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        <identifier>oai:figshare.com:article/33885025</identifier>
        <datestamp>2026-09-17T10:44:18Z</datestamp>
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          <dc:title>Data for Real-space renormalisation approach to the Chalker-Coddington model revisited : improved statistics</dc:title>
          <dc:creator>Syl Shaw (25013863)</dc:creator>
          <dc:creator>Rudolf A. Roemer (22037333)</dc:creator>
          <dc:subject>Quantum Hall effect</dc:subject>
          <dc:subject>Phase transformations (Statistical physics)</dc:subject>
          <dc:subject>Renormalization (Physics)</dc:subject>
          <dc:subject>Renormalization group</dc:subject>
          <dc:subject>Geometric analysis</dc:subject>
          <dc:subject>Migrated from ePrints</dc:subject>
          <dc:description>The real-space renormalisation group method can be applied to the Chalker-Coddington model of the quantum Hall transition to provide a convenient numerical estimation of the localisation critical exponent, $\nu$. Previous such studies found $\nu\sim 2.39$ which falls considerably short of the current best estimates by transfer matrix ($\nu=2.593 \substack{+0.005\\-0.006}$) and exact-diagonalisation studies ($\nu=2.58(3)$). By increasing the amount of data $500$ fold we can now measure closer to the critical point and find an improved estimate $\nu=2.51\substack{+0.11\\-0.11}$. This deviates only $\sim 3\%$ from the previous two values and is already better than the $\sim 7\%$ accuracy of the classical small-cell renormalisation approach from which our method is adapted. We also study a previously proposed mixing of the Chalker-Coddington model with a classical scattering model which is meant to provide a route to understanding why experimental estimates give a lower $\nu\sim 2.3$. Upon implementing this mixing into our RG unit, we find only further increases to the value of $\nu$.</dc:description>
          <dc:date>2026-09-17T10:44:18Z</dc:date>
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