Pulsar Timing Array experiments probe the presence of possible scalar or pseudoscalar ultralight dark matter particles through decade-long timing of an ensemble of galactic millisecond radio pulsars. With the second data release of the European Pulsar Timing Array, we focus on the most robust scenario, in which dark matter interacts only gravitationally with ordinary baryonic matter. Our results show that ultralight particles with masses 10-24.0 eV 10-23.3 eV cannot constitute 100% of the measured local dark matter density, but can have at most local density ρ 0.3 GeV/cm3.

Second Data Release from the European Pulsar Timing Array: Challenging the Ultralight Dark Matter Paradigm / C. Smarra, B. Goncharov, E. Barausse, J. Antoniadis, S. Babak, A.B. Nielsen, C.G. Bassa, A. Berthereau, M. Bonetti, E. Bortolas, P.R. Brook, M. Burgay, R.N. Caballero, A. Chalumeau, D.J. Champion, S. Chanlaridis, S. Chen, I. Cognard, G. Desvignes, M. Falxa, R.D. Ferdman, A. Franchini, J.R. Gair, E. Graikou, J. Grießmeier, L. Guillemot, Y.J. Guo, H. Hu, F. Iraci, D. Izquierdo-Villalba, J. Jang, J. Jawor, G.H. Janssen, A. Jessner, R. Karuppusamy, E.F. Keane, M.J. Keith, M. Kramer, M.A. Krishnakumar, K. Lackeos, K.J. Lee, K. Liu, Y. Liu, A.G. Lyne, J.W. Mckee, R.A. Main, M.B. Mickaliger, I.C. Niţu, A. Parthasarathy, B.B.P. Perera, D. Perrodin, A. Petiteau, N.K. Porayko, A. Possenti, H.Q. Leclere, A. Samajdar, S.A. Sanidas, A. Sesana, G. Shaifullah, L. Speri, R. Spiewak, B.W. Stappers, S.C. Susarla, G. Theureau, C. Tiburzi, E. van der Wateren, A. Vecchio, V.V. Krishnan, J. Wang, L. Wang, Z. Wu. - In: PHYSICAL REVIEW LETTERS. - ISSN 1079-7114. - 131:17(2023 Oct 27), pp. 171001.1-171001.9. [10.1103/PhysRevLett.131.171001]

Second Data Release from the European Pulsar Timing Array: Challenging the Ultralight Dark Matter Paradigm

A. Franchini;
2023

Abstract

Pulsar Timing Array experiments probe the presence of possible scalar or pseudoscalar ultralight dark matter particles through decade-long timing of an ensemble of galactic millisecond radio pulsars. With the second data release of the European Pulsar Timing Array, we focus on the most robust scenario, in which dark matter interacts only gravitationally with ordinary baryonic matter. Our results show that ultralight particles with masses 10-24.0 eV 10-23.3 eV cannot constitute 100% of the measured local dark matter density, but can have at most local density ρ 0.3 GeV/cm3.
Settore PHYS-05/A - Astrofisica, cosmologia e scienza dello spazio
   Astrophysics and Cosmology Research at the JBCA 2020-2023
   UK Research and Innovation
   STFC
   ST/T000414/1

   Astrophysics at the University of Birmingham - Consolidated grant 2022-2025
   UK Research and Innovation
   STFC
   ST/W000946/1

   Large European Array for Pulsars
   LEAP
   European Commission
   SEVENTH FRAMEWORK PROGRAMME
   227947

   ARGOS Conceptual Design Study: Designing a next-generation radio facility for multi-messenger astronomy
   ARGOS-CDS
   European Commission
   Horizon Europe Framework Programme
   101094354

   Gravitational Universe: Challenges and Opportunities
   GRU
   European Commission
   Horizon 2020 Framework Programme
   101007855

   Imaging the Event Horizon of Black Holes
   BLACKHOLECAM
   European Commission
   SEVENTH FRAMEWORK PROGRAMME
   610058

   Binary massive black hole astrophysics
   B Massive
   European Commission
   Horizon 2020 Framework Programme
   818691

   Gravitational Universe: Challenges and Opportunities
   GRU
   European Commission
   Horizon 2020 Framework Programme
   101007855

   AccelNet-Implementation: The International Pulsar Timing Array
   National Science Foundation
   Office of the Director
   2114721
27-ott-2023
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1160135
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