Remnants and thermal corrections in Horndeski black holes with non-minimal kinetic coupling
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy,Fluid Flow and Transfer Processes
Link
https://link.springer.com/content/pdf/10.1140/epjp/s13360-022-03036-4.pdf
Reference89 articles.
1. G.W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space. Int. J. Theor. Phys. 10, 363 (1974)
2. R.P. Woodard, Scholarpedia 10, 32243 (2015). http://arxiv.org/abs/1506.02210 [hep-th]
3. E.N. Saridakis, S.V. Sushkov, Quintessence and phantom cosmology with non-minimal derivative coupling. Phys. Rev. D 81, 083510 (2010). [http://arxiv.org/abs/1002.3478 [gr-qc]]
4. C. Charmousis, E.J. Copeland, A. Padilla, and P.M. Saffin, General second-order scalar-tensor theory and self-tuning, Phys. Rev. Lett. 108, 051101 (2012). [http://arxiv.org/abs/1106.2000 [hepth]]
5. A. Maselli, H.O. Silva, M. Minamitsuji, E. Berti, Neutron stars in Horndeski gravity. Phys. Rev. D 93, 124056 (2016)
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