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D. Mukherjee

4 papers hereh-index 341 citations16 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • hep-ph2
  • astro-ph.SR1
  • stat.ME1
same name
  • D. Mukherjee — 5 papers, h 48
  • D. Mukherjee — 5 papers
  • D. Mukherjee — 4 papers, h 5
  • D. Mukherjee — 3 papers, h 1
  • D. Mukherjee — 3 papers, h 7
  • D. Mukherjee — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2026

Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube

Dwaipayan Mukherjee, Mohamed Rameez, Basudeb Dasgupta

Simulations of core-collapse supernovae have revealed an epoch of hydrodynamic instability in which the matter of the collapsing star undergoes quasi-periodic oscillations, known a…

stat.ME2026

Some bivariate distributions on a discrete torus with application to wind direction datasets

Brajesh Kumar Dhakad, Jayant Jha, Debepsita Mukherjee

Many datasets are observed on a finite set of equally spaced directions instead of the exact angles, such as the wind direction data. However, in the statistical literature, bivari…

hep-ph2026

Sufficient and Necessary Conditions for Collective Neutrino Instability: Fast, Slow, and Mixed

Basudeb Dasgupta, Dwaipayan Mukherjee

Collective neutrino oscillations exhibit instabilities that induce appreciable flavor conversion, with crucial astrophysical implications. While the importance of initial phase-spa…

hep-ph2025

IceCube PeV neutrinos from heavy dark matter decay with 12 years HESE data

Diptarko Mukherjee, Ashadul Halder, Debasish Majumdar +1

The decay of superheavy dark matter from the early universe may undergo decay via QCD cascades and electroweak cascade to produce neutrinos as one of the decay products. We conside…

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