activity
19932026
most citedObservation of interstellar lithium in the low-metallicity Small Magellanic Cloud

70 citations · 495 across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2026

Neutron Star Merger Universality Relations for a Quark--Hadron Crossover Equation of State

Wei Sun, Grant J. Mathews, Atul Kedia

A crossover transition from hadronic to quark matter during the merger of neutron stars can lead to interesting observational consequences in the emergent gravitational radiation.…

astro-ph.CO2026

Loss-Cone-Limited Dark Matter Accretion onto Early Black Hole Seeds

Brian Zhang, Grant J. Mathews

The rapid appearance of supermassive black holes at high redshift motivates a reassessment of non-baryonic growth channels. We develop a loss-cone framework for collisionless dark-…

nucl-ex2026

Precision Mass Measurements of \textsuperscript{130}Te, \textsuperscript{130}Sn, and Their Impact on Models for R-Process Nucleosynthesis

A. Cannon, W. S. Porter, A. A. Valverde +12

The astrophysical rapid neutron capture nucleosynthesis process (r-process) remains an active area of research due to the fact that it occurs in extreme conditions and involves rea…

astro-ph.HE2018★ 2 cited

On the role of the Kerr-Newman black hole in the GeV emission of long gamma-ray bursts

R. Ruffini, R. Moradi, J. A. Rueda +13

X-ray Flashes (XRFs), binary-driven hypernovae (BdHNe) are long GRB subclasses with progenitor a CO, undergoing a supernova (SN) explosion and hypercritically accretin…

astro-ph.HE2018

On the Short GRB GeV emission from a Kerr Black hole

R. Ruffini, M. Muccino, Y. Aimuratov +10

It has recently become clear that in both short and long gamma-ray bursts (GRBs) it coexists a sequence of different events, each characterized by specific physical processes and c…

astro-ph.HE2017★ 29 cited

On a GRB afterglow model consistent with hypernovae observations

R. Ruffini, M. Karlica, N. Sahakyan +5

We describe the afterglows of the long gamma-ray-burst (GRB) 130427A within the context of a binary-driven hypernova (BdHN). The afterglows originate from the interaction between a…