Abstract
Physics has known about and dealt with wave phenomena for a long time. In fact, Physics courses feature a variety of treatments of waves in fluids, electromagnetic waves, and related subjects. On very general grounds we may define a “wave” as a solution of a wave equation. This is not a mere tautology, but an accurate statement that includes many possibilities related to the Physics of wave phenomena. More specifically, a wave equation may contain a variety of terms, but two mandatory ingredients are the second time derivative and the second spatial derivative of some dynamical variable to be determined. Gravitational waves are a true revolution in the understanding of compact objects and gravity itself, a frontier opened a few years ago of high importance in the field.
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References
A. Pais, Subtle Is the Lord: The Science and the Life of Albert Einstein (Oxford University Press, Oxford, 2005)
R. Matzner, Introduction to Gravitational Waves (Springer, Dordrecht, Netherlands, 2010)
K. Thorne, Gravitational-wave research: Current status and future prospects. Rev. Mod. Phys. 52, 285 (1980)
J.M. Weisberg and J.H. Taylor, The relativistic binary pulsar B1913+16: Thirty years of observations and analysis, in Binary Radio Pulsars, ASP Conference Series 328, eds. F.A. Rasio and I.H. Stairs (2005), p. 25
J.A. Batlle, R. Lopez, Revisiting the border between Newtonian mechanics and General Relativity: The periastron advance. Contrib. Sci. 10, 65–72 (2014)
M. Burgay et al., An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system. Nature 426, 531 (2003)
J. Weber, Evidence for discovery of gravitational radiation. Phys. Rev. Lett. 22, 1320 (1969)
P.R. Saulson, Interferometric gravitational wave detectors. Int. J. Mod. Phys. D 27, 1840001 (2018)
B.P. Abbott at el., Prospects for observing and localizing gravitational-wave transients with Advanced LIGO and Advanced Virgo. Living Rev. Relati. 19, 1 (2016)
A. Blaut, Parameter estimation accuracies of Galactic binaries with ELISA. Astropart. Phys. 101, 17 (2018)
C.J. Moore, R.H. Cole, C.P.L. Berry, Gravitational-wave sensitivity curves. Class. Quant. Grav. 32, 015014 (2015)
B.P. Abbott et al., Observation of gravitational waves from a binary black hole merger. Phys. Rev. Lett. 116, 061102 (2016)
B.P. Abbott et al., GW170817: Observation of gravitational waves from a binary neutron star inspiral. Phys. Rev. Lett. 119, 161101 (2017)
J.E. Horvath, The binaries of the NS–NS merging events, in Proceedings of the Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy, AIP Conf. Proc.2127 (2019), p. 020015
R.D. Ferdman et al., Asymmetric mass ratios for bright double neutron-star mergers. Nature 583, 211 (2020)
B.P. Abbott et al., Gravitational waves and gamma-rays from a binary neutron star merger: GW170817 and GRB 170817A. Astrophys. J. Lett. 848, L13 (2017)
S. Covino et al., The unpolarized macronova associated with the gravitational wave event GW 170817. Nature Astron. 1, 791 (2017)
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Horvath, J.E. (2022). Gravitational Waves. In: High-Energy Astrophysics. Undergraduate Lecture Notes in Physics. Springer, Cham. https://doi.org/10.1007/978-3-030-92159-0_10
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DOI: https://doi.org/10.1007/978-3-030-92159-0_10
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