Tsujikawa, Phys. Rev. D 77, 023507 (2008)

Tsujikawa, Phys. Rev. D 77, 023507 (2008) Tsujikawa, Phys. Rev. D 77, 023507 (2008)

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I. IntroductionNo. 3・ Recent observations of Supernova (SN) Ia confirmed thatthe current expansion of the universe is accelerating.[Perlmutter et al. [Supernova Cosmology Project Collaboration], Astrophys. J. 517,565 (1999)][Riess et al. [Supernova Search Team Collaboration], Astron. J. 116, 1009 (1998)][Astier et al. [The SNLS Collaboration], Astron. Astrophys. 447, 31 (2006)]・ There are two approaches to explain the current cosmicacceleration. [Copeland, Sami and Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006)][Tsujikawa, arXiv:1004.1493 [astro-ph.CO]]< Gravitational field equation > G ö÷G ö÷ = ô 2 T ö÷GravityMatter(1) General relativistic approachT ö÷(2) Extension of gravitational theory2011 Nobel Prize in Physics: Einstein tensor: Energy-momentum tensor: Planck massDark Energy

I. IntroductionNo. 3・ Recent observations of Supernova (SN) Ia confirmed thatthe current expansion of the universe is accelerating.[Perlmutter et al. [Supernova Cosmology Project Collaboration], Astrophys. J. 517,565 (1999)][Riess et al. [Supernova Search Team Collaboration], Astron. J. 116, 1009 (1998)][Astier et al. [The SNLS Collaboration], Astron. Astrophys. 447, 31 (2006)]・ There are two approaches to explain the current cosmicacceleration. [Copeland, Sami and <strong>Tsujikawa</strong>, Int. J. Mod. <strong>Phys</strong>. D 15, 1753 (2006)][<strong>Tsujikawa</strong>, arXiv:1004.1493 [astro-ph.CO]]< Gravitational field equation > G ö÷G ö÷ = ô 2 T ö÷GravityMatter(1) General relativistic approachT ö÷(2) Extension of gravitational theory2011 Nobel Prize in <strong>Phys</strong>ics: Einstein tensor: Energy-momentum tensor: Planck massDark Energy

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