvariant="italic">log</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<p>The R/S statistic is known to asymptotically follow the relation shown in <xref ref-type="disp-formula" rid="e4">Equation 4</xref> (<xref ref-type="bibr" rid="B23">Hurst, 1951</xref>)<disp-formula id="e4">
<mml:math id="m42">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>R</mml:mi>
<mml:mo>/</mml:mo>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:msub>
<mml:mo>&#x223c;</mml:mo>
<mml:mi>C</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:msubsup>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
<mml:mi>H</mml:mi>
</mml:msubsup>
</mml:mrow>
</mml:math>
<label>(4)</label>
</disp-formula>where <inline-formula id="inf31">
<mml:math id="m43">
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the Hurst exponent. Hence, <inline-formula id="inf32">
<mml:math id="m44">
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> can be estimated using a simple linear regression using <xref ref-type="disp-formula" rid="e5">Equation 5</xref>:<disp-formula id="e5">
<mml:math id="m45">
<mml:mrow>
<mml:mi mathvariant="italic">Log</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>R</mml:mi>
<mml:mo>/</mml:mo>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>l</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>g</mml:mi>
<mml:mi>C</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>H</mml:mi>
<mml:mi>l</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>g</mml:mi>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(5)</label>
</disp-formula>
</p>
</sec>
<sec id="s2-2">
<title>2.2 DFA estimator</title>
<p>The detrended fluctuation analysis (DFA), introduced by Peng et al. (<xref ref-type="bibr" rid="B37">Peng et al., 1995</xref>) mitigates spurious detection of long-range dependence (<xref ref-type="bibr" rid="B6">Bariviera, 2017</xref>). Unlike the R/S method that measures the maximum range in both directions, DFA calculates the average of the squared vertical distance of <inline-formula id="inf33">
<mml:math id="m46">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>s</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> from the ordinary least squares (OLS) line (<xref ref-type="bibr" rid="B31">Mielniczuk and Wojdy&#x142;&#x142;o, 2007</xref>).</p>
<p>The DFA procedure involves five steps (<xref ref-type="bibr" rid="B38">Penzel et al., 2003</xref>).<list list-type="simple">
<list-item>
<p>(i) Determine the cumulative demeaned series <inline-formula id="inf34">
<mml:math id="m47">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> of <inline-formula id="inf35">
<mml:math id="m48">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, referred to as the &#x201c;profile&#x201d;:</p>
</list-item>
</list>
<disp-formula id="equ9">
<mml:math id="m49">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mi>t</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mi>t</mml:mi>
</mml:munderover>
</mml:mstyle>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mrow>
</mml:math>
</disp-formula>where <inline-formula id="inf36">
<mml:math id="m50">
<mml:mrow>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the mean of <inline-formula id="inf37">
<mml:math id="m51">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>.<list list-type="simple">
<list-item>
<p>(ii) Divide <inline-formula id="inf38">
<mml:math id="m52">
<mml:mrow>
<mml:msub>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mi>t</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> into <inline-formula id="inf39">
<mml:math id="m53">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> non-overlapping subseries of equal length <inline-formula id="inf40">
<mml:math id="m54">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>:</p>
</list-item>
</list>
<disp-formula id="equ10">
<mml:math id="m55">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>c</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>l</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>n</mml:mi>
<mml:mi>g</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mo>/</mml:mo>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</disp-formula>which may result in a short segment at the end of the profile. To mitigate its impact, the procedure is repeated from the opposite end, resulting in a total of <inline-formula id="inf41">
<mml:math id="m56">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> subperiods.<list list-type="simple">
<list-item>
<p>(iii) Compute the local trend for each subperiod using an OLS regression. Then, determine the variance for each subperiod using <xref ref-type="disp-formula" rid="e6">Equation 6</xref>:</p>
</list-item>
</list>
<disp-formula id="e6">
<mml:math id="m57">
<mml:mrow>
<mml:msubsup>
<mml:mi>F</mml:mi>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mn>2</mml:mn>
</mml:msubsup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2261;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<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:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:munderover>
</mml:mstyle>
<mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mi>p</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
<label>(6)</label>
</disp-formula>where <inline-formula id="inf42">
<mml:math id="m58">
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>,</mml:mo>
<mml:mo>&#x2026;</mml:mo>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>. And <inline-formula id="inf43">
<mml:math id="m59">
<mml:mrow>
<mml:msub>
<mml:mi>p</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula> is the fitting polynomials in segment <inline-formula id="inf44">
<mml:math id="m60">
<mml:mrow>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. In the OLS fitting procedure, the polynomial could be linear, quadratic, cubic, or higher order, conventionally called, DFA1, DFA2, DFA3, respectively. We chose DFA1 as the fitting polynomial, as DFA2 does not improve accuracy relative to the degree of freedom of the noise-like return time series.<list list-type="simple">
<list-item>
<p>(iv) Obtain the fluctuation function by taking the square root of averaged variances over <inline-formula id="inf45">
<mml:math id="m61">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> subperiods, as shown in <xref ref-type="disp-formula" rid="e7">Equation 7</xref>:</p>
</list-item>
</list>
<disp-formula id="e7">
<mml:math id="m62">
<mml:mrow>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2261;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mrow>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>N</mml:mi>
</mml:mrow>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:munderover>
</mml:mstyle>
<mml:mrow>
<mml:msubsup>
<mml:mi>F</mml:mi>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mn>2</mml:mn>
</mml:msubsup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>s</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mrow>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
<label>(7)</label>
</disp-formula>
<list list-type="simple">
<list-item>
<p>(v)Repeat steps (i)-(iv) for different time scale <inline-formula id="inf46">
<mml:math id="m63">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
</list-item>
</list>
</p>
<p>If the time series <inline-formula id="inf47">
<mml:math id="m64">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> exhibits long-range correlation following a power law, the fluctuation function should follow the relation (<xref ref-type="bibr" rid="B37">Peng et al., 1995</xref>):<disp-formula id="equ11">
<mml:math id="m65">
<mml:mrow>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mi>C</mml:mi>
<mml:mo>&#xd7;</mml:mo>
<mml:msubsup>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
<mml:mi>H</mml:mi>
</mml:msubsup>
</mml:mrow>
</mml:math>
</disp-formula>
</p>
<p>Similarly, <inline-formula id="inf48">
<mml:math id="m66">
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> can be estimated using a log-log regression:<disp-formula id="equ12">
<mml:math id="m67">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>g</mml:mi>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>l</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>g</mml:mi>
<mml:mi>C</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>H</mml:mi>
<mml:mi>l</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>g</mml:mi>
<mml:msub>
<mml:mi>L</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
</disp-formula>
</p>
</sec>
<sec id="s2-3">
<title>2.3 Sliding window</title>
<p>The sliding window technique involves employing a fixed window size, denoted as, <inline-formula id="inf49">
<mml:math id="m68">
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, which is moved through the time series <inline-formula id="inf50">
<mml:math id="m69">
<mml:mrow>
<mml:msub>
<mml:mi>x</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> to analyze the dynamics of Hurst exponents. We tested window sizes of <inline-formula id="inf51">
<mml:math id="m70">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>256</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf52">
<mml:math id="m71">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>512</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, and <inline-formula id="inf53">
<mml:math id="m72">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1024</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, respectively, but only the results for <inline-formula id="inf54">
<mml:math id="m73">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>512</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> are presented.</p>
<p>This approach impacts the estimation procedures of R/S and DFA by substituting <inline-formula id="inf55">
<mml:math id="m74">
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> for <inline-formula id="inf56">
<mml:math id="m75">
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. Consequently, the number of estimations for each time series is determined by <inline-formula id="inf57">
<mml:math id="m76">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>W</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>. For instance, considering the length of <inline-formula id="inf58">
<mml:math id="m77">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mi>T</mml:mi>
<mml:mi>H</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> as 2319, if <inline-formula id="inf59">
<mml:math id="m78">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>512</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, then <inline-formula id="inf60">
<mml:math id="m79">
<mml:mrow>
<mml:msub>
<mml:mi>N</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>W</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2319</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>512</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1808</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
</sec>
</sec>
<sec sec-type="results" id="s3">
<title>3 Results</title>
<p>
<xref ref-type="table" rid="T1">Table 1</xref> displays the summary statistics of cryptocurrency and bitcoin-derived cryptocurrency prices. Notably, the bitcoin-derived prices do not exhibit significant deviations from their direct prices regarding minimum, maximum, mean, and standard deviation. This observation suggests that the Bitcoin blockchain&#x2019;s interoperability maintains unbiasedness from an unconditional statistical perspective.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Summary statistics of the cryptocurrency prices and their bitcoin-derived prices.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Series</th>
<th align="left">Obs</th>
<th align="left">Min</th>
<th align="left">Max</th>
<th align="left">Mean</th>
<th align="left">S.D.</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">ETHUSD</td>
<td align="left">2319</td>
<td align="left">84.31</td>
<td align="left">4812.09</td>
<td align="left">1291.52</td>
<td align="left">1140.60</td>
</tr>
<tr>
<td align="left">BETHUSD</td>
<td align="left">2319</td>
<td align="left">84.31</td>
<td align="left">4812.11</td>
<td align="left">1291.80</td>
<td align="left">1140.68</td>
</tr>
<tr>
<td align="left">USDTUSD</td>
<td align="left">2319</td>
<td align="left">0.97</td>
<td align="left">1.07</td>
<td align="left">1.00</td>
<td align="left">0.01</td>
</tr>
<tr>
<td align="left">BUSDTUSD</td>
<td align="left">2319</td>
<td align="left">0.91</td>
<td align="left">1.13</td>
<td align="left">1.00</td>
<td align="left">0.01</td>
</tr>
<tr>
<td align="left">BNBUSD</td>
<td align="left">2319</td>
<td align="left">1.51</td>
<td align="left">675.68</td>
<td align="left">173.13</td>
<td align="left">175.50</td>
</tr>
<tr>
<td align="left">BBNBUSD</td>
<td align="left">2319</td>
<td align="left">1.51</td>
<td align="left">675.71</td>
<td align="left">173.14</td>
<td align="left">175.41</td>
</tr>
<tr>
<td align="left">XRPUSD</td>
<td align="left">2319</td>
<td align="left">0.14</td>
<td align="left">3.37</td>
<td align="left">0.52</td>
<td align="left">0.33</td>
</tr>
<tr>
<td align="left">BXRRUSD</td>
<td align="left">2319</td>
<td align="left">0.14</td>
<td align="left">3.38</td>
<td align="left">0.52</td>
<td align="left">0.33</td>
</tr>
<tr>
<td align="left">SOLUSD</td>
<td align="left">1438</td>
<td align="left">0.52</td>
<td align="left">258.93</td>
<td align="left">48.91</td>
<td align="left">55.08</td>
</tr>
<tr>
<td align="left">BSOLUSD</td>
<td align="left">1438</td>
<td align="left">0.52</td>
<td align="left">258.91</td>
<td align="left">48.82</td>
<td align="left">54.95</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>Note: Obs. Refers to the number of observations. S.D., refers to standard deviation.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>
<xref ref-type="table" rid="T2">Table 2</xref> provides the descriptive statistics of the return rates associated with arbitrage between the bitcoin-derived and direct prices. While the mean of the arbitrage return rates is nearly zero across all cases, the daily standard deviations range between 1% and 2%, implying that approximately 95% of the data points exhibit deviations from the mean within the range of &#x2212;6%&#x2013;6%. Some extreme values are observed, such as a 38% negative deviation for Ripple and a 12% positive deviation for USDT. Furthermore, these return series exhibit skewed leptokurtic and non-normal characteristics.</p>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>Summary statistics of the arbitrage return rates.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Series</th>
<th align="left">Obs</th>
<th align="left">Min</th>
<th align="left">Max</th>
<th align="left">Mean</th>
<th align="left">S.D.</th>
<th align="left">Skewness</th>
<th align="left">Kurtosis</th>
<th align="left">J-B</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">
<inline-formula id="inf61">
<mml:math id="m80">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mi>T</mml:mi>
<mml:mi>H</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">2319</td>
<td align="left">&#x2212;0.08</td>
<td align="left">0.04</td>
<td align="left">0.00</td>
<td align="left">0.01</td>
<td align="left">&#x2212;2.47</td>
<td align="left">47.20</td>
<td align="left">191195<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<inline-formula id="inf62">
<mml:math id="m81">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
<mml:mi>T</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">2319</td>
<td align="left">&#x2212;0.08</td>
<td align="left">0.12</td>
<td align="left">0.00</td>
<td align="left">0.01</td>
<td align="left">1.36</td>
<td align="left">17.38</td>
<td align="left">20703<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<inline-formula id="inf63">
<mml:math id="m82">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>B</mml:mi>
<mml:mi>N</mml:mi>
<mml:mi>B</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">2319</td>
<td align="left">&#x2212;0.12</td>
<td align="left">0.07</td>
<td align="left">0.00</td>
<td align="left">0.01</td>
<td align="left">&#x2212;2.10</td>
<td align="left">49.88</td>
<td align="left">214040<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<inline-formula id="inf64">
<mml:math id="m83">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>X</mml:mi>
<mml:mi>R</mml:mi>
<mml:mi>P</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">2319</td>
<td align="left">&#x2212;0.38</td>
<td align="left">0.10</td>
<td align="left">0.00</td>
<td align="left">0.02</td>
<td align="left">&#x2212;3.52</td>
<td align="left">71.64</td>
<td align="left">460160<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
<tr>
<td align="left">
<inline-formula id="inf65">
<mml:math id="m84">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>O</mml:mi>
<mml:mi>L</mml:mi>
<mml:mi>U</mml:mi>
<mml:mi>S</mml:mi>
<mml:mi>D</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">1438</td>
<td align="left">&#x2212;0.18</td>
<td align="left">0.09</td>
<td align="left">0.00</td>
<td align="left">0.02</td>
<td align="left">&#x2212;1.83</td>
<td align="left">21.16</td>
<td align="left">20561<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>Note: J-B refers to the Jarque-Bera test for normality.</p>
</fn>
<fn id="Tfn1">
<label>
<sup>a</sup>
</label>
<p>Significant at 1% level.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>
<xref ref-type="fig" rid="F2">Figure 2</xref> displays the time series of arbitrage returns, with red dashed lines indicating breakpoints. Each series exhibits a mean-reverting characteristic with occasional spikes. However, a sudden increase in fluctuation magnitudes was observed towards the end of the time series across all five cryptocurrencies. We employ the Bai-Perron test (<xref ref-type="bibr" rid="B4">Bai and Perron, 2003</xref>) to identify potential structural changes in each arbitrage return series and determine the locations of these breakpoints. Two breakpoints are highlighted in <xref ref-type="fig" rid="F2">Figure 2</xref> with red dashed lines. Notably, one common breakpoint occurred for all five return processes between 13 March 2023, and 13 April 2023. These observations raise questions about the Bitcoin blockchain&#x2019;s interoperability: Are these fluctuations persistent and predictable? What caused such a change? Partial answers to these questions lie in the values of the Hurst exponents. <xref ref-type="table" rid="T3">Table 3</xref> provides summary statistics of the Hurst exponents estimates.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>The arbitrage returns with potential breakpoints.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g002.tif"/>
</fig>
<table-wrap id="T3" position="float">
<label>TABLE 3</label>
<caption>
<p>Summary statistics of Hurst estimates.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left"/>
<th colspan="2" align="center">ETH</th>
<th colspan="2" align="center">USDT</th>
<th colspan="2" align="center">BNB</th>
<th colspan="2" align="center">XRP</th>
<th colspan="2" align="center">SOL</th>
</tr>
<tr>
<th align="left"/>
<th align="left">R/S</th>
<th align="left">DFA</th>
<th align="left">R/S</th>
<th align="left">DFA</th>
<th align="left">R/S</th>
<th align="left">DFA</th>
<th align="left">R/S</th>
<th align="left">DFA</th>
<th align="left">R/S</th>
<th align="left">DFA</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">Obs</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">1808</td>
<td align="left">927</td>
<td align="left">927</td>
</tr>
<tr>
<td align="left">Min</td>
<td align="left">0.44</td>
<td align="left">0.06</td>
<td align="left">0.47</td>
<td align="left">0.35</td>
<td align="left">0.48</td>
<td align="left">0.19</td>
<td align="left">0.42</td>
<td align="left">0.31</td>
<td align="left">0.47</td>
<td align="left">0.33</td>
</tr>
<tr>
<td align="left">Max</td>
<td align="left">0.69</td>
<td align="left">1.23</td>
<td align="left">0.70</td>
<td align="left">0.68</td>
<td align="left">0.69</td>
<td align="left">0.84</td>
<td align="left">0.66</td>
<td align="left">0.61</td>
<td align="left">0.68</td>
<td align="left">0.72</td>
</tr>
<tr>
<td align="left">Mean</td>
<td align="left">0.56</td>
<td align="left">0.48</td>
<td align="left">0.60</td>
<td align="left">0.54</td>
<td align="left">0.58</td>
<td align="left">0.52</td>
<td align="left">0.53</td>
<td align="left">0.42</td>
<td align="left">0.60</td>
<td align="left">0.52</td>
</tr>
<tr>
<td align="left">Median</td>
<td align="left">0.56</td>
<td align="left">0.44</td>
<td align="left">0.63</td>
<td align="left">0.57</td>
<td align="left">0.58</td>
<td align="left">0.50</td>
<td align="left">0.54</td>
<td align="left">0.41</td>
<td align="left">0.59</td>
<td align="left">0.50</td>
</tr>
<tr>
<td align="left">S.D.</td>
<td align="left">0.05</td>
<td align="left">0.11</td>
<td align="left">0.06</td>
<td align="left">0.08</td>
<td align="left">0.05</td>
<td align="left">0.09</td>
<td align="left">0.04</td>
<td align="left">0.06</td>
<td align="left">0.03</td>
<td align="left">0.07</td>
</tr>
<tr>
<td align="left">Skewness</td>
<td align="left">&#x2212;0.12</td>
<td align="left">1.83</td>
<td align="left">&#x2212;0.65</td>
<td align="left">&#x2212;0.46</td>
<td align="left">0.36</td>
<td align="left">0.13</td>
<td align="left">0.44</td>
<td align="left">1.00</td>
<td align="left">0.35</td>
<td align="left">0.26</td>
</tr>
<tr>
<td align="left">Kurtosis</td>
<td align="left">2.28</td>
<td align="left">10.45</td>
<td align="left">2.13</td>
<td align="left">2.20</td>
<td align="left">2.36</td>
<td align="left">2.59</td>
<td align="left">3.27</td>
<td align="left">3.92</td>
<td align="left">2.65</td>
<td align="left">2.73</td>
</tr>
<tr>
<td align="left">J-B</td>
<td align="left">42.71<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">5186.50<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">183.93<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">112.52<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">69.47<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">17.90<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">63.64<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">365.83<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">24.10<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
<td align="left">13.00<xref ref-type="table-fn" rid="Tfn2">
<sup>a</sup>
</xref>
</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>Note: J-B refers to the Jarque-Bera test for normality.</p>
</fn>
<fn id="Tfn2">
<label>
<sup>a</sup>
</label>
<p>Significant at 1% level.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>
<xref ref-type="fig" rid="F3">Figure 3</xref> illustrates Ethereum&#x2019;s Hurst exponents estimated using the R/S and DFA methods. Both series exhibit a similar trend, with the R/S estimates mostly above the DFA&#x2019;s. The DFA estimator (H_dfa_ETH) displays increased volatility in the middle section of the series. These findings suggest that while the DFA broadly aligns with the R/S regarding changes in H values, they diverge in terms of their levels: the R/S tends to overestimate H, whereas the DFA tends to underestimate H but is more sensitive to anomalies. Both methods indicate that Ethereum&#x2019;s arbitrage return series lacks strong, predictable persistence over the sample period: the R/S implies a random walk process, while the DFA suggests a mean-reverting process. However, from July 2021 to April 2023, the serial dependence strengthened, particularly in the DFA, which exhibits evident long-term memory despite its volatility. Interestingly, both estimators return to non-persistent levels after April 2023, indicating that the highly oscillating period in the latter part of Ethereum&#x2019;s arbitrage returns (see Panel (a) of <xref ref-type="fig" rid="F1">Figure 1</xref>) does not enhance predictability. Though mean-reverting processes could suggest predictability, <xref ref-type="bibr" rid="B17">Fama (1998)</xref> concludes that anomalies tend to reverse, so unpredictability still holds in the long term.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Ethereum&#x2019;s R/S Hurst exponents and DFA Hurst exponents.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g003.tif"/>
</fig>
<p>The stablecoin examined in our study, Tether, has demonstrated significant serial dependence strength since April 2021 (refer to <xref ref-type="fig" rid="F4">Figure 4</xref>). This suggests that the Bitcoin blockchain encountered challenges in facilitating transactions between USDT users and U.S. dollars. This period of malfunction could lead to predictable profits. However, after the conclusion of 2023, there appears to be a declining trend in the estimated Hurst exponents for USDT. Correspondingly, USDT&#x2019;s arbitrage return behavior exhibited volatility during this period.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>USDT&#x2019;s R/S Hurst exponents and DFA Hurst exponents.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g004.tif"/>
</fig>
<p>Regarding Binance, the Hurst exponents estimated through the R/S method indicate either a random walk pattern or a limited level of serial dependence strength, as depicted in <xref ref-type="fig" rid="F5">Figure 5</xref>. The DFA estimator tended to highlight a strong trend post-July 2021 but has reverted to indicating a random walk process since the onset of 2024.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>BNB&#x2019;s R/S Hurst exponents and DFA Hurst exponents.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g005.tif"/>
</fig>
<p>The disparity between the R/S Hurst and DFA Hurst exponents is most pronounced for Ripple&#x2019;s arbitrage returns, as illustrated in <xref ref-type="fig" rid="F6">Figure 6</xref>. This indicates that the R/S method perceives the return pattern as more identifiable and predictable, while the DFA considers it white noise. However, since the conclusion of 2022, Ripple&#x2019;s arbitrage returns have exhibited a strong trend, which has dissipated since July 2023. The observed disparity between these methods, particularly for Ripple&#x2019;s arbitrage returns, can be attributed to the distinct sensitivities of each technique to different types of data noise and trends. Specifically, the DFA method mitigates the spurious detection of long-range dependence (<xref ref-type="bibr" rid="B6">Bariviera, 2017</xref>).</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Ripple&#x2019;s R/S Hurst exponents and DFA Hurst exponents.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g006.tif"/>
</fig>
<p>Finally, Solona&#x2019;s arbitrage returns demonstrated significant persistence from January 2022 to June 2022 (see <xref ref-type="fig" rid="F7">Figure 7</xref>). Afterwards, the DFA Hurst exponents displayed high oscillations, suggesting increased and cyclic predictability from June 2022 to March 2023. Subsequently, there was a divergence between the R/S and DFA estimators. Both estimators indicated a higher level of dependence strength at the beginning of 2024.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Solana&#x2019;s R/S Hurst exponents and DFA Hurst exponents.</p>
</caption>
<graphic xlink:href="fbloc-07-1410191-g007.tif"/>
</fig>
</sec>
<sec sec-type="conclusion" id="s4">
<title>4 Conclusion</title>
<p>Cross-blockchain interoperability is a critical concern for facilitating transactions across various existing cryptocurrencies, with the interoperability heavily reliant on a trusted third party. One viable option is to utilize a blockchain as this intermediary party to bridge cross-blockchain transactions. Given its substantial market capitalization, the Bitcoin blockchain is a strong contender for fulfilling this role, encompassing approximately 50% of the market share. Consequently, our investigation focused on assessing the interoperability of the bitcoin blockchain with the other top five cryptocurrencies by market capitalization: Ethereum, Tether, BNB, Solana, and Ripple.</p>
<p>We introduced a middle-ground approach wherein each cryptocurrency is linked to US dollars via the Bitcoin blockchain instead of directly facilitating transactions between two cryptocurrencies. This approach mitigates ambiguity arising from asymmetric influences of individual cryptocurrencies. Subsequently, interoperability was examined by comparing the dollar price derived through the Bitcoin blockchain with each cryptocurrency&#x2019;s &#x201c;direct&#x201d; dollar price. The deviation rate between these two prices served as the arbitrage-return rate. Adhering to efficient market theories, we scrutinized whether long-term serial dependence existed in all arbitrage-return time series.</p>
<p>The dynamics of Hurst exponents, estimated using the R/S and DFA methods, indicate weak evidence of memory persistence, with characteristics leaning more towards a random walk or white noise pattern over our sample period from 11 November 2017, to 18 March 2024. These results are consistent with <xref ref-type="bibr" rid="B15">Fama&#x2019;s (1970</xref>, <xref ref-type="bibr" rid="B16">1990)</xref> efficient market hypothesis, suggesting that prices follow a random walk with returns reverting to a trivial mean.</p>
<p>Some sub-periods exhibited pronounced strength of dependence, accompanied by volatility and cyclical behavior. The observed autocorrelation may originate from a sluggish reaction to new information (<xref ref-type="bibr" rid="B5">Barberis and Shleifer, 2012</xref>). Cyclical behavior, likely caused by the investor overreaction (<xref ref-type="bibr" rid="B13">De Bondt and Thaler, 1985</xref>), aligns with <xref ref-type="bibr" rid="B17">Fama&#x2019;s (1998)</xref> assertion that most long-term return anomalies tend to dissipate, leading to a pattern where past winners become future losers and <italic>vice versa</italic>. Concerning the high volatility observed in all five arbitrage return series after April 2023, <xref ref-type="bibr" rid="B29">Malkiel (2003)</xref> concludes his research by saying that regardless of how high the price volatility is, capital markets may still be efficient if the price is less predictable. These findings suggest that the values of cryptocurrencies passing through the Bitcoin blockchain do not result in predictable deviations from the prices determined within their respective blockchains through their consensus mechanisms.</p>
<p>Consequently, we infer that the semantic layer of the Bitcoin blockchain&#x2019;s interoperability generally operated effectively, assuming the exclusion of the technical layer and other layers beyond the scope of this study. Nonetheless, we observed a significant increase in volatility clustering since April 2023 across all cryptocurrencies. These phenomena may stem from structural changes in the functionality of the Bitcoin blockchain. We propose further exploration into the potential decreased dependency of other cryptocurrencies on Bitcoin as a topic for future research.</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>ZN: Conceptualization, Data curation, Formal Analysis, Funding acquisition, Investigation, Methodology, Project administration, Resources, Software, Supervision, Validation, Visualization, Writing&#x2013;original draft, Writing&#x2013;review and editing.</p>
</sec>
<sec sec-type="funding-information" id="s7">
<title>Funding</title>
<p>The author(s) declare that no financial support was received for the research, authorship, and/or publication of this article.</p>
</sec>
<ack>
<p>We are deeply grateful to the referees for their valuable suggestions and insightful comments, which have greatly improved our paper&#x27;s quality and clarity.</p>
</ack>
<sec sec-type="COI-statement" id="s8">
<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>
<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/fbloc.2024.1410191/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/fbloc.2024.1410191/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet1.DOCX" id="SM1" mimetype="application/DOCX" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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