<?xml version="1.0"?>
<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Spectral function of a bipolaron coupled to dispersive optical phonons</dc:title><dc:creator>Kovač,	Klemen	(Avtor)
	</dc:creator><dc:creator>Bonča,	Janez	(Avtor)
	</dc:creator><dc:subject>condensed matter physics</dc:subject><dc:subject>quantum physics</dc:subject><dc:subject>optical phonons</dc:subject><dc:subject>polarons</dc:subject><dc:subject>Holstein model</dc:subject><dc:subject>Hubbard model</dc:subject><dc:subject>electron-phonon coupling</dc:subject><dc:description>Using an efficient variational exact diagonalization method, we computed the electron removal spectral function within the framework of the Holstein-Hubbard model containing two electrons with opposite spins coupled to dispersive quantum optical phonons. We focus on how the interplay between the electron-phonon coupling and on-site Coulomb repulsion shapes the spectral function, a quantity directly relevant to angle-resolved photoemission spectroscopy (ARPES). Tuning the strengths of the electron-phonon coupling and the Hubbard interaction allows us to examine the evolution of the spectral properties of the system as it crosses over from a bound bipolaron to separate polarons. We find that phonon dispersion plays an important role: It substantially redistributes the spectral weight across the low- and the high-energy features and controls the emergence and the structure of distinct multiphonon continua. In regimes of strong electron-phonon coupling and low Coulomb repulsion, the spectral function exhibits a broad distribution reflecting bound bipolaronic states. Increasing the Coulomb repulsion weakens bipolaron binding, shifts the primary quasiparticle peak closer to polaronic behavior and confines the spectral weight near the Brillouin-zone center. Our results provide a framework for interpreting ARPES measurements in systems where phonon–mediated attraction competes with direct Coulomb repulsion.</dc:description><dc:date>2025</dc:date><dc:date>2025-03-14 13:03:10</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>167837</dc:identifier><dc:identifier>UDK: 538.9</dc:identifier><dc:identifier>ISSN pri članku: 2469-9950</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevB.111.115133</dc:identifier><dc:identifier>COBISS_ID: 229057027</dc:identifier><dc:language>sl</dc:language></metadata>
