Repeated Gravitational Wave Bursts from Cosmic Strings

التفاصيل البيبلوغرافية
العنوان: Repeated Gravitational Wave Bursts from Cosmic Strings
المؤلفون: Auclair, Pierre, Steer, Danièle A., Vachaspati, Tanmay
المساهمون: AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
سنة النشر: 2023
مصطلحات موضوعية: High Energy Physics - Theory, LISA, wave function, Cosmology and Nongalactic Astrophysics (astro-ph.CO), string tension, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), localization, General Relativity and Quantum Cosmology, detector: sensitivity, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), VIRGO, High Energy Physics - Theory (hep-th), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], gravitational radiation: burst, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], string: closed, KAGRA, LIGO, cosmic string, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], signature, Astrophysics - Cosmology and Nongalactic Astrophysics
الوصف: A characteristic observational signature of cosmic strings are short duration gravitational wave (GW) bursts. These have been searched for by the LIGO-Virgo-KAGRA (LVK) collaboration, and will be searched for with LISA. We point out that these burst signals are repeated, since cosmic string loops evolve quasi-periodically in time, and will always appear from essentially the same position in the sky. We estimate the number of GW repeaters for LVK and LISA, and show that the string tension that can be probed scales as detector sensitivity to the sixth power, which raises hope for detection in future GW detectors. The observation of repeated GW bursts from the same cosmic string loop helps distinguish between the GW waveform parameters and the sky-localization.
5 pages, 2 figures, prepared for submission to Physical Review
اللغة: English
الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb0dba8390301f9cd7fd8888f7f84808Test
http://arxiv.org/abs/2306.08331Test
حقوق: OPEN
رقم الانضمام: edsair.doi.dedup.....bb0dba8390301f9cd7fd8888f7f84808
قاعدة البيانات: OpenAIRE