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Title: The gamma-ray luminosity function of millisecond pulsars and implications for the GeV excess

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2]
  1. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  2. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Kansas, Lawrence, KS (United States)

It has been proposed that a large population of unresolved millisecond pulsars (MSPs) could potentially account for the excess of GeV-scale gamma-rays observed from the region surrounding the Galactic Center. The viability of this scenario depends critically on the gamma-ray luminosity function of this source population, which determines how many MSPs Fermi should have already detected as resolved point sources. In this paper, we revisit the gamma-ray luminosity function of MSPs, without relying on uncertain distance measurements. Our determination, based on a comparison of models with the observed characteristics of the MSP population, suggests that Fermi should have already detected a significant number of sources associated with such a hypothesized Inner Galaxy population. As a result, we cannot rule out a scenario in which the MSPs residing near the Galactic Center are systematically less luminous than those present in the Galactic Plane or within globular clusters.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1249200
Report Number(s):
FERMILAB-PUB-15-559-A; arXiv:1512.04966; 1409878
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 1603, Issue 03; ISSN 1475-7516
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 37 works
Citation information provided by
Web of Science

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Cited By (21)

Model-independent analysis of the DAMPE excess journal February 2018
Lepton-flavor violating mediators journal March 2017
Hidden Higgs portal vector dark matter for the Galactic center gamma-ray excess from the two-step cascade annihilation, and muon g − 2 journal August 2018
Disrupted globular clusters and the gamma-ray excess in the Galactic Centre journal January 2018
Bayesian model comparison and analysis of the Galactic disc population of gamma-ray millisecond pulsars journal September 2018
Analyzing the gamma-ray sky with wavelets journal August 2018
Inverse Compton emission from millisecond pulsars in the Galactic bulge journal June 2019
Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM journal May 2018
Impact of Cosmic-Ray Physics on Dark Matter Indirect Searches journal December 2018
Multimessenger Multi-TeV Dark Matter journal April 2019
Millisecond Pulsar Origin of the Galactic Center Excess and Extended Gamma-Ray Emission from Andromeda: A Closer Look journal July 2018
Population Syntheses of Millisecond Pulsars from the Galactic Disk and Bulge journal August 2018
Ruling Out ∼100–300 GeV Thermal Relic Annihilating Dark Matter by Radio Observation of the Andromeda Galaxy journal February 2019
ESTIMATING THE GeV EMISSION OF MILLISECOND PULSARS IN DWARF SPHEROIDAL GALAXIES journal November 2016
Lepton-Flavor Violating Mediators text January 2016
Disrupted Globular Clusters and the Gamma-Ray Excess in the Galactic Centre text January 2017
Model-independent analysis of the DAMPE excess text January 2017
Bayesian Model Comparison and Analysis of the Galactic Disk Population of Gamma-Ray Millisecond Pulsars text January 2018
Population syntheses of millisecond pulsars from the Galactic Disk and Bulge text January 2018
Ruling out $\sim 100-300$ GeV thermal relic annihilating dark matter by radio observation of the Andromeda galaxy text January 2019
An alternative Explanation for the Fermi GeV Gamma-Ray Excess preprint January 2016

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