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M. Riquelme

21 papers hereh-index 10863 citations29 works total

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

author position
  • first author10
  • middle author7
  • last author3

Across the 20 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph4
  • astro-ph.SR2
  • physics.plasm-ph1
  • physics.space-ph1
same name
  • M. Riquelme — 15 papers, h 14
  • M. Riquelme — 3 papers
  • M. Riquelme — 2 papers, h 1
  • M. Riquelme — 1 paper, h 1

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
20052026
most citedThe microphysics of collisionless shock waves

272 citations · 1k across the 21 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 174 cited

Non-linear Study of Bell's Cosmic Ray Current-driven Instability

Mario A. Riquelme, Anatoly Spitkovsky

The cosmic ray current-driven (CRCD) instability, predicted by Bell (2004), consists of non-resonant, growing plasma waves driven by the electric current of cosmic rays (CRs) that…

astro-ph2007★ 59 cited

Lower Metal Enrichment of Virialized Gas in Minihalos

Renyue Cen, Mario A. Riquelme

We differentiate between the metal enrichment of the gas in virialized minihalos and that of the intergalactic medium at high redshift, pertinent to cosmological reionization, with…

astro-ph2006★ 12 cited

Separating the Weak Lensing and Kinetic SZ Effects from CMB Temperature Maps

Mario A. Riquelme, David N. Spergel

A new generation of CMB experiments will soon make sensitive high resolution maps of the microwave sky. At angular scales less than ∼10 arcminutes, most CMB anisotropies are g…

astro-ph2005★ 9 cited

Neutrino emission rates in highly magnetized neutron stars revisited

Mario Riquelme, Andreas Reisenegger, Olivier Espinosa +1

Magnetars are a subclass of neutron stars whose intense soft-gamma-ray bursts and quiescent X-ray emission are believed to be powered by the decay of a strong internal magnetic fie…

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