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. 2023 Oct 27;131(17):171001.
doi: 10.1103/PhysRevLett.131.171001.

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

Clemente Smarra  1   2 Boris Goncharov  3   4 Enrico Barausse  1   2 J Antoniadis  5   6 S Babak  7 A-S Bak Nielsen  6   8 C G Bassa  9 A Berthereau  10   11 M Bonetti  12   13   14 E Bortolas  12   13   14 P R Brook  15 M Burgay  16 R N Caballero  17 A Chalumeau  12 D J Champion  6 S Chanlaridis  5 S Chen  18 I Cognard  10   11 G Desvignes  6 M Falxa  7   10 R D Ferdman  19 A Franchini  12   13 J R Gair  20 E Graikou  6 J-M Grießmeier  10   11 L Guillemot  10   11 Y J Guo  6 H Hu  6 F Iraci  16   21 D Izquierdo-Villalba  12   13 J Jang  6 J Jawor  6 G H Janssen  9   22 A Jessner  6 R Karuppusamy  6 E F Keane  23 M J Keith  24 M Kramer  6   24 M A Krishnakumar  6   8 K Lackeos  6 K J Lee  5   6   11 K Liu  6 Y Liu  8   25 A G Lyne  24 J W McKee  26   27 R A Main  6 M B Mickaliger  24 I C Niţu  24 A Parthasarathy  6 B B P Perera  28 D Perrodin  16 A Petiteau  7   29 N K Porayko  6   12 A Possenti  16 H Quelquejay Leclere  7 A Samajdar  30 S A Sanidas  24 A Sesana  12   13   14 G Shaifullah  12   13   16 L Speri  20 R Spiewak  24 B W Stappers  24 S C Susarla  31 G Theureau  10   11   32 C Tiburzi  16 E van der Wateren  9   22 A Vecchio  15 V Venkatraman Krishnan  6 J Wang  8   33   34 L Wang  24 Z Wu  25 European Pulsar Timing Array
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Free article

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

Clemente Smarra et al. Phys Rev Lett. .
Free article

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≲m≲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/cm^{3}.

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