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researcher

A. Bret

49 papers hereh-index 242.4k citations148 works total

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

author position
  • sole author19
  • first author13
  • middle author12
  • last author3

Across the 47 of 49 papers where every author was matched, so the position is known.

fields
  • physics.plasm-ph34
  • astro-ph.HE12
  • astro-ph1
  • astro-ph.SR1
  • physics.pop-ph1
same name
  • A. Bret — 20 papers, h 6
  • A. Bret — 8 papers, h 2
  • A. Bret — 3 papers, h 1
  • A. Bret — 1 paper, h 4

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

activity
20052023
most citedThe microphysics of collisionless shock waves

272 citations · 984 across the 47 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.HEShow all

4 papers · 2 filters

astro-ph.HE2012★ 37 cited

Nonrelativistic parallel shocks in unmagnetized and weakly magnetized plasmas

Jacek Niemiec, Martin Pohl, Antoine Bret +1

We present results of 2D3V particle-in-cell simulations of non-relativistic plasma collisions with absent or parallel large-scale magnetic field for parameters applicable to the co…

astro-ph.HE2012

CfA Plasma Talks

Antoine Bret

Notes from a series of 13 one hour (or more) lectures on Plasma Physics given to Ramesh Narayan' research group at the Harvard-Smithsonian Center for Astrophysics, between January…

astro-ph.HE2012★ 8 cited

PIC simulation of a thermal anisotropy-driven Weibel instability in a circular rarefaction wave

M. E. Dieckmann, G. Sarri, G. C. Murphy +6

The expansion of an initially unmagnetized planar rarefaction wave has recently been shown to trigger a thermal anisotropy-driven Weibel instability (TAWI), which can generate magn…

astro-ph.HE2012★ 13 cited

Could Cosmic Rays Affect Instabilities in the Transition Layer of Nonrelativistic Collisionless Shocks?

Thomas Stroman, Martin Pohl, Jacek Niemiec +1

There is an observational correlation between astrophysical shocks and non-thermal particle distributions extending to high energies. As a first step toward investigating the possi…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.