Nuclear Theory·nucl-th
9 papers—6 primary·3 cross-listed
In this talk I review the current status of lattice QCD calculations at nonzero temperature and density. I focus on the QCD phase structure and bulk QCD thermodynamics at zero and nonzero chemical potentials.
B. Pire🇫🇷 · L. Szymanowski🇵🇱 · J. Wagner🇵🇱
We calculate the leading order in QCD amplitude for exclusive neutrino and antineutrino production of a pseudoscalar charmed meson on an unpolarized nucleon. We work in the framework of the collinear QCD approach where generalized parton distributions (GPDs) factorize from perturbatively calculable coefficient functions. We include both terms in the coefficient functions and mass term contributions in the heavy meson distribution amplitudes. We emphasize the sensitivity of specific observables on the transversity quark GPDs.
V. Dexheimer🇺🇸 · B. Franzon🇩🇪 · S. Schramm🇩🇪
It is understood that strong magnetic fields affect the structure of neutron stars. Nevertheless, many calculations for magnetized neutron stars are still being performed using symmetric solutions of Einstein's equations. In this conference proceeding, we review why this is not the correct procedure and we also discuss the effects of magnetic fields on the stellar population and temperature profiles.
first authorsco-authorsvia INSPIRE