Cosmological implications of the tetron model of elementary particles

• Autorzy: Bodo Lampe
• Języki publikacji: EN

Abstrakty

EN

Based on a possible solution to the tetron spin problem, a modification of the standard Big Bang scenario is suggested, where the advent of a space-time manifold is connected to the appearance of tetronic bound states. The metric tensor is constructed from tetron constituents and the reason for cosmic inflation is elucidated. Furthermore, there are natural dark matter candidates in the tetron model. The ratio of ordinary to dark matter in the universe is calculated to be 1:5.

Słowa kluczowe

EN

dark matter; tetron model; elementary particles

• Czasopismo: Open Physics
• Rocznik: 2010
• Tom: 8
• Numer: 5
• Strony: 771-781

Daty

wydano

2010-10-01

online

2010-07-22

Twórcy

autor

Bodo Lampe,

Bibliografia

• [1] R. N. Mohapatra, J. C. Pati, Phys. Rev. D 11, 566 (1975) http://dx.doi.org/10.1103/PhysRevD.11.566[Crossref]
• [2] B. Lampe, Found. Phys. 39, 215 (2009) http://dx.doi.org/10.1007/s10701-009-9278-9[Crossref]
• [3] B. Lampe, J. Phys. G 34, (2007) 1 http://dx.doi.org/10.1088/0954-3899/34/9/006[Crossref]
• [4] B. Lampe, Mod. Phys. Lett. A 23, 2835 (2008) http://dx.doi.org/10.1142/S0217732308028284[Crossref]
• [5] A. H. Guth, Phys. Rev. D 23, 347 (1981) http://dx.doi.org/10.1103/PhysRevD.23.347[Crossref]
• [6] K. Freeman, G. McNamara, In Search of Dark Matter (Birkhäuser, 2006)
• [7] S. Nesseris, L. Perivolaropoulos, Phys. Rev. D 70, 043531 (2004) http://dx.doi.org/10.1103/PhysRevD.70.043531[Crossref]
• [8] J. M. Cline, J. Vinet, Phys. Rev. D68, 025015 (2003) http://dx.doi.org/10.1103/PhysRevD.68.025015[Crossref]
• [9] P. J. E. Peebles, B. Ratra, Rev. Mod. Phys. 75, 559 (2003) http://dx.doi.org/10.1103/RevModPhys.75.559[Crossref]
• [10] C. Wetterich, arXiv:astro-ph/0110211v1
• [11] E. Seiler, A. Patrascioiu, Phys. Rev. D 64, 065006 (2001) http://dx.doi.org/10.1103/PhysRevD.64.065006[Crossref]
• [12] P. Hasenfratz, F. Niedermayer, Nucl. Phys. B 596, 481 (2001) http://dx.doi.org/10.1016/S0550-3213(00)00696-9[Crossref]
• [13] R. C. Johnson, Phys. Lett. 114 B, 147 (1982)
• [14] J. Conway, D. Smith, On Octonions and Quaternions (Peters Publishing, Natick, MA,2003)
• [15] I. L. Kantor, A. S. Solodovnikov, Hypercomplex Numbers - an Elementary Introduction to Algebras (Springer-Verlag, Berlin, 1989)
• [16] R. D. Schafer, An Introduction to Nonassociative Algebras (Academic Press, New York and London, 1966)
• [17] G. M. Dixon, arXiv:hep-th/9504040v1
• [18] E. Magliaroac, C. Perinibc, C. Rovelli, arXiv:0704.0992v2 [WoS]
• [19] J. D. Bekenstein, Phys. Rev. D 70, 083509 (2004) http://dx.doi.org/10.1103/PhysRevD.70.083509[Crossref]
• [20] E. Cartan, Ann. Sci. Ecole Norm. S. 41, 1 (1924)
• [21] J. S. Griffith, Irreducible Tensor Methods for Molecular Symmetry Groups (Dover Publications, 2006)
• [22] G. R. Farrar, P. J. Peebles, arXiv:astro-ph/0307316
• [23] G. W. Anderson, S. M. Carroll, arXiv:astro-ph/9711288
• [24] B. A. Bassett, S. Tsujikawa, D. Wands, arXiv:astro-ph/0507632v2
• [25] A. O. Barvinsky, A. Yu. Kamenshchik, A. A. Starobinsky, J. Cosmol. Astropart. P. 11, 21 (2008) http://dx.doi.org/10.1088/1475-7516/2008/11/021[Crossref]
• [26] F. Bezrukov, M. Shaposhnikov, arXiv:hep-th/0710.3755v2
• [27] S. Weinberg, E. Witten, Phys. Lett. B 96, 59 (1980) http://dx.doi.org/10.1016/0370-2693(80)90212-9[Crossref]
• [28] A. A. Belavin, A. M. Polyakov, A. B. Zamolodchikov, Nucl. Phys. B 241, 333 (1984) http://dx.doi.org/10.1016/0550-3213(84)90052-X[Crossref]

Identyfikatory

DOI

10.2478/s11534-010-0002-3