Multimessenger science reach and analysis method for common sources of gravitational waves and high-energy neutrinos

B. Baret; Imre Bartos; B. Bouhou; E. Chassande-Mottin; Alessandra Corsi; Irene Di Palma; Corinne Donzaud; Marco Drago; Chad Finley; Gareth Jones; Sergey Klimenko; A. Kouchner; Szabolcs Márka; Zsuzsa Márka; Luciano Moscoso; Maria Alessandra Papa; T. Pradier; Giovanni Prodi; Peter Raffai; Virginia Re; Jameson Rollins; Francesco Salemi; Patrick Sutton; Maggie Tse; V. Van Elewyck; Gabriele Vedovato

HAL : in2p3-00709825, version 1

arXiv : arXiv:1112.1140

Code Bibliographique ADS : 2012PhRvD..85j3004B

DOI : 10.1103/PhysRevD.85.103004

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Multimessenger science reach and analysis method for common sources of gravitational waves and high-energy neutrinos
Baret B., Bartos I., Bouhou B., Chassande-Mottin E., Corsi A. et al
Physical Review D 85 (2012) 103004 - http://hal.in2p3.fr/in2p3-00709825

Thème(s) :

Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie

Physique/Astrophysique/Phénomènes cosmiques de haute energie

Titre :

Multimessenger science reach and analysis method for common sources of gravitational waves and high-energy neutrinos

Auteur :

B. Baret¹, Imre Bartos, B. Bouhou¹, E. Chassande-Mottin¹, Alessandra Corsi, Irene Di Palma, Corinne Donzaud, Marco Drago, Chad Finley, Gareth Jones, Sergey Klimenko, A. Kouchner, Szabolcs Márka, Zsuzsa Márka, Luciano Moscoso, Maria Alessandra Papa, T. Pradier², Giovanni Prodi, Peter Raffai, Virginia Re, Jameson Rollins, Francesco Salemi, Patrick Sutton, Maggie Tse, V. Van Elewyck¹, Gabriele Vedovato

Laboratoire :

1 :	APC - AstroParticule et Cosmologie

http://www.apc.univ-paris7.fr/

CNRS : UMR7164 – IN2P3 – Observatoire de Paris – Université Paris VII - Paris Diderot – CEA : DSM/IRFU

10, rue Alice Domon et Léonie Duquet 75205 Paris Cedex 13

France

2 :	IPHC - Institut Pluridisciplinaire Hubert Curien

CNRS : UMR7178 – Université de Strasbourg

France

équipe(s) de recherche :

APC - AHE
APC - ADAMIS

Résumé :

We present the baseline multimessenger analysis method for the joint observations of gravitational waves (GW) and high-energy neutrinos (HEN), together with a detailed analysis of the expected science reach of the joint search. The analysis method combines data from GW and HEN detectors, and uses the blue-luminosity-weighted distribution of galaxies. We derive expected GW+HEN source rate upper limits for a wide range of source parameters covering several emission models. Using published sensitivities of externally triggered searches, we derive joint upper limit estimates both for the ongoing analysis with the initial LIGO-Virgo GW detectors with the partial IceCube detector (22 strings) HEN detector and for projected results to advanced LIGO-Virgo detectors with the completed IceCube (86 strings). We discuss the constraints these upper limits impose on some existing GW+HEN emission models.

Type de publication :

Articles dans des revues avec comité de lecture

Date de publication
ou d'écriture :

05/2012

Nom du périodique :

Physical Review D (Phys. Rev. D)
Publisher	American Physical Society
ISSN	1550-7998 (eISSN : 1550-2368)

Volume :

Page/Article :

103004

Mot(s)-clé(s) :

Gravitational radiation detectors – mass spectrometers – and other instrumentation and techniques – Neutrino – muon – pion – and other elementary particle detectors – cosmic ray detectors – Supernovae – gamma-ray sources – gamma-ray bursts

Lien vers le texte intégral :

http://fr.arXiv.org/abs/arXiv:1112.1140


in2p3-00709825, version 1
http://hal.in2p3.fr/in2p3-00709825
oai:hal.in2p3.fr:in2p3-00709825
Contributeur : Bruny Baret <>
Soumis le : Mardi 19 Juin 2012, 15:05:58
Dernière modification le : Mercredi 20 Juin 2012, 14:58:32