In this talk, I will present a new decomposition of QCD splitting functions, carried out systematically up to second order in the strong coupling. The core idea is to separate the splitting functions ...

We first review the decade-old, broad collider physics research program dubbed energy-peaks. We consider the energy distribution of a massless particle in the lab frame arising from the two-body decay ...

The AmpRed package has been updated with an improved method for analytic continuation of complex integrals. Compared to the previous version, the new implementation significantly enhances ...

Strange quark stars (SQSs), namely compact stars entirely composed of deconfined quark matter, are characterized by similar masses and compactness to neutron stars (NSs) and have been theoretically ...

The U-dualities of maximally supersymmetric supergravity theories lead to celebrated non-perturbative constraints on the structure of quantum gravity. They can also lead to the presence of global ...

We apply a recently proposed chiral-Lagrangian model to discuss the anomalous (unnatural-parity) decays of the low-lying vector and axial-vector mesons. First, about twenty "SU(3) relatives" of the ...

HIAS, UCAS, Hangzhou. Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences (HIAS, UCAS). Hangzhou Institute for Advanced Study, U ...

The electron hopping between the two sites in a lattice is of fundamental importance in condensed matter physics. Precise control of the hopping strength allows for the prospect of manipulating the ...

Orsay, LAL. CALICEHKROC: an integrated readout chip designed to facilitate the readout of a large number of photomultiplier tubes for the next generation of neutrino experiments ...

Published in: Mon.Not.Roy.Astron.Soc. 527 (2024) 7459-7481 ...

physics and astro-ph and mathMade with by the INSPIRE Team ...

We have carried out an intensive survey of the northern region of the Fornax dwarf spheroidal galaxy with the aim of detecting the galaxy's short--period pulsating stars (P<0.25 days). Observations ...