activity
20232026
most citedGravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors

11 citations · 62 across the 22 of their papers we have counts for

collaborators

22 papers

hep-ph2026

Getting Warmer: IceCube Nears Freeze Out

Mainak Mukhopadhyay, Gordan Krnjaic

IceCube has recently detected a diffuse population of high-energy neutrinos arising from the Milky Way. We use this high-significance detection to place new limits on dark matter (…

astro-ph.HE2026

Constraints on magnetic monopoles from X-ray observations of neutron stars

Mainak Mukhopadhyay, Daniele Perri, Edward W. Kolb

Magnetic monopoles are captured efficiently by neutron stars, and if they catalyze nucleon decay, the decay products would thermalize and generate observable X-ray surface emission…

hep-ph2026

Galactic Center Neutrinos from Cosmic Ray-Dark Matter Interactions

Jorge Terol Calvo, Pedro de la Torre Luque, Mainak Mukhopadhyay +2

The IceCube and ANTARES collaborations have recently reported evidence for high-energy neutrinos associated with the Galactic plane and the Galactic Ridge, offering a new pathway t…

astro-ph.HE2026

Ultra high-energy cosmic rays from relativistic outflows in accretion induced collapse of white dwarfs

Mainak Mukhopadhyay, Shunsaku Horiuchi

When a rapidly-rotating, highly magnetized white dwarf (WD) approaches the Chandrashekhar limit through mass accretion, it can undergo an accretion-induced collapse (AIC) to form a…

astro-ph.HE2026

High-energy neutrino constraints on primordial black holes as dark matter

Mainak Mukhopadhyay, Joaquim Iguaz Juan

Primordial black holes (PBHs) are one of the most appealing dark matter candidates over a wide range of masses and abundances. This broad parameter space has been constrained by a…

astro-ph.HE2026

Neutrino and electromagnetic signatures from Superluminous Supernovae: a case study for SN 2017egm

Mainak Mukhopadhyay, Shigeo S. Kimura, Indrek Vurm +1

Superluminous supernovae (SLSNe) are rare transients that are times more luminous than ordinary stellar explosions, reaching peak optical luminosities $\sim 10^{44}…