Blucher Physics Proceedings

Setembro 2017, vol.4, num.1 - VIII Encontro Científico de Física Aplicada
Artigo Completo - Open Access Idioma principal | Segundo principal

BETOCS using the 157 gold SNe Ia Data: Hubble is not humble

BETOCS using the 157 gold SNe Ia Data: Hubble is not humble

Colistete Jr., R.; Giostri, R.

Artigo Completo:

The type Ia supernovae observational data is one of the most important in observational cosmology nowadays. Here we present the first public version of BETOCS (BayEsian Tools for Observational Cosmology using SNe Ia), which is a powerful and high productivity tool aimed to help the theoretical physicist community investigate cosmological models using type Ia supernovae (SNe Ia) observational data. BETOCS is applied to the generalized Chaplygin gas model (GCGM), traditional Chaplygin gas model (CGM) and LCDM, ranging from 5 to 3 free parameters, respectively. The “gold sample” of 157 supernovae data is used. It is shown that the Chaplygin gas scenario is viable (in most cases the LCDM is disfavoured) and the quartessence scenario (that unifies the description for dark matter and dark energy) is favoured. The Hubble parameter (H0) is important and should not be fixed and it can be estimated or marginalized with or without the Hubble Space Telescope prior.

The type Ia supernovae observational data is one of the most important in observational cosmology nowadays. Here we present the first public version of BETOCS (BayEsian Tools for Observational Cosmology using SNe Ia), which is a powerful and high productivity tool aimed to help the theoretical physicist community investigate cosmological models using type Ia supernovae (SNe Ia) observational data. BETOCS is applied to the generalized Chaplygin gas model (GCGM), traditional Chaplygin gas model (CGM) and LCDM, ranging from 5 to 3 free parameters, respectively. The “gold sample” of 157 supernovae data is used. It is shown that the Chaplygin gas scenario is viable (in most cases the LCDM is disfavoured) and the quartessence scenario (that unifies the description for dark matter and dark energy) is favoured. The Hubble parameter (H0) is important and should not be fixed and it can be estimated or marginalized with or without the Hubble Space Telescope prior.

Download (PDF)

Palavras-chave:

DOI: 10.5151/phypro-viii-efa-36

Referências bibliográficas
  • [1] Riess, A.; et al. Astron. J. v. 116, p. 1009, 1998.
  • [2] Perlmutter, S.; et al. Astrophys. J., v. 517, p. 565, 1999.
  • [3] Spergel, D. N.; et al. Astrophys. J. Suppl., v. 148, p. 175, 2003.
  • [4] Turner, E. L.; Ostriker, J. P.; Gott III, J. R. Astrophys. J., v.284, p. 1, 1984.
  • [5] Fukugita, M.; Futamase, T.; Kasai, M. Mont. Not. R. Astron. Soc., v. 246, p. 24, 1990.
  • [6] Allen, S. W.; et al., Monthly Notices of the Royal Astron. Society, v. 353, p. 457, 2004.
  • [7] Bagla, J. S.; Padmanabhan, T.; Narlikar, J. V. Comments on Astrophysics, v. 18, p. 275, 1996; arXiv:astro-ph/9511102.
  • [8] Weinberg, S. Rev. Mod. Phys., v. 61, p. 1, 1989.
  • [9] Carroll, S. M. Living Rev. Rel., v. 4, p. 1, 2001.
  • [10] Caldwell, R. R.; Dave R.; Steinhardt, P. J. Phys. Rev. Lett., v. 80, p. 1582, 1998.
  • [11] Zlatev, I.; Wang, L.; Steinhardt, P. J. Phys. Rev. Lett., v. 82, p. 896, 1999.
  • [12] Kamenshchik, A.; Moschella, U.; Pasquier, V. Phys. Lett. B, v. 511, p. 265, 2001.
  • [13] Makler, M. Gravitational Dynamics of Structure Formation in the Universe, PhD Thesis, Brazilian Center for Research in Physics, 2001.
  • [14] Bili´c, N.; Tupper, G.B.; Viollier, R. D. Phys. Lett. B, v. 535, p. 17, 2002.
  • [15] Bento, M. C.; Bertolami, O.; Sen, A. A. Phys. Rev. D, v. 66, p. 043507, 2002.
  • [16] Jackiw, R. A particle field theorist’s lectures on supersymmetric, nonabelian fluid mechanics and d-branes, arXiv:physics/0010042.
  • [17] Fabris, J. C.; Gonçalves, S. V. B.; de Souza, P. E. Gen. Rel. Grav., v. 34, p. 53, 2002.
  • [18] Sandvik, H.; Tegmark, M.; Zaldarriaga, M.; Waga, I. Phys. Rev. D, v. 69, p. 123524, 2004.
  • [19] Bec¸a, L. M. G.; Avelino, P. P.; de Carvalho, J. P. M.; Martins, C. J. A. P. Phys. Rev. D, v. 67, p. 101301, 2003.
  • [20] Colistete Jr., R.; Fabris, J. C. Class. Quantum Grav., v. 22, p. 2813, 2005.
  • [21] Colistete Jr., R.; Fabris, J. C.; Gonçalves, S. V. B.; de Souza, P. E. Int. J. Mod. Phys. D, v. 13, p. 669, 2004.
  • [22] Colistete Jr., R.; Fabris, J. C.; Gonçalves, S. V. B. Int. J. Mod. Phys. D, v. 14, p. 775, 2005.
  • [23] Colistete Jr., R. BayEsian Tools for Observational Cosmology using SNe Ia (BETOCS), available on the Internet site http://www.RobertoColistete.net/BETOCS, access in 2017.
  • [24] Wolfram, S. The Mathematica Book, 5th ed., Cambridge University Press, 2003.
  • [25] Freedman, W. Astrophys. J., v. 553, p. 47, 2001.
  • [26] Riess, A. G.; et al. Astrophys. J., v. 607, p. 665, 2004.
  • [27] Makler, M.; Oliveira, S. Q.; Waga, I. Phys. Lett. B, v. 555, p. 1, 2003.
  • [28] Loredo, T. J. Maximum Entropy and Bayesian Methods, ed. P. F. Fougere, Kluwer Academic Publishers, Dordrecht, 1990.
  • [29] Loredo, T. J. Statistical Challenges in Modern Astronomy, ed. E. D. Feigelson and G. J. Babu, Springer-Verlag, New York, 1992.
  • [30] Gregory, P. C.; Loredo, T. J. Astrophys. J., v. 398, p. 146, 1992.
  • [31] Abroe, M. E.; et al. Mon. Not. R. A. Soc., v. 334, p. 11, 2002.
  • [32] Krauss, L. M. The state of the Universe: cosmological parameters, 2002; arXiv:astroph/0301012.
  • [33] Casarejos, F.; Fabris, J. C.; Gonçalves, S. V. B.; da Rocha, J. F. V. Phys. Lett. A, v. 367, p. 423, 2007.
  • [34] Astier, P.; et al. (SNLS colaboration). Astron. Astrophys., v. 447, p. 31, 2006.
  • [35] Nesseris, S.; Perivolaropoulos, L. Phys. Rev. D, v. 70, p. 043531, 2004.
  • [36] Jassal, H. K.; Bagla, J. S.; Padmanabhan, T. Mon. Not. Roy. Astron. Soc., v. 405, p. 2639, 2010.
  • [37] Nesseris, S.; Perivolaropoulos, L. JCAP, v. 01, p. 018, 2007.
  • [38] Cunha, J. V.; Alcaniz, J. S.; Lima, J. A. S. Phys. Rev. D, v. 69, p. 083501, 2004.
  • [39] Amendola, L.; Makler, M.; Reis, R. R. R.; Waga, I.; Phys. Rev. D, v. 74, p. 063524, 2006.
Como citar:

Colistete Jr., R.; Giostri, R.; "BETOCS using the 157 gold SNe Ia Data: Hubble is not humble", p-165-180. In: . São Paulo: Blucher, 2017.
ISSN 23582359, DOI 10.5151/phypro-viii-efa-36

últimos 30 dias

98
downloads

253
visualizações

744
indexações