Emission of gravitational radiation in scalar-tensor and f(R)-theories

Références bibliographiques

• Abbott BP et al (2016) GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence. Phys Rev Lett 116(24):241103
• Abbott BP et al (2016) Binary black hole mergers in the first advanced LIGO observing run. Phys Rev X 6(4):041015. [Erratum: Phys.Rev.X 8, 039903 (2018)]
• Abbott BP et al (2016) Properties of the binary black hole merger GW150914. Phys Rev Lett 116(24):241102
• Abbott BP et al (2016) Tests of general relativity with GW150914. Phys Rev Lett 116(22):221101. [Erratum: Phys.Rev.Lett. 121, 129902 (2018)]
• Amendola L and Euclid Theory Working Group (2013) Cosmology and fundamental physics with the Euclid satellite. Living Rev Relativ 16(6)
• Amendola L, Tsujikawa S (2008) Phantom crossing, equation-of-state singularities, and local gravity constraints in f(r) models. Phys Lett B 660(3):125–132
• Antoniadis J, Freire PCC, Wex N, Tauris TM, Lynch RS, van Kerkwijk MH, Kramer M, Bassa C, Dhillon VS, Driebe T et al (2013) A massive pulsar in a compact relativistic binary. Science 340(6131):1233232–1233232
• Arun KG, Iyer BR, Qusailah MSS, Sathyaprakash BS (2006) Probing the non-linear structure of general relativity with black hole binaries. Phys Rev D 74:024006
• Barrow JD, Ottewill AC (1983) The stability of general relativistic cosmological theory. J Phys A Math Gen 16(12):2757–2776
• Bekenstein JD (1973) Gravitational-radiation recoil and runaway black holes. Astrophys J 183:657–664
• Bertone G, Hooper D (2018) History of dark matter. Rev Mod Phys 90(4):045002
• Bertone G, Hooper D, Silk J (2005) Particle dark matter: evidence, candidates and constraints. Phys Rep 405(5–6):279–390
• Blanchet L, Damour T, Iyer BR Gravitational waves from inspiralling compact binaries: energy loss and wave form to second postNewtonian order. Phys Rev D 51:5360 (1995) [Erratum: Phys.Rev.D 54, 1860 (1996)]
• Blanchet L, Sathyaprakash BS (1994) Signal analysis of gravitational wave tails. Class Quantum Grav 11(11):2807–2831
• Bogdanos C, Capozziello S, De Laurentis M, Nesseris S (2010) Massive, massless and ghost modes of gravitational waves from higher-order gravity. Astropart Phys 34(4):236–244
• Brans C, Dicke RH (1961) Mach’s principle and a relativistic theory of gravitation. Phys Rev 124:925–935
• Buonanno A, Iyer B, Ochsner E, Pan Y, Sathyaprakash BS (2009) Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors. Phys Rev D 80:084043
• Capozziello S, Cardone VF, Troisi A (2007) Low surface brightness galaxy rotation curves in the low energy limit of rn gravity: no need for dark matter? Mon Not R Astron Soc 375(4):1423–1440
• Capozziello S, De Laurentis M (2011) Extended theories of gravity. Phys Rep 509(4–5):167–321
• Capozziello S, De Laurentis M (2012) The dark matter problem from f(R) gravity viewpoint. Ann Phys 524(9–10):545–578
• Capozziello S, De Laurentis M, Nojiri S, Odintsov SD (2009) f(r) gravity constrained by ppn parameters and stochastic background of gravitational waves. Gen Relativ Gravit 41(10):2313–2344
• Capozziello S, Troisi A (2005) PPN-limit of fourth order gravity inspired by scalar-tensor gravity. Phys Rev D 72:044022
• Capozziello S, Vignolo S (2009) The cauchy problem for metric-affine f(r)-gravity in the presence of perfect-fluid matter. Class Quantum Grav 26(17):175013
• Capozziello S, Corda C, De Laurentis M (2007) Stochastic background of relic scalar gravitational waves from scalar-tensor gravity. Mod Phys Lett A 22:2647–2655
• Chandrasekhar S (1985) The mathematical theory of black holes. Springer
• Coleman Miller M (2016) Implications of the gravitational wave event GW150914. Gen Rel Grav 48(7):95
• Damour T, Esposito-Farèse G (1998) Gravitational-wave versus binary-pulsar tests of strong-field gravity. Phys Rev D 58(4):042001
• de Felice A, Tsujikawa S (2010) f(R) theories. Living Rev Relativ 13:3
• De Laurentis M, Capozziello S (2011) Quadrupolar gravitational radiation as a test-bed for f(r)-gravity. Astropart Phys 35(5):257–265
• De Laurentis M, De Martino I (2013) Testing f (R) theories using the first time derivative of the orbital period of the binary pulsars. Mon Not R Astron Soc 431(1):741–748
• de Laurentis M, de Martino I (2015) Probing the physical and mathematical structure of f(R)-gravity by PSR J0348 + 0432. Int J Geom Meth Mod Phys 12(4):1550040
• De Laurentis M, De Martino I, Lazkoz R (2018) Analysis of the Yukawa gravitational potential in f (R ) gravity. II. Relativistic periastron advance. Phys Rev D 97(10):104068
• De Laurentis M, De Martino I, Lazkoz R Modified gravity revealed along geodesic tracks. Eur Phys J C 78(11):916 (2018)
• De Laurentis M, Capozziello S (2009) Stochastic background of relic scalar gravitational waves tuned by extended gravity. Nucl Phys B Proc Suppl 194:212–217 New Horizons for Modern Cosmology
• De Laurentis M, Porth O, Bovard L, Ahmedov B, Abdujabbarov A (2016) Constraining alternative theories of gravity using GW150914 and GW151226. Phys Rev D 94(12):124038
• Dvali G, Gabadadze G, Porrati M (2000) 4d gravity on a brane in 5d Minkowski space. Phys Lett B 485(1–3):208–214
• Eardley DM, Lee DL, Lightman AP (1973) Gravitational-wave observations as a tool for testing relativistic gravity. Phys Rev D 8:3308–3321
• Eardley DM, Lee DL, Lightman AP, Wagoner RV, Will CM (1973) Gravitational-wave observations as a tool for testing relativistic gravity. Phys Rev Lett 30:884–886
• Eddington AS (1924) The mathematical theory of relativity. Cambridge University Press, London
• Faraoni V (2005) Phantom cosmology with general potentials. Class Quantum Grav 22(16):3235–3246
• Feng JL (2010) Dark matter candidates from particle physics and methods of detection. Annu Rev Astron Astrophys 48:495–545
• Fierz M (1956) On the physical interpretation of P.Jordan’s extended theory of gravitation. Helv Phys Acta 29:128–134
• Finn LS, Sutton PJ (1993) Observing binary inspiral in gravitational radiation: one interferometer. Phys Rev D 47:2198–2219
• Hinterbichler K, Khoury J (2010) Screening long-range forces through local symmetry restoration. Phys Rev Lett 104:231301
• Hu W, Sawicki I (2007) Models of f(r) cosmic acceleration that evade solar system tests. Phys Rev D 76:064004
• Hulse RA, Taylor JH (1975) Discovery of a pulsar in a binary system. Astrophys J Lett 195:L51–L53
• Husa S, Khan S, Hannam M, Pürrer M, Ohme F, Jiménez Forteza X, Bohé A (2016) Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. New numerical waveforms and anatomy of the signal. Phys Rev D 93(4):044006
• Isaacson RA (1968) Gravitational radiation in the limit of high frequency. I. The linear approximation and geometrical optics. Phys Rev 166:1263–1271
• Isaacson RA (1968) Gravitational radiation in the limit of high frequency. II. Nonlinear terms and the effective stress tensor. Phys Rev 166:1272–1279
• Jacobson T (2007) Einstein-aether gravity: a Status report. PoS QG-PH:020
• Jacobson T, Mattingly D (2001) Gravity with a dynamical preferred frame. Phys Rev D 64:024028
• Jordan P (1955) Schwerkraft und Weltall. Friedrich Vieweg and Sohn, Braunschweig
• Kahya EO, Desai S (2016) Constraints on frequency-dependent violations of Shapiro delay from GW150914. Phys Lett B 756:265–267
• Kahya EO, Desai S (2016) Constraints on frequency-dependent violations of Shapiro delay from GW150914. Phys Lett B 756:265–267
• Khoury J, Weltman A (2004) Chameleon fields: awaiting surprises for tests of gravity in space. Phys Rev Lett 93:171104
• Khoury J, Wyman M (2009) N-body simulations of dgp and degravitation theories. Phys Rev D 80(6):64023
• Kopeikin SM (1996) Proper motion of binary pulsars as a source of secular variations of orbital parameters. Astrophys J Lett 467:L93
• Landau LD, Lifshitz EM (1962) The classical theory of fields. Addison-Wesley Publication Co., Inc., Reading
• Li B, Barrow JD (2007) Cosmology of f(r) gravity in the metric variational approach. Phys Rev D 75:084010
• Li TGF, Del Pozzo W, Vitale S, Van Den Broeck C, Agathos M, Veitch J, Grover K, Sidery T, Sturani R, Vecchio A (2012) Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence. Phys Rev D 85:082003
• Maggiore M (2007) Gravitational waves: theory and experiments. Oxford University Press
• Miranda V, Jorás SE, Waga I, Quartin M (2009) Viable singularity-free f(r) gravity without a cosmological constant. Phys Rev Lett 102:221101
• Mirshekari S, Will CM (2013) Compact binary systems in scalar-tensor gravity: equations of motion to 2.5 post-Newtonian order. Phys Rev D 87(8):084070
• Mishra CK, Arun KG, Iyer BR, Sathyaprakash BS (2010) Parametrized tests of post-Newtonian theory using advanced LIGO and Einstein telescope. Phys Rev D 82:064010
• Nicolis A, Rattazzi R, Trincherini E (2009) Galileon as a local modification of gravity. Phys Rev D 79:064036
• Noether E (1971) Invariant variation problems. Transp Theory Stat Phys 1(3):186–207
• Nojiri S, Odintsov SD, Tsujikawa S (2005) Properties of singularities in the (phantom) dark energy universe. Phys Rev D 71(6):063004
• Weyl H, Pauli W (1919) Zur Theorie der Gravitation und der Elektrizität. Phys Z 20:457–467
• Poisson E, Will CM (2014) Gravity: Newtonian, Post-Newtonian, relativistic. Cambridge University Press
• Primack JR (2012) Triumphs and tribulations of ΛCDM, the double dark theory. Ann Phys 524(9–10):535–544
• Rubano C, Scudellaro P (2005) Variable G and Λ: scalar-tensor versus RG-improved cosmology. Gen Relativ Gravit 37(3):521–539
• Saffer A, Yunes N, Yagi K (2018) The gravitational wave stress–energy (pseudo)-tensor in modified gravity. Class Quant Grav 35(5):055011
• Shklovskii IS (1970) Possible causes of the secular increase in pulsar periods. Sov Astron 13:562
• Sotiriou TP (2006) f(R) gravity and scalar-tensor theory. Class Quant Grav 23:5117–5128
• Sotiriou TP, Faraoni V (2010) f(R) theories of gravity. Rev Mod Phys 82:451–497
• Stairs IH (2004) Pulsars in binary systems: probing binary stellar evolution and general relativity. Science 304(5670):547–552
• Stairs IH (2003) Testing general relativity with pulsar timing. Living Rev Relativ 6(1):1–49
• Starobinsky AA (1980) A new type of isotropic cosmological models without singularity. Phys Lett B 91:99
• Starobinsky AA (2007) Disappearing cosmological constant in f(r) gravity. JETP Lett 86:157
• Uzan J-P (2003) The fundamental constants and their variation: observational and theoretical status. Rev Mod Phys 75:403–455
• van Dam H, Veltman MJG (1970) Massive and massless Yang-Mills and gravitational fields. Nucl Phys B 22:397–411
• Wagoner RV (1970) Scalar tensor theory and gravitational waves. Phys Rev D 1:3209–3216
• Wei J-J, Gao H, Wu X-F, Mészáros P (2015) Testing Einstein’s equivalence principle with fast radio bursts. Phys Rev Lett 115(26):261101
• Weinberg S (1972) Gravitation and cosmology. Wiley, New York
• Weisberg JM, Huang Y (2016) Relativistic measurements from timing the binary pulsar PSR B1913+16. Astrophys J 829(1):55
• Weisberg JM, Nice DJ, Taylor JH (2010) Timing measurements of the relativistic binary pulsar psr b1913+16. Astrophys J 722(2):1030–1034
• Weisberg JM, Taylor JH (2002) Radio pulsars. M. Bailes
• Weyl H (1918) Math Zeit 2:384, https://doi.org/10.1007/BF01199420
• Will CM (2018) Theory and experiment in gravitational physics, 2 edn. Cambridge University Press
• Wu X-F, Gao H, Wei J-J, Mészáros P, Zhang B, Dai Z-G, Zhang S-N, Zhu Z-H (2016) Testing Einstein’s weak equivalence principle with gravitational waves. Phys Rev D 94:024061
• Yunes N, Pretorius F (2009) Fundamental theoretical bias in gravitational wave astrophysics and the parameterized post-Einsteinian framework. Phys Rev D 80:122003