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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., Di Palma, I., et al. (2011). Multimessenger Science Reach and Analysis Method for Common Sources of Gravitational Waves and High-energy Neutrinos. Physical Review D, 85: 103004. doi:10.1103/PhysRevD.85.103004.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-7C94-8 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-7C95-6
Genre: Journal Article

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1112.1140v2.pdf (Preprint), 2MB
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 Creators:
Baret, Bruny, Author
Bartos, Imre, Author
Bouhou, Boutayeb, Author
Chassande-Mottin, Eric, Author
Corsi, Alessandra, Author
Di Palma, Irene1, Author              
Donzaud, Corinne, Author
Drago, Marco, Author
Finley, Chad, Author
Jones, Gareth, Author
Klimenko, Sergey, Author
Kouchner, Antoine, Author
Márka, Szabolcs, Author
Márka, Zsuzsa, Author
Moscoso, Luciano, Author
Papa, Maria Alessandra2, Author              
Pradier, Thierry, Author
Prodi, Giovanni, Author
Raffai, Peter, Author
Re, Virginia, Author
Rollins, Jameson, AuthorSalemi, Francesco1, Author              Sutton, Patrick, AuthorTse, Maggie, AuthorVan Elewyck, Véronique, AuthorVedovato, Gabriele, Author more..
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24011              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: 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.

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 Dates: 2011
 Publication Status: Published in print
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 Identifiers: DOI: 10.1103/PhysRevD.85.103004
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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : Published for the American Physical Society by the American Institute of Physics
Pages: - Volume / Issue: 85 Sequence Number: 103004 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111088197762258