On inflation and variation of the strong coupling constant

Variation of constants in the very early universe can generate inflation. We consider a scenario where the strong coupling constant was changing in time and where the gluon condensate underwent a phase transition ending the inflation. © World Scientific Publishing Company.

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Detalles Bibliográficos
Autor principal: Chamoun, N.
Otros Autores: Landau, S.J, Vucetich, H.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2007
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
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100 1 |a Chamoun, N. 
245 1 3 |a On inflation and variation of the strong coupling constant 
260 |c 2007 
270 1 0 |m Chamoun, N.; Departamento de Física, Universidad Nacional de la Plata, c.c. 67, 1900 La Plata, Argentina 
506 |2 openaire  |e Política editorial 
504 |a Guth, A.H., (1981) Phys. Rev. D, 23 (2), p. 347 
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504 |a Moffat, J., (1993) Founda. Phys, 23, p. 411 
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504 |a Khoury, J., Ovrut, B., Seiberg, N., Steindhardt, P., Turok, N., (2002) Phys. Rev. D, 65, p. 086007 
504 |a Khoury, J., Ovrut, B., Steindhardt, P., Turok, N., (2001) Phys. Rev. D, 64, p. 123522 
504 |a Vanchurin, V., Vilenkin, A., (2000) Phys. Rev. D, 61, p. 083507 
504 |a Chamoun, N., Landau, S., Vucetich, H., (2001) Phys. Lett. B, 504 (1). , astro-ph/0008436 
504 |a de Bernardis, P., (2000) Nature, 404, p. 995 
504 |a Hanany, S., (2000) Astrophys. J, 545, pp. L5 
504 |a Peiris, H.V., First year Wilkinson microwave anisotropy probe (WMAP) observations: Implications for inflation (2003) Astrophys. J. Suppl, 148, p. 213. , astro-ph/0302225 
504 |a Spergel, D., Wilkinson microwave anisotropy probe (WMAP) three year results: Implications for cosmology astro-ph/0603449; Greiner, W., Schafer, A., (1995) Quantum Chromodynamics, , 2nd Edn, Springer 
504 |a Guth, A.H., (1999) Proc. Cosmic Questions 1999, , The New York Academy of Sciences Press, astro-ph/0101507 
504 |a Hawking, S., (1982) Phys. Lett. B, 115 (4), p. 295 
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504 |a Brandenberger, R., (1997) ICTP 1997 Summer School in High Energy Physics and Cosmology, , eds. E. Gava et al, World Scientific 
504 |a Brandenberger, R., (1994) Invited Lectures at TASI-94, , Colorado June, astro-ph/9411049 
504 |a Mukhanov, V., Feldman, H., Brandenberger, R., (1992) Phys. Rep, 215, p. 203 
504 |a (2000), http://pdg.lbl.gov, Particle Data Group, 14 June; Bachas, C.P., (2000) Class. Quant. Grav, 17, p. 951. , hep-th/0001093 
504 |a Antoniadis, I., Pioline, B., (1999) Nucl. Phys. B, 550, p. 41. , hep-th/9902055 
520 3 |a Variation of constants in the very early universe can generate inflation. We consider a scenario where the strong coupling constant was changing in time and where the gluon condensate underwent a phase transition ending the inflation. © World Scientific Publishing Company.  |l eng 
536 |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas 
536 |a Detalles de la financiación: This work was supported in part by CONICET, Argentina. N. Chamoun recognizes economic support from TWAS. 
593 |a Departamento de Física, Universidad Nacional de la Plata, c.c. 67, 1900 La Plata, Argentina 
593 |a Department of Physics, Higher Institute for Applied Sciences and Technology, P. O. Box 31983, Damascus, Syrian Arab Republic 
593 |a Observatorio Astronómico, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina 
593 |a Departamento de Física, Universidad Nacional de Buenos Aires, Ciudad Universitaria - Pab. 1, 1428 Buenos Aires, Argentina 
593 |a CONICET, Argentina 
690 1 0 |a INFLATION 
690 1 0 |a QCD 
690 1 0 |a VARIATION OF CONSTANTS 
700 1 |a Landau, S.J. 
700 1 |a Vucetich, H. 
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