دورية أكاديمية

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

التفاصيل البيبلوغرافية
العنوان: Second Data Release from the European Pulsar Timing Array: Challenging the Ultralight Dark Matter Paradigm.
المؤلفون: Smarra C; SISSA-International School for Advanced Studies, Via Bonomea 265, 34136, Trieste, Italy and INFN, Sezione di Trieste.; IFPU-Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy., Goncharov B; Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy.; INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy., Barausse E; SISSA-International School for Advanced Studies, Via Bonomea 265, 34136, Trieste, Italy and INFN, Sezione di Trieste.; IFPU-Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy., Antoniadis J; Institute of Astrophysics, FORTH, Nikolaou Plastira 100, 70013, Heraklion, Greece.; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Babak S; Université Paris Cité CNRS, Astroparticule et Cosmologie, 75013 Paris, France., Nielsen AB; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.; Fakultät für Physik, Universität Bielefeld, Postfach 100131, 33501 Bielefeld, Germany., Bassa CG; ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, The Netherlands., Berthereau A; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France., Bonetti M; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INAF - Osservatorio Astronomico di Brera, via Brera 20, I-20121 Milano, Italy., Bortolas E; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INAF - Osservatorio Astronomico di Brera, via Brera 20, I-20121 Milano, Italy., Brook PR; Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom., Burgay M; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy., Caballero RN; Hellenic Open University, School of Science and Technology, 26335 Patras, Greece., Chalumeau A; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy., Champion DJ; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Chanlaridis S; Institute of Astrophysics, FORTH, Nikolaou Plastira 100, 70013, Heraklion, Greece., Chen S; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China., Cognard I; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France., Desvignes G; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Falxa M; Université Paris Cité CNRS, Astroparticule et Cosmologie, 75013 Paris, France.; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France., Ferdman RD; School of Physics, Faculty of Science, University of East Anglia, Norwich NR4 7TJ, United Kingdom., Franchini A; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy., Gair JR; Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Muühlenberg 1, 14476 Potsdam, Germany., Graikou E; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Grießmeier JM; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France., Guillemot L; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France., Guo YJ; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Hu H; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Iraci F; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy.; Universitá di Cagliari, Dipartimento di Fisica, S.P. Monserrato-Sestu Km 0,700-09042 Monserrato (CA), Italy., Izquierdo-Villalba D; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy., Jang J; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Jawor J; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Janssen GH; ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, The Netherlands.; Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands., Jessner A; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Karuppusamy R; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Keane EF; School of Physics, Trinity College Dublin, College Green, Dublin 2, D02 PN40, Ireland., Keith MJ; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Kramer M; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Krishnakumar MA; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.; Fakultät für Physik, Universität Bielefeld, Postfach 100131, 33501 Bielefeld, Germany., Lackeos K; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Lee KJ; Institute of Astrophysics, FORTH, Nikolaou Plastira 100, 70013, Heraklion, Greece.; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France., Liu K; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Liu Y; Fakultät für Physik, Universität Bielefeld, Postfach 100131, 33501 Bielefeld, Germany.; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China., Lyne AG; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., McKee JW; E.A. Milne Centre for Astrophysics, University of Hull, Cottingham Road, Kingston-upon-Hull, HU6 7RX, United Kingdom.; Centre of Excellence for Data Science, Artificial Intelligence and Modelling (DAIM), University of Hull, Cottingham Road, Kingston-upon-Hull, HU6 7RX, United Kingdom., Main RA; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Mickaliger MB; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Niţu IC; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Parthasarathy A; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Perera BBP; Arecibo Observatory, HC3 Box 53995, Arecibo, Puerto Rico 00612., Perrodin D; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy., Petiteau A; Université Paris Cité CNRS, Astroparticule et Cosmologie, 75013 Paris, France.; IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France., Porayko NK; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy., Possenti A; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy., Leclere HQ; Université Paris Cité CNRS, Astroparticule et Cosmologie, 75013 Paris, France., Samajdar A; Institut für Physik und Astronomie, Universität Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, 14476, Potsdam, Germany., Sanidas SA; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Sesana A; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INAF - Osservatorio Astronomico di Brera, via Brera 20, I-20121 Milano, Italy., Shaifullah G; Dipartimento di Fisica 'G. Occhialini', Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy.; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy., Speri L; Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Muühlenberg 1, 14476 Potsdam, Germany., Spiewak R; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Stappers BW; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Susarla SC; Ollscoil na Gaillimhe-University of Galway, University Road, Galway H91 TK33, Ireland., Theureau G; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Université d'Orléans/CNRS, 45071 Orléans Cedex 02, France.; Observatoire Radioastronomique de Nançay, Observatoire de Paris, Université PSL, Université d'Orléans, CNRS, 18330 Nançay, France.; Laboratoire Univers et Théories LUTh, Observatoire de Paris, Université PSL, CNRS, Université de Paris, 92190 Meudon, France., Tiburzi C; INAF - Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy., van der Wateren E; ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, The Netherlands.; Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands., Vecchio A; Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom., Krishnan VV; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany., Wang J; Fakultät für Physik, Universität Bielefeld, Postfach 100131, 33501 Bielefeld, Germany.; Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute (AIRUB), 44780 Bochum, Germany.; Advanced Institute of Natural Sciences, Beijing Normal University, Zhuhai 519087, China., Wang L; Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom., Wu Z; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China.
مؤلفون مشاركون: European Pulsar Timing Array
المصدر: Physical review letters [Phys Rev Lett] 2023 Oct 27; Vol. 131 (17), pp. 171001.
نوع المنشور: Journal Article
اللغة: English
بيانات الدورية: Publisher: American Physical Society Country of Publication: United States NLM ID: 0401141 Publication Model: Print Cited Medium: Internet ISSN: 1079-7114 (Electronic) Linking ISSN: 00319007 NLM ISO Abbreviation: Phys Rev Lett Subsets: PubMed not MEDLINE; MEDLINE
أسماء مطبوعة: Original Publication: New York : American Physical Society
مستخلص: 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}.
تواريخ الأحداث: Date Created: 20231113 Latest Revision: 20231113
رمز التحديث: 20240628
DOI: 10.1103/PhysRevLett.131.171001
PMID: 37955508
قاعدة البيانات: MEDLINE
الوصف
تدمد:1079-7114
DOI:10.1103/PhysRevLett.131.171001