2008

SO(10) SUSY GUTs, the gravitino problem, non-thermal leptogenesis and axino dark matter

Baer, Howard, Summy, Heaya

Understand

Simple SUSY GUT models based on the gauge group SO(10) require t-b-\tau Yukawa coupling unification, in addition to gauge coupling and matter unification.

The Yukawa coupling unification places strong constraints on the expected superparticle mass spectrum, with scalar masses \sim 10 TeV while gaugino masses are quite light.
A problem generic to all supergravity models comes from overproduction of gravitinos in the early universe: if gravitinos are unstable, then their late decays may destroy the predictions of Big Bang nucleosynthesis.
We present a Yukawa-unified SO(10) SUSY GUT scenario which avoids the gravitino problem, gives rise to the correct matter-antimatter asymmetry via non-thermal leptogenesis, and is consistent with the WMAP-measured abundance of cold dark matter due to the presence of an axino LSP.

Built on

H. Georgi and S. Glashow,
1978
Earlier work this paper cites.
P. Minkowski,
1980
Earlier work this paper cites.
H. P. Nilles and S. Raby,
1984
Earlier work this paper cites.
B. Ananthanarayan, G. Lazarides and Q. Shafi,
1993
Earlier work this paper cites.
R. Hempfling,
1994
Earlier work this paper cites.
M. Fukugita and T. Yanagida,
1996
Earlier work this paper cites.
G. Lazarides and Q. Shafi,
1999
Earlier work this paper cites.
S. Profumo,
2000
Earlier work this paper cites.
J. Feng, C. Kolda and N. Polonsky,
2000
Earlier work this paper cites.
Y. Kawamura,
2001
Earlier work this paper cites.
H. Baer, M. Diaz, J. Ferrandis and X. Tata,
2001
Earlier work this paper cites.

Similar

L. Covi, J. E. Kim and L. Roszkowski,
2001
Cited alongside, same era.
H. Baer, C. Balazs and A. Belyaev,
2002
Cited alongside, same era.
K. Hamaguchi, H. Murayama and T. Yanagida,
2002
Cited alongside, same era.
H. Baer and J. Ferrandis,
2003
Cited alongside, same era.
T. Blazek, R. Dermisek and S. Raby,
2003
Cited alongside, same era.
J. L. Feng, A. Rajaraman and F. Takayama,
2003
Cited alongside, same era.
H. Georgi, in
2004
Cited alongside, same era.
D. Auto, H. Baer, A. Belyaev and T. Krupovnickas,
2004
Cited alongside, same era.
S. Weinberg,
2004
Cited alongside, same era.
W. Buchmüller, P. Di Bari and M. Plumacher,
2004
Cited alongside, same era.
A. Brandenburg and F. Steffen, JCAP
2004
Cited alongside, same era.

Then

M. Ibe, K.-I. Izawa and T. Yanagida,
2005
Later among the works it cites.
M. Ibe, T. Moroi and T. Yanagida,
2005
Later among the works it cites.
H. Baer and X. Tata,
2006
Later among the works it cites.
ISAJET v7.74, by H. Baer, F. Paige, S. Protopopescu and X. Tata, hep-ph/0312045; for details on the Isajet spectrum calculation, see H. Baer, J. Ferrandis, S. Kraml and W. Porod,
2006
Later among the works it cites.
D. N. Spergel
2006
Later among the works it cites.
K. Kohri, T. Moroi and A. Yotsuyanagi,
2006
Later among the works it cites.
K. Jedamzik, M. Lemoine and G. Moultaka, JCAP
2006
Later among the works it cites.
M. Bolz, A. Brandenburg and W. Buchmüller,
2007
Later among the works it cites.
H. Baer, S. Kraml, S. Sekmen and H. Summy,
2008
Closest in time.
H. Baer, H. Prosper and H. Summy,
Original
2008
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…