Abstract
In this short comment, we notice that the model-independent axion contribution to the graviton mass at just outside the Schwarzschild radius is completely negligible in GW150914. The modelindependent axion contribution to the graviton mass at the order 10−22 eV might be possible for merger of black holes of mass of order 2 × 1014 kg.
References
B. P. Abbott et al.. (LIGO Scientific Collaboration and Virgo Collaboration), Phys. Rev. Lett. 116, 061102 (2016) [arXiv:1602.03837].
B. P. Abbott et al.. (LIGO Scientific Collaboration and Virgo Collaboration), Phys. Rev. Lett. 116, 221101 (2016) [arXiv:1602.03841].
M. Fierz and W. Pauli, Proc. Roy. Soc. Lond. A173 (1939), p. 211 [doi:10.1098/rspa.1939.0140].
H. van Dam and M. J. G. Veltman, Nucl. Phys. B 22, 397 (1970) [doi:10.1016/0550-3213(70)90416-5].
A. I. Vainshtein, Phys. Lett. B 39, 393 (1972) [doi:10.1016/0370-2693(72)90147-5].
M. B. Green and J. Schwarz, Phys. Lett. B 149, 117 (1984) [doi: 10.1016/0370-2693(84)91565-X].
E. Witten, Phys. Lett. B 149, 351 (1984) [doi: 10.1016/0370-2693(84)90422-2].
K. Choi and J. E. Kim, Phys. Lett. B 154, 393 (1985) [doi: 10.1016/0370-2693(85)90416-2].
For a recent figure, see, J. E. Kim, Phys. Lett. B 759, 58 (2016) [arXiv:1604.00716 [hep-ph]].
J. E. Kim, Phys. Rep. 150, 1 (1987) [doi:10.1016/0370- 1573(87)90017-2].
B. J. Carr, K. Kohri, Y. Sendouda and J. Yokoyama, Phys. Rev. D 81, 104019 (2010) [arXiv:0912.5297 [astroph. CO]].
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Kim, J.E. Gravity wave and model-independent axion. Journal of the Korean Physical Society 71, 127–129 (2017). https://doi.org/10.3938/jkps.71.127
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.3938/jkps.71.127