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<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>$B \to \rho \ell \bar{\nu}$ resonance form factors from $B \to \pi \pi \ell \bar{\nu}$ in lattice QCD</dc:title><dc:creator>Leskovec,	Luka	(Avtor)
	</dc:creator><dc:creator>Meinel,	Stefan	(Avtor)
	</dc:creator><dc:creator>Petschlies,	Marcus	(Avtor)
	</dc:creator><dc:creator>Negele,	John W.	(Avtor)
	</dc:creator><dc:creator>Paul,	Srijit	(Avtor)
	</dc:creator><dc:creator>Pochinsky,	Andrew	(Avtor)
	</dc:creator><dc:subject>physics of elementary particles</dc:subject><dc:subject>particle interactions</dc:subject><dc:subject>lattice QCD</dc:subject><dc:subject>form factors</dc:subject><dc:description>The decay $B \to \rho \ell \bar{\nu}$ is an attractive process for determining the magnitude of the smallest Cabibbo-Kobayashi-Maskawa matrix element, $|V_{ub}|$, and can provide new insights into the origin of the longstanding exclusive-inclusive discrepancy in determinations of this standard-model parameter. This requires a nonperturbative QCD calculation of the $B \to \rho$ form factors $V$, $A_0$, $A_1$, and $A_{12}$. The unstable nature of the $\rho$ resonance has prevented precise lattice QCD calculations of these form factors to date. Here, we present the first lattice QCD calculation of the $B \to \rho$ form factors in which the $\rho$ is treated properly as a resonance in $P$-wave $\pi \pi$ scattering. To this end, we use the Lellouch-Lüscher finite-volume formalism to compute the $B \to \pi \pi$ form factors as a function of both momentum transfer and $\pi \pi$ invariant mass, and then analytically continue to the $\rho$ resonance pole. This calculation is performed with 2 + 1 dynamical quark flavors at a pion mass of approximately 320 MeV, and demonstrates a clear path toward results at the physical point.</dc:description><dc:date>2025</dc:date><dc:date>2025-04-24 11:37:47</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>168786</dc:identifier><dc:identifier>UDK: 539.120.811</dc:identifier><dc:identifier>ISSN pri članku: 0031-9007</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevLett.134.161901</dc:identifier><dc:identifier>COBISS_ID: 234136323</dc:identifier><dc:language>sl</dc:language></metadata>
