We present our methods to fit the two point correlators for light, strange, and charmed pseudoscalar meson physics with the highly improved staggered…

Neutron stars and black holes are the astrophysical systems with the strongest gravitational fields in the universe. In this article, I review the pr…

We present preliminary results for light, strange and charmed pseudoscalar meson physics from simulations using four flavors of dynamical quarks with…

The role of electron-phonon interactions is experimentally and theoretically investigated near the saddle point absorption peak of graphene. The diff…

We calculate the leptonic decay constants of heavy-light pseudoscalar mesons with charm and bottom quarks in lattice quantum chromodynamics on four-f…

Dynamical mass measurements to date have allowed determinations of the mass M and the distance D of a number of nearby supermassive black holes. In t…

We have proved the factorization of two-jet event shape distributions in soft collinear effective theory without assuming the factorization of hadronic final states into separate colored collinear and soft sectors as in previous discussions. To do t…

We present a new analysis of two-jet event shape distributions in soft collinear effective theory. Extending previous results, we observe that a larg…

The AMS-02 experiment has recently released data which confirms a rise in the cosmic-ray positron fraction as a function of energy up to approximatel…

We assess the potential of nuclear starburst disks to obscure the Seyfert-like AGN that dominate the hard X-ray background at z~1. Over 1200 starburs…

According to string theory, string ball is a highly excited long string which decays to standard model particles at the Hagedorn temperature with the…

We explore electroweak precision observables (EWPO) and $B$-physics observables (BPO) in the CMSSM, the mGMSB and the mAMSB. We perform a chi^2 analy…

We review the latest attempts to determine the accretion geometry in radio-loud active galactic nuclei (AGN). These objects, which comprise ~10-20% o…

Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real t…

We calculate the number of dark matter particles that a neutron star accumulates over its lifetime as it rotates around the center of a galaxy, when …

We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC and the Large Hadron Collider to constrain pertu…

We investigate the evolution of extreme ultraviolet (XUV) spectral lineshapes in an optically-thick helium gas under near-infrared (IR) perturbation.…

This paper describes a revised photometric calibration of the \emph{Galaxy Evolution Explorer} magnitudes, based on measurements of DA white dwarfs. …

According to the no-hair theorem, astrophysical black holes are uniquely described by their mass and spin. In this paper, we review a new framework f…

According to the no-hair theorem, an astrophysical black hole is uniquely described by only two quantities, the mass and the spin. In this series of …

We present a progress report on our calculation of the decay constants $f_B$ and $f_{B_s}$ from lattice-QCD simulations with highly-improved staggere…

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