Massive, massless and ghost modes of gravitational waves from higher-order gravity
被引:92
|
作者:
Bogdanos, Charalampos
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机构:
Univ Paris 11, LPT, F-91405 Orsay, FranceUniv Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
Bogdanos, Charalampos
[2
]
Capozziello, Salvatore
论文数: 0引用数: 0
h-index: 0
机构:
Univ Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
Compl Univ Monte S Angelo, INFN Sez Napoli, I-80126 Naples, ItalyUniv Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
Capozziello, Salvatore
[1
,3
]
De Laurentis, Mariafelicia
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h-index: 0
机构:
Univ Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
Compl Univ Monte S Angelo, INFN Sez Napoli, I-80126 Naples, ItalyUniv Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
De Laurentis, Mariafelicia
[1
,3
]
Nesseris, Savvas
论文数: 0引用数: 0
h-index: 0
机构:
Niels Bohr Inst, Niels Bohr Int Acad, DK-2100 Copenhagen O, DenmarkUniv Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
Nesseris, Savvas
[4
]
机构:
[1] Univ Napoli Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy
[2] Univ Paris 11, LPT, F-91405 Orsay, France
[3] Compl Univ Monte S Angelo, INFN Sez Napoli, I-80126 Naples, Italy
[4] Niels Bohr Inst, Niels Bohr Int Acad, DK-2100 Copenhagen O, Denmark
Gravitational waves;
Alternative theories of gravity;
Cosmology;
D O I:
10.1016/j.astropartphys.2010.08.001
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We linearize the field equations for higher order theories that contain scalar invariants other than the Ricci scalar. We find that besides a massless spin-2 field (the standard graviton), the theory contains also spin-0 and spin-2 massive modes. Then, we investigate the possible detectability of such additional polarization modes of a stochastic gravitational wave by ground-based and space interferometric detectors. Finally, we extend the formalism of the cross-correlation analysis, including the additional polarization modes, and calculate the detectable energy density of the spectrum for a stochastic background of the relic gravity waves that corresponds to our model. For the situation considered here, we find that these massive modes are certainly of interest for direct detection by the LISA experiment. (C) 2010 Elsevier B.V. All rights reserved.
机构:
Univ Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Univ Illinois, Dept Phys, Champaign, IL 61820 USAUniv Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Perkins, Scott E.
Nair, Remya
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机构:
Montana State Univ, Dept Phys, eXtreme Grav Inst, Bozeman, MT 59717 USAUniv Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Nair, Remya
Silva, Hector O.
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机构:
Univ Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Univ Illinois, Dept Phys, Champaign, IL 61820 USA
Albert Einstein Inst, Max Planck Inst Gravitat Phys, Muhlenberg 1, D-14476 Potsdam, GermanyUniv Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Silva, Hector O.
Yunes, Nicolas
论文数: 0引用数: 0
h-index: 0
机构:
Univ Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA
Univ Illinois, Dept Phys, Champaign, IL 61820 USAUniv Illinois, Illinois Ctr Adv Study Universe, Champaign, IL 61820 USA