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researcher

D. Marsh

83 papers hereh-index 409.1k citations93 works total

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

author position
  • sole author9
  • first author16
  • middle author41
  • last author16

Across the 82 of 83 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO47
  • hep-ph22
  • hep-th9
  • astro-ph.HE2
  • astro-ph.IM1
  • gr-qc1
same name
  • D. Marsh — 5 papers, h 55
  • D. Marsh — 5 papers, h 4
  • D. Marsh — 2 papers, h 2
  • D. Marsh — 1 paper, h 1
  • D. Marsh — 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
20072024
most citedAxion Cosmology

2k citations · 9.3k across the 79 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.COShow all

4 papers · 2 filters

astro-ph.CO2013★ 23 cited

Constraining SUSY with Heavy Scalars -- using the CMB

Luca Iliesiu, David J. E. Marsh, Kavilan Moodley +1

If low-energy SUSY exists, LHC data favors a high mass scale for scalar superpartners (above a TeV), while sfermions and the dark matter can be parametrically lighter -- leading to…

astro-ph.CO2013★ 55 cited

Constraints on primordial magnetic fields from CMB distortions in the axiverse

Hiroyuki Tashiro, Joseph Silk, David J. E. Marsh

Measuring spectral distortions of the cosmic microwave background (CMB) is attracting considerable attention as a probe of high energy particle physics in the cosmological context,…

astro-ph.CO2013★ 237 cited

A Model For Halo Formation With Axion Mixed Dark Matter

David J. E. Marsh, Joe Silk

There are several issues to do with dwarf galaxy predictions in the standard ΛCDM cosmology that have suscitated much recent debate about the possible modification of the nature…

astro-ph.CO2013★ 28 cited

Axiverse cosmology and the energy scale of inflation

David J. E. Marsh, Daniel Grin, Renée Hlozek +1

Ultra-light axions (ma​≲10−18eV), motivated by string theory, can be a powerful probe of the energy scale of inflation. In contrast to heavier axions the isocurvature…

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