Proton Decay at DUSEL - PowerPoint PPT Presentation

1 / 35
About This Presentation
Title:

Proton Decay at DUSEL

Description:

P & P' parity affect boundary conditions. at fixed points. Title of talk. 21 ... Heterotic Road to the MSSM with R parity,'' arXiv:0708.2691 [hep-th] Title of ... – PowerPoint PPT presentation

Number of Views:66
Avg rating:3.0/5.0
Slides: 36
Provided by: nwgPh
Category:

less

Transcript and Presenter's Notes

Title: Proton Decay at DUSEL


1
Proton Decay at DUSEL
Stuart Raby

DUSEL Town Meeting Washington, D.C. November 3,
2007
2
Motivation for Deep Underground Science
Laboratory
  • Long-baseline neutrino oscillations
  • q13 , leptonic CP viol.
  • Astrophysical neutrinos - SN, solar,
    neutrino bkgd.
  • Neutrino masses - neutrinoless 2b decay
  • Direct dark matter detection
  • n-nbar oscillations
  • Proton decay
  • Can all be done with one large detector
  • Conclusions

3
Outline
  • SUSY GUTs
  • motivation and consequences
  • Proton decay
  • Conclusions

4
Supersymmetric Standard Model
Motivation ??
Solve hierarchy problem MZ/MPl 10-16
SM - fine-tuning 10-32
SUSY
technically natural
Dynamical
5
Phenomenology of SUSY GUTs
  • charge quantization

6
Pati-Salam SU(4)CxSU(2)LxSU(2)R
7
Georgi-Glashow
Pati-Salam
8
Charge quantization
Georgi Fritzsch Minkowski
spinor repsn. of SO( 10 )
9
Phenomenology
  • charge quantization
  • gauge coupling unification

10
Gauge coupling unification
11
Phenomenology
  • charge quantization
  • gauge coupling unification
  • neutrino masses
  • See-Saw scale ( .01 - .1 ) MGUT

12
Phenomenology
  • charge quantization
  • gauge coupling unification
  • neutrino masses
  • LSP- dark matter candidate
  • baryogenesis via leptogenesis
  • quark and lepton masses

13
Fermion Masses in SO(10)
l 16 10 16
top, bottom, tau, nt Yukawa unification
Minimal SO(10) Model
Mohapatra, Babu, Senjanovic, Bajc, Aulakh, Chen,
Mahanthappa,
14
Minimal SO(10) Model
II
Albright, Anderson, Babu, Barr, Barbieri,
Berezhiani, Blazek, Carena, Dermisek,
Dimopoulos, Hall, Pati, Raby, Romanino, Rossi,
Starkman, Wagner, Wilczek, Wiesenfeldt,
Willenbrock
Possible UV completion to strings !!
15
SO(10) x D3 x U(1) family sym. Yukawa
Unification for 3rd Family
Dermisek Raby hep-ph/0507045 Dermisek,
Harada S.R. hep-ph/0606055
16
SO(10) x D3 x U(1) family sym. Yukawa
Unification for 3rd Family
Fits fermion masses and mixing angles well
Requires soft SUSY breaking paras
Blazek, Dermisek Raby PRL 88 (2002)
17
Global c2 analysis of DR Model
24 parameters at GUT scale
compare to SM - 27 parameters
MSSM - 32 parameters
18
Recent analysis of DR Model
Challenging SO(10) SUSY GUTs with
family symmetries through FCNC processes Albrecht
, Altmannshofer, Buras, Guadagnoli, Straub
arXiv0707.3954 hep-ph

Find good fits to quark, charged lepton
neutrino masses and mixing angles Also test
flavor violation in b physics some tension
between b ? s g b ? s l l-
19
UV completion
Orbifold GUTs in 5 or 6 dimensions GUT
symmetry breaking Doublet-Triplet splitting
Kawamura Hall Nomura Contino, Pilo, Rattazzi
Trincherini Altarelli, Feruglio Masina
Dermisek Mafi H.D. Kim Raby Asaka,
Buchmuller Covi Lee Hebecker March-Russell
20
M4 x S1/(Z2xZ2)

P
P
P P parity affect boundary conditions at
fixed points
21
E6 Orbifold GUT on M4 x S1/(Z2xZ2)
Kobayashi, SR Zhang
22
UV completion
Orbifold GUTs in 5 or 6 dimensions Derived
from Heterotic string in 10 D
Kobayashi, Raby Zhang Forste, Nilles,
Vaudrevange Wingerter Buchmuller,
Hamaguchi, Lebedev Ratz JE Kim, JH Kim
Kyae Buchmuller, Ludeling Schmidt
23
E8 x E8 Heterotic string in 10D
Compactify 6D on (T2)3
Then mod by Z6 (Z3 x Z2) and Add Wilson
lines
Z6 embedded in E8 x E8 gauge lattice as shift
V6 consistent with mod. inv. !
24
First consider (T2)3/Z3 W3
Wilson line in
SU3 torus
Massless modes From Untwisted sector
(G2 , SU3) twisted sector
E6 GUT in 5D
25
Recently obtained MSSM
from heterotic string With 3 families, no
light exotics and non-trivial
quark lepton masses Lebedev et
al. The Heterotic Road to the MSSM with R
parity,''
arXiv0708.2691 hep-th
26
Phenomenology
  • charge quantization
  • gauge coupling unification
  • neutrino masses
  • dark matter candidate
  • baryogenesis via leptogenesis
  • quark and lepton masses
  • proton decay

27
Proton Decay -- gauge exchange
Lucas Raby, Murayama Pierce
MX gt 7x 1015 GeV tp gt 1.5x1034
years
28
Proton Decay -- higgs exchange
29
Proton Decay -- higgs exchange
  • c color triplet Yukawa coupling --
  • In a complete GUT its constrained by
  • fermion masses and mixing angles
  • blattice - a 0.0118(21) GeV3
  • ß 0.0118(21) GeV3
  • Y. Aoki
    et al. hep-lat/0607002

30
Proton Decay -- higgs exchange
  • Loop factor
  • gauginos (light), 12 gen. scalars
    (heavy)
  • constrained by gauge coupling
  • unification and GUT breaking sectors

31
Proton Decay -- higgs exchange
Babu, Pati Wilczek, Altarelli, Feruglio
Masina, Dermisek, Mafi Raby
SUSY GUTs Under siege !!
Dermisek, Mafi Raby
32
Proton Decay Orbifold GUTs
  • 5 6 dimensionful orbifold GUTs
  • dim. 5 operators - can be suppressed
  • dim. 6 operators - typically
    enhanced
  • MX lt MGUT
  • String orbifolds
  • dim. 5 operators strike back
  • dim. 6 operators - likely enhanced

33
Conclusions
  • SUSY GUTs predict proton neutron
  • decay with lifetimes exceeding BUT near
  • Super-K bounds
  • 5D Orbifold GUTs can suppress dim. 5
  • BUT enhance dim. 6 operators
  • Strings may enhance both ?
  • Observation of proton decay would
  • dramatically change our understanding of
  • nature !!

34
Conclusions
Proton decay should be just around the
corner BUT which mode dominates ? The
answer is model dependent !!
35
Conclusions
Proton decay should be just around the
corner BUT which mode dominates ? The
answer is model dependent !!
Write a Comment
User Comments (0)
About PowerShow.com