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M. Rummel

31 papers hereh-index 17974 citations46 works total

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

author position
  • first author1
  • middle author12
  • last author11

Across the 24 of 31 papers where every author was matched, so the position is known.

fields
  • hep-th13
  • hep-ph10
  • gr-qc4
  • astro-ph.HE2
  • astro-ph.CO1
  • cs.LG1
same name
  • M. Rummel — 1 paper, h 12

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
20112021
most citedBuilding an explicit de Sitter

107 citations · 813 across the 31 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

hep-ph2014★ 18 cited

Observational consistency and future predictions for a 3.5 keV ALP to photon line

Pedro D. Alvarez, Joseph P. Conlon, Francesca V. Day +2

Motivated by the possibility of explaining the 3.5 keV line through dark matter decaying to axion-like particles that subsequently convert to photons, we study ALP-photon conversio…

hep-th2014★ 4 cited

De Sitter Vacua from a D-term Generated Racetrack Uplift

Markus Rummel, Yoske Sumitomo

We propose an uplift mechanism using a structure of multi-Kähler moduli dependence in the F-term potential of type IIB string theory compactifications. This mechanism requires a D-…

hep-ph2014★ 13 cited

ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster

David Kraljic, Markus Rummel, Joseph P. Conlon

It was recently found that the soft X-ray excess in the center of the Coma cluster can be fitted by conversion of axion-like-particles (ALPs) of a cosmic axion background (CAB) to…

hep-ph2014★ 99 cited

A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line

Michele Cicoli, Joseph P. Conlon, M. C. David Marsh +1

Galaxy clusters can efficiently convert axion-like particles (ALPs) to photons. We propose that the recently claimed detection of a 3.55--3.57 keV line in the stacked spectra of a…

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