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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>Doubly charm tetraquark channel with isospin 1 from lattice QCD</dc:title><dc:creator>Meng,	Lu	(Avtor)
	</dc:creator><dc:creator>Ortiz Pacheco,	Emmanuel	(Avtor)
	</dc:creator><dc:creator>Baru,	Vadim	(Avtor)
	</dc:creator><dc:creator>Epelbaum,	Evgeny	(Avtor)
	</dc:creator><dc:creator>Padmanath,	M.	(Avtor)
	</dc:creator><dc:creator>Prelovšek,	Saša	(Avtor)
	</dc:creator><dc:subject>physics of elementary particles</dc:subject><dc:subject>lattice QCD</dc:subject><dc:description>Experimentally, the doubly charm tetraquark channel $cc\bar{q}\bar{q}$ with $q=u$, $d$ features an exotic hadron, $T_{cc}$, with isospin $I=0$ near the $DD^*$ threshold, while no peak was observed for $I=1$. We present a lattice QCD study of this channel with $I=1$, $J^P=1^+$,and $m_{\pi} \simeq 280$ MeV. Finite-volume energies calculated across five charm quark masses consistently feature a positive energy shift with respect to noninteracting energies, indicating repulsive interaction at energies near the threshold. These energies are used to compute the $DD^*$ scattering amplitude using both the standard Lüscher method and the recently proposed effective field theory-based approach in the plane wave basis, which incorporates the long-range interactions and the left-hand cut. Both analyses render a small negative scattering length and a scattering amplitude that does not feature any poles in the energy region near the $DD^*$ threshold, in line with the LHCb results. We identify that the Wick contraction, resembling $t$-channel isovector-vector meson exchanges between $D$ and $D^*$, plays a key role in distinguishing between the $I=0$ and $I=1$ channels, leading to repulsion in the $I=1$ and attraction in the $I=0$ channel.</dc:description><dc:date>2025</dc:date><dc:date>2025-03-05 16:30:18</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>167666</dc:identifier><dc:identifier>UDK: 539.120.811</dc:identifier><dc:identifier>ISSN pri članku: 2470-0010</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevD.111.034509</dc:identifier><dc:identifier>COBISS_ID: 228099075</dc:identifier><dc:language>sl</dc:language></metadata>
