A Cosmological Model without Singularity Based on RW Metric (1) ()

Shihao Chen

Yue-Hong Institute for Advanced Study, Yunnan University, Kunming, China.

**DOI: **10.4236/ijaa.2014.41023
PDF HTML XML
4,069
Downloads
5,577
Views
Citations

Yue-Hong Institute for Advanced Study, Yunnan University, Kunming, China.

A new conjecture is proposed that there are two sorts of matter called s-matter and v-matter which are symmetric, whose masses are positive, but whose gravitational masses are opposite to each other. Based on the conjecture and the *SU _{S}*(5) ×

Share and Cite:

Chen, S. (2014) A Cosmological Model without Singularity Based on RW Metric (1). *International Journal of Astronomy and Astrophysics*, **4**, 264-293. doi: 10.4236/ijaa.2014.41023.

Conflicts of Interest

The authors declare no conflicts of interest.

[1] | Hawking, S.W. and Ellis, G.F.R. (1999) The Large Scale Structure of Space-Time, Cambridge University Press, 7, 98, 101, 137, 256-298. |

[2] | Brandenberger, R., Mukhanov, V. and Sornborger, A. (1993) Cosmological Theory without Singularities. Physical Review D, 48, 1629-1642. http://dx.doi.org/10.1103/PhysRevD.48.1629 |

[3] | Frolov, V.P, Markov M.A. and Mukhanov V.F. (1990) Black Holes as Possible Sources of Closed and Semiclosed Worlds. Physical Review D, 41, 383-394. http://dx.doi.org/10.1103/PhysRevD.41.383 |

[4] | Caldwell, R.R. (2004) Dark Energy. Physics World, 17, 37-42. |

[5] | Padmanabhan, T. (2003) Cosmological Constant—The Weight of the Vacuum. Physics Reports, 380, 235-320. http://dx.doi.org/10.1016/S0370-1573(03)00120-0 |

[6] | Peebles P.J.E. and Ratra, B. (2003) The Cosmological Constant and Dark Energy. Reviews of Modern Physics, 75, 559. http://dx.doi.org/10.1103/RevModPhys.75.559 |

[7] | Weinberg, S. (1987) Anthropic Bound on the Cosmological Constant. Physical Review Letters, 59, 2607-2610. http://dx.doi.org/10.1103/PhysRevLett.59.2607 |

[8] | Martel, H., Shapiro, P.R. and Weinberg, S. (1998) Likely Values of the Cosmological Constant. The Astrophysical Journal, 492, 29-40. http://dx.doi.org/10.1086/305016 |

[9] | Peebles, P.J.E. and Ratra, B. (1988) Cosmology with a Time-Variable Cosmological “Constant”. The Astrophysical Journal, 325, L17-L20. http://dx.doi.org/10.1086/185100 |

[10] | Ratra, B. and Peebles, P.J.E. (1988) Cosmological Consequences of a Rolling Homogeneous Scalar Field. Physical Review D, 37, 3406; http://dx.doi.org/10.1103/PhysRevD.37.3406 |

[11] | Peebles, P.J.E. and Ratra, B. (2003) The Cosmological Constant and Dark Energy. Reviews of Modern Physics, 75, 559. http://dx.doi.org/10.1103/RevModPhys.75.559 |

[12] | Hall, L.J. Nomura Y. and Oliver, S.J., (2005) Evolving Dark Energy with w≠-1. Physical Review Letters, 95, 14. http://dx.doi.org/10.1103/PhysRevLett.95.141302 |

[13] | Chen, S.H. (2002) Quantum Field Theory without Divergence A. arXiv: hep-th/0203220. |

[14] | Chen, S.H. (2002) Significance of Negative Energy State in Quantum Field Theory A. arXiv: hep-th/0203230. |

[15] | Chen, S.H. (2005) Quantum Field Theory without Divergence. In: Kovras, O., Ed., Quantum Field Theory: New Research, Nova Science Publishers, Hauppauge, 103-170. |

[16] | Chen, S.H. (2001) A Possible Candidate for Dark Matter. arXiv: hep-th/0103234. |

[17] | Chen, S.H. (2005) A Possible Candidate for Dark Matter. In: Val Blain, J., Progress in Dark Matter Research, Nova Science Publishers, Hauppauge, 65-72. |

[18] | Peacock, J.A. (1999) Cosmological Physics. Cambridge University Press, 78, 89, 90, 296, 458, 460-464, 579, 664. |

[19] | Chen, S.-H. (2009) Discussion of a Possible Universal Model without Singularity. arXiv: 0908.1495v2. |

[20] | Chen, S.-H. (2006) A Possible Universal Model without Singularity and its Explanation for Evolution of the Universe. High Energy Physics—Phenomenology, arXiv:hep-ph/0611283. |

[21] | Gibbons, G.W. and Hawking, S.W. (1977) Action Integrals and Partition Functions in Quantum Gravity. Physical Review D, 15, 2752. http://dx.doi.org/10.1103/PhysRevD.15.2752 |

[22] | Chaichian, M. and Nelipa, N.F. (1984) Introduction to Gauge Field Theories. Springer-Verlag, Berlin, Heidelberg, 269. |

[23] | Ross, G.G. (1984) Grand Unified Theories. Benjamin/Cummings Publishing Company, Inc., 177-183. |

[24] | Weinberg, S. (1972) Gravitation and Cosmology. Wiley, New York, Chapter 12, Section 3. |

[25] | Coleman, S. and Weiberg, E.J. (1973) Radiative Corrections as the Origin of Spontaneous Symmetry Breaking. Physical Review D, 7, 1888-1910. http://dx.doi.org/10.1103/PhysRevD.7.1888 |

[26] | Brandenberg, R.H. (1985) Quantum Field Theory Methods and Inflationary Universe Models. Reviews of Modern Physics, 57, 1-60. http://dx.doi.org/10.1103/RevModPhys.57.1 |

[27] | Liu, L., Jiang, Y. and Qian, Z. (1989) The Inflationary Universe Scenario in 10?35 Sec after Big-Bang. Progress in Physics, 9, 121-187. (in Chinese) |

[28] | Guth, A.H. (1981) Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems. Physical Review D, 23, 347-356. http://dx.doi.org/10.1103/PhysRevD.23.347.53 |

Journals Menu

Contact us

customer@scirp.org | |

+86 18163351462(WhatsApp) | |

1655362766 | |

Paper Publishing WeChat |

Copyright © 2023 by authors and Scientific Research Publishing Inc.

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.