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Matt L Sampson

5 papers hereh-index 347 citations6 works total

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

author position
  • first author3
  • middle author1
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • Matt L Sampson — 5 papers, h 3

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
20222025
most citedTurbulent diffusion of streaming cosmic rays in compressible, partially ionised plasma

30 citations · 47 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2025

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium

Matt L. Sampson, James R. Beattie, Romain Teyssier +5

Cosmic rays (CRs) are an integral part of the non-thermal pressure budget in the interstellar medium (ISM) and are the leading-order ionization mechanism in cold molecular clouds.…

astro-ph.GA2022★ 30 cited

Turbulent diffusion of streaming cosmic rays in compressible, partially ionised plasma

Matt L. Sampson, James R. Beattie, Mark R. Krumholz +3

Cosmic rays (CRs) are a dynamically important component of the interstellar medium (ISM) of galaxies. The ∼GeV CRs that carry most CR energy and pressure are likely confined b…

astro-ph.GA2022★ 1 cited

Ion Alfvén velocity fluctuations and implications for the diffusion of streaming cosmic rays

James R. Beattie, Mark R. Krumholz, Christoph Federrath +2

The interstellar medium (ISM) of star-forming galaxies is magnetized and turbulent. Cosmic rays (CRs) propagate through it, and those with energies from ∼GeV−TeV…

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