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Leptogenesis, neutrino mixing data and the absolute neutrino mass scale
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LEPTOGENESIS, NEUTRINO MIXING DATA AND THE ABSOLUTE
NEUTRINO MASS SCALE a
P. Di Bari
IFAE, Universitat Auto?noma de Barcelona, 08193 Bellaterra (Barcelona), Spain
Recent developments in thermal leptogenesis are reviewed. Neutrino mixing data favor a
simple picture where the matter-anti matter asymmetry is generated by the decays of the
heavy RH neutrinos mildly close to thermal equilibrium and, remarkably, in the full non
relativistic regime. This results into predictions of the final baryon asymmetry not depending
on the initial conditions and with minimized theoretical uncertainties. After a short outline of a
geometrical derivation of the CP asymmetry bound, we derive analytic bounds on the lightest
RH neutrino mass and on the absolute neutrino mass scale. Neutrino masses larger than
0.1 eV are not compatible with the minimal leptogenesis scenario. We discuss how the results
get just slightly modified within the minimal supersymmetric standard model. In particular
a conservative lower bound on the reheating temperature, TR 10
9 GeV, is obtained in the
relevant effective neutrino mass range m?1 3×10
?3 eV. We also comment on the existence of
a ‘too-short-blanket problem’ in connection with the possibility of evading the neutrino mass
upper bound.
aCompendium of 1 and 2 mostly based on 3 with some new results in 3.4, 3.8 and 3.9.
1 Introduction
Cosmic rays and CMBR observations indicate that our observable Universe is baryon asym-
metric 4. Moreover the observation of the acoustic peaks in the power spectrum of CMBR
5, combined with large scale structures observations 6, provide a precise and robust mea-
surement of such an asymmetry that can be expressed in terms of the baryon to photon
number ratio at the recombination time,
ηCMBB = (6.3 ± 0.3) × 10?10 , (1)
in very good agreement with the latest determination from (NACRE updated) Standard
BBN and primordial Deuterium measurements that give 7
ηS
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