activity
20182026
most citedSelf-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

53 citations · 67 across the 5 of their papers we have counts for

collaborators

8 papers

hep-ph2026

Solar-System Abundances of -Nuclides Probe Collective Neutrino Oscillations in Supernovae

Alexander Friedland, Derek J. Li, Giuseppe Lucente +3

Direct evidence for collective neutrino oscillations in core-collapse supernovae remains elusive. We show that this quantum phenomenon leaves a footprint on the abundance pattern o…

astro-ph.HE2023★ 1 cited

Successful -process in neutrino-driven outflows in core-collapse supernovae

Alexander Friedland, Payel Mukhopadhyay, Amol V. Patwardhan

The origin of the solar system abundances of several proton-rich isotopes, especially Mo and Ru, has been an enduring mystery in nuclear astrophysics. An attrac…

astro-ph.HE2023

A Hierarchical Framework for explaining the Cosmic Ray Spectrum using Diffusive Shock Acceleration

Roger Blandford, Paul Simeon, Noémie Globus +3

The hypothesis that the entire cosmic ray spectrum, from to energy, can be accounted for by diffusive shock acceleration on increasin…

astro-ph.HE2023★ 13 cited

Reacceleration of Galactic Cosmic Rays Beyond the Knee at the Termination Shock of a Cosmic-Ray-Driven Galactic Wind

Payel Mukhopadhyay, Enrico Peretti, Noemie Globus +2

The origin of cosmic rays above the knee in the spectrum is an unsolved problem. We present a wind model in which interstellar gas flows along a non-rotating, expanding flux tube w…

astro-ph.HE2021★ 53 cited

Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

Payel Mukhopadhyay, Tim Linden

Observations have shown that spatially extended "TeV halos" are a common (and potentially generic) feature surrounding young and middle-aged pulsars. However, their morphology is n…

astro-ph.HE2021

Celestial-Body Focused Dark Matter Annihilation Throughout the Galaxy

Rebecca K. Leane, Tim Linden, Payel Mukhopadhyay +1

Indirect detection experiments typically measure the flux of annihilating dark matter (DM) particles propagating freely through galactic halos. We consider a new scenario where cel…