107 reads
Non-singular Oscillating Cosmology on Randall-Sundrum II: References
by Cosmological thinking: time, space and universal causation May 26th, 2024
Too Long; Didn't Read
In this paper, researchers propose a non-singular cosmology model on Randall-Sundrum II brane, featuring oscillations and phantom dark energy.
This paper is available on arxiv under CC 4.0 license.
Authors:
(1) Rikpratik Sengupta, Department of Physics, Aliah University, Kolkata 700 160, West Bengal, India (E-mail addresses: [email protected](RS))
Table of Links
References
[1] Knop, R.A., et al. Astrophys.J. 598 102 (2003)
[2] Spergel, D.N., et al, Astrophys.J.Suppl. 148 175 (2003) [3] Tegmark, M. et al, Phys. Rev. D 69 103501 (2004)
[4] S. W. Hawking, Phys. Rev. Lett. 17 443 (1966).
[5] S. W. Hawking and R. Penrose, Proc. Roy. Soc. London A314 529 (1970).
[6] A. Borde, A. H Guth and A. Vilenkin, Phys. Rev. Lett. 90 151301 (2003).
[7] J. Polchinski, String Theory, Vol. 2, Superstring Theory and Beyond (Cambridge University Press, 1998).
[8] R. Gambini and J. Pullin, A First Course in Loop Quantum Gravity (Oxford University Press, 2011)
[9] L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690 (1999).
10] Y. Shtanov and V. Sahni, Phys. Lett. B 557, 1 (2003)
[11] A. Ashtekar, T. Pawlowski and P. Singh, Phys. Rev. D 74, 084003 (2006).
[12] P. Singh, Class. Quantum Grav. 26 125005 (2009).
[13] G. Efstathiou and S. Gratton, MNRAS Lett. 496 (2020) L91.
[14] S. Vagnozzi et al., Phys. Dark Univ. 33 (2021) 100851.
[15] S. Vagnozzi, A. Loeb and M. Moresco, Astrophys. J. 908 (2021) 84.
[16] S. Dhawan, J. Alsing and S. Vagnozzi, Mon. Not. Roy. Astron. Soc. 506 (2021) L1.
[17] R. Sengupta et al., Class. Quant. Grav. 39 105004.
[18] G F. R. Ellis, J. Murugan and C. G. Tsagas, Class. Quant. Grav. 21 (2004) 223.
[19] S. J. Perlmutter et al., Nature 391 51 (1998).
[20] Riess, A.G. et al., Astron. J. 116 1009 (1998).
[21] Zlatev, I., Wang, L. and Steinhardt, P.J., Phys. Rev. Lett. 82 896 (1999).
[22] Ure˜na-L´opez, L.A. and Liddle, A., Phys. Rev. D 66 083005 (2002).
[23] Kamenshchik, A., Moschella, U. and Pasquier, V., Phys. Lett. B 511 265 (2001)
[24] U. Debnath, A. Banerjee, and S. Chakraborty, Class. Quant. Grav. 21 (2004) 5609.
[25] Caldwell, R.R., Phys. Lett. B 545, 23 (2002)
[26] Frampton, P. and Takahashi, T., Phys. Lett. B 557 135 (2003).
[27] G. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 485 208 (2000)
[28] C. Deffayet, G. Dvali, and G. Gabadadze, Phys. Rev. D 65 (2002) 044023.
[29] S. Nojiri and S. D. Odintsov, Int. J. Geom. Methods Mod. Phys., 4 (2007) 115.
[30] J. M. Cline, S. Jeon and G. D. Moore, Phys. Rev. D70, 043543 (2004)
[31] L. Parker and A. Raval, Phys. Rev. Lett. 86, 749 (2001). [32] R. Caldwell, M. Kamionkowski and N. Weinberg, Phys. Rev. Lett. 91 071301 (2003).
[33] P. Davies, Annales Poincare Phys. Theor. 49 297 (1988).
[34] R. Sengupta et al., Phys. Rev. D 102 (2020) 024037.
[35] L. Visinelli, N. Bolis, and S. Vagnozzi, Phys. Rev. D 97, 064039 (2018).
[36] S. Vagnozzi and L. Visinelli, Phys. Rev. D 100, 024020 (2019).
[37] I. Banerjee, T. Paul and S. Sengupta, JCAP 02, 041 (2021).
L O A D I N G
. . . comments & more!
. . . comments & more!
