activity
20132025
most citedSensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run

415 citations · 3.6k across the 40 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2018★ 5 cited

Time variability of TeV cosmic ray sky map

Rahul Kumar, Noemie Globus, David Eichler +1

The variation in the intensity of cosmic rays at small angular scales is attributed to the interstellar turbulence in the vicinity of the Solar system. We show that {a turbulent or…

astro-ph.HE2016★ 7 cited

Ultrahigh Energy Cosmic Rays: A Galactic Origin?

David Eichler, Noemie Globus, Rahul Kumar +1

It is suggested that essentially all of the UHECRs we detect, including those at the highest energy, originate in our Galaxy. It is shown that even if the density of sources decrea…

astro-ph.HE2015

Electron Heating in a Relativistic, Weibel-Unstable Plasma

Rahul Kumar, David Eichler, Michael Gedalin

The dynamics of two initially unmagnetized relativistic counter-streaming homogeneous ion-electron plasma beams are simulated in two dimensions using the particle-in-cell (PIC) met…

astro-ph.HE2013★ 13 cited

The isotropy problem of Sub-ankle Ultra-high energy cosmic rays

Rahul Kumar, David Eichler

We study the time dependent propagation of sub-ankle ultra-high energy cosmic rays (UHECRs) originating from point-like Galactic sources. We show that drift in the Galactic magneti…

astro-ph.HE2013★ 34 cited

Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +875

Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massive stars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We inv…

astro-ph.HE2013★ 5 cited

Is the Galactic Cosmic Ray Spectrum Constant in Time?

David Eichler, Rahul Kumar, Martin Pohl

The hypothesis is considered that the present Galactic cosmic ray spectrum is at present softer than its time average due to source intermittency. Measurements of muogenic nuclides…