Effective theory for binary stars and its application to gravitational waves

Authors

  • Anthonny Freddy Canazas Garay Facultad de Ciencias, Universidad Nacional de Ingeniería, Lima-Perú

DOI:

https://doi.org/10.21754/tecnia.v25i2.51

Keywords:

Gravitational waves, Effective field theory, General relativity, Astrophysics, Black hole., Neutron star

Abstract

The recent detections of gravitational waves have brought renewed attention to the problem of obtaining high accuracy predictions for the gravitational radiation spectra emitted by binary systems with black holes or neutron stars constituents. This work explains how effective field theory applied to gravitation can be used to describe a gravitationally interacting extended object as in the binary system case. Gravitational wave emission from the binary system is shown by using methods that are usually applied in quantum field theory.

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References

[1] http://www.ictp-saifr.org/?page_id=9163

[2] Porto, R. A.,“The effective field theorist’s approach to gravitational dynamics”, Phys.Rept. 633 (2016) 1-104.

[3] Abbott, B. P.et al.“Observation of gravitational waves from a binary black hole merger”,Phys.Rev.Lett. 116 (2016) no.6, 061102.

[4] Abbott, B. P. et al.“GW151226: Observation of gravitational waves from a 22-solar-mass binary black hole coalescence”, Phys.Rev.Lett. 116 (2016) no.24, 241103.

[5] Chakrabarti, S., Delsate, Tr., Steinhoff, J.,“New perspectives on neutron star and black hole spectroscopy and dynamic tides”, arXiv:1304.2228 [gr-qc]

[6] Porto, R. A., Ross, A., Rothstein, I. Z., “Spin induced multipole moments for the gravitationalwaveamplitude frombinaryinspirals to 2.5 Post-Newtonian order”, JCAP 1209 (2012) 028.

Published

2015-12-01

How to Cite

[1]
A. F. Canazas Garay, “Effective theory for binary stars and its application to gravitational waves”, TECNIA, vol. 25, no. 2, pp. 75–83, Dec. 2015.

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Section

Articles