activity
20242026
collaborators

17 papers

astro-ph.HE2026

The location of the upper edge of the pair-instability supernovae black hole mass gap

Jeremy Sakstein, Djuna Croon

Gravitational wave observations are beginning to probe the upper edge of the pair-instability supernova (PISN) black hole mass gap, a key prediction of stellar evolution. In this w…

astro-ph.SR2026

Precision constraints on stellar physics from main sequence detached eclipsing binaries

Mitchell T. Dennis, Harry Desmond, Jeremy Sakstein

We present a Bayesian framework to constrain {mass (), metallicity (), stellar age (), and the convective mixing length parameter ()} in main-sequence (MS)…

hep-ph2026

Millicharged Particle Constraints from Asymptotic Giant Branch Stars

Damiano F. G. Fiorillo, Giuseppe Lucente, Jeremy Sakstein +1

We investigate the effect of millicharged particles (MCPs) with electric charge and mass on the late-stage evolution phases of low-mass stars in globular clusters.…

astro-ph.CO2026

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions

William Giarè, Jeremy Sakstein

We investigate whether early- and late-time dark energy could arise from a single scalar field. Adopting a bottom-up perspective, we first identify the sequence of dynamical regime…

hep-ph2026

Millicharged Particle Production During Late-Stage Stellar Evolution

Damiano F. G. Fiorillo, Giuseppe Lucente, Jeremy Sakstein +1

Stars are natural sources of feebly interacting particles, including putative particles with mass and electric charge . The emission of such millicharged particles (MCPs…

hep-ph2026

The Black Hole Mass Gap as a New Probe of Millicharged Particles

Damiano F. G. Fiorillo, Giuseppe Lucente, Jeremy Sakstein +2

We investigate the impact of millicharged particles (MCPs) on massive stars undergoing pulsational pair-instability supernovae and on the location of the lower edge of the black ho…