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Degenerate neutrino as a Dark Energy. 12 th Marcel Grossmann Meeting, 12-18 July 2009, Paris Hyung Won Lee, Inje University July 15, 2009 Collaboration with K.Y. Kim, R. Ruffini. Contents. Introduction Properties of degenerate neutrino Evolution of density parameters
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Degenerate neutrino as a Dark Energy 12th Marcel Grossmann Meeting, 12-18 July 2009, Paris Hyung Won Lee, Inje University July 15, 2009 Collaboration with K.Y. Kim, R. Ruffini
Contents • Introduction • Properties of degenerate neutrino • Evolution of density parameters • Possibility as a dark energy • Remarks
Apparent Bolometric Magnitude m(z) Introduction • Universe is in accelerating expansionRiess & Perlmutter
Introduction • Universe is in accelerating expansionRiess & Perlmutter
Introduction • Universe is in accelerating expansionRiess & Perlmutter
Introduction • Universe is in accelerating expansionRiess & Perlmutter
Introduction • The present Universe • accelerated expansion supernova type Ia (SN Ia) data EOS (equation of state) • Main issue of the present cosmology : How to explain the present accelerating universe?negative pressure : Dark Energy candidate: cosmological constant , quintessence , k- essence , holographic dark energy , phantom matter , MaVaN …
Introduction • All candidates have weakness • No physical explanation is given • Can we explain dark energy or accelerating expansion with some physical principle? • Can we explain accelerating expansion with neutrinos?
Properties of degenerate neutrino • Decouple at early time • Energy density proportional to degeneracy parameter • It may have mass
Evolution of density parameters • Hubble equation • Distance modulus
Evolution of density parameters • (0.1, 0.9), (0.3, 0.7), (0.5, 0.7), LCDM
Possibility as a dark energy • Light mass : do not generate structure • May dominate energy density with degeneracy • Evolution may different from standard cosmology
Possibility as a dark energy • It is not possible to explain with standard consideration • Need to study carefully Boltzmann equation
Remarks • It seems not possible as a dark energy except mass varying with scalar field coupling • Cosmological integration of kinematic equation