Holography, Charge, and Baryon Asymmetry

T. R. Mongan

84 Marin Avenue, Sausalito, CA 94965 USA.

DOI: 10.4236/jmp.2012.37079                

Abstract

The reason for baryon asymmetry in our universe has been an open question for many years. This note shows that the holographic principle requires a charged preon model underlying the Standard Model of particle physics and, in consequence, requires baryon asymmetry. The baryon asymmetry predicted by a specific charged preon model in our closed inflationary Friedmann universe is consistent with observations.

Keywords

Baryon Asymmetry; Charged Preon Models; Holographic Principle

Conflicts of Interest

The authors declare no conflicts of interest.

References

[1]	M. Dine and A. Kusenko, “The Origin of the Matter-Antimatter Asymmetry,” Reviews of Modern Physics, Vol. 76, No. 1, 2004.
[2]	R. Bousso, “The Holographic Principle,” Reviews of Modern Physics, Vol. 74, No. 3, 2002, pp. 825-874. doi:10.1103/RevModPhys.74.825
[3]	T. Padmanabhan, “A Physical Interpretation of Gravitational Field Equations,” arXiv:0911.1403.
[4]	T. Padmanabhan, “A Dialogue on the Nature of Gravity,” arXiv:0910.0839.
[5]	R. Easther and D. Lowe, “Holography, Cosmology and the Second Law of Thermodynamics,” Physical Review Letters, Vol. 82, No. 25, 1999, pp. 4967-4970. doi:10.1103/PhysRevLett.82.4967
[6]	D. Bak and S. Rey, “Cosmic Holography,” Classical and Quantum Gravity, Vol. 17, No. 15, 2000, L83. doi:10.1088/0264-9381/17/15/101
[7]	N. Kaloper and A. Linde, “Cosmology vs. Holography,” Physical Review, Vol. 60, No. 10, 1999, p. 103509. doi:10.1103/PhysRevD.60.103509 T. Mongan, “A Simple Quantum Cosmology,” General Relativity and Gravitation, Vol. 33, No. 8, 2001, pp. 1415-1424. doi:10.1023/A:1012065826750
[8]	D. Boyanovksy, H. de Vega and R. Holman, “Non- Equilibrium Phase Transitions in Condensed Matter and Cosmology: Spinodal Decomposition, Condensates and Defects,” Lectures at NATO Advanced Study Institute: Topological Defects and the Non-Equilibrium Dynamics of Symmetry Breaking Phase Transitions, [hep-ph/ 9903534].
[9]	S. Dodelson, “Modern Cosmology,” Academic Press, San Diego, 2003.
[10]	A. Siemiginowska, et al, “The 300 kpc Long X-Ray Jet in PKS 1127-145, z = 1.18 Quasar: Constraining X-Ray Emission Models,” Astrophysical Journal, Vol. 657, No. 1, 2007, p. 145. doi:10.1086/510898
[11]	J. Islam, “An Introduction to Mathematical Cosmology,” 2nd Edition, Cambridge University Press, Cambridge, 2002.
[12]	C. Bennet, et al, “First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results,” Astrophysical Journal, Suppl. 1, 2003, p. 175 [astro-ph/0302207].
[13]	T. Mongan, “A Holographic Charged Preon Model,” arXiv:0801.3670.
[14]	A. Adriani, et al., “Observation of an Anomalous Positron Abundance in the Cosmic Radiation,” Nature, Vol. 458, 2009, pp. 607-609. doi:10.1038/nature07942
[15]	P. Serpico, “Possible Causes of a Rise with Energy of the Cosmic Ray Positron Fraction,” Physical Review, Vol. 79, No. 2, 2009, p. 021302. doi:10.1103/PhysRevD.79.021302
[16]	P. Jean, et al., “Early SPI/INTEGRAL Measurements of Galactic 511 keV Line Emission from Positron Annihilation,” Astronomy & Astrophysics, Vol. 407, 2003, L55. doi:10.1051/0004-6361:20031056