Transcript Dark Matter in LR models - National Tsing Hua University
Dark Matter stability and boost factor from DM conversions Yu-Feng Zhou
Z.P.Liu, W.L.Guo,Y.L.Wu, C. Zhuang
Institute of theoretical physics (ITP), Chinese Academy of Sciences (CAS).
PRD79,055015(2009); PRD81,075014(2010) ArXiv:1008.4479 (PRD),
work in progress
The second DM/DE workshop, Nov.5, 2010
Part-I: by P and CP symmetries
A model with dark matter stabilized
The stability of DM A LR model with DM stabilized by P and CP Phenomenology: relic density & Direct detection
Part II: from DM conversion
a scenario for large boost factor
Boost factor required by PAMELA/Fermi LAT Dark matter decay through tiny C- breaking terms Predictions for cosmic-ray neutrinos and diffuse gamma rays Boost factor from late time DM conversion Numerical results Simple models .
Symmetries for DM stability
Well known: R-parity, KK-parity, T-parity Kadastik, Kanikel, Raidal 09 ’ , Frigerio and Hambye 09
Hidden sector U(1) symmetry
Ackerman,buckley,Carroll, Kamonkowski 08’ Feng, Tu, Yu 08’, Feng, Kaplinghat, Tu, Yu 09’ Foot etal. 10’
kinetic mixing Broken U(1): a massive Z ’ , a scalar
Pospelov, Ritz, voloshin 07’ Gpoalakrishnal,Jung,Wells 08’ Gpoalakrishnal,Lee,Wells 08’ Mambrini 10’
Higgs portal kinetic mixing
Large SU(2)_L multiplets (minimal DM) Cirelli, Fornengol, Strumia 06’ Cirelli, Strumia, Tamburini 07’
Hidden custodial symmetry vector DM
Custodial symmetry SU(2)_C keep vector bosons stable
DM in minimal extensions of the SM
Extension to SM with scalar DM
SM Scalar DM
Silveira, Zee, 1985 McDondald, 1994, Burgess, Pospelov & Veldhuis, 2001 Barger,Langacker, KcCaskey, 2007 Shafi, Okada, 2009 He,Li, Tsai, 2007,2009 Extension to LRM with scalar DM
Left-Right Model Scalar DM
Stability can be protected by P and CP
A LR model with spontaneous P and CP violation Gauge interaction: Flavor contents
Two bi-doublet required for spontaneous CP violation.
Only one bi-doublet cannot give the correct CP phase
P- and CP-transformations
If P and CP are only broken spontaneously
S_D does not participate gauge Interactions, as it is gauge singlet Require that S_D does not develop a nonzero VEV S_D a DM particle
Guo, Wu, YFZ, PRD81,075014 (2010)
Main annihilation channels Thermally averaged cross section & relic density
Relic density and direct detection
Parameter space from relic density Prediction for direct detection rate
one bi-doublet case two bi-doublet case Guo, Wang, Wu, YFZ, Zhuang,PRD79,055015(2009);
A special case
: large Yukawa couplings to light quarks • Relic density is dominated by heavy quark, not light ones • DM-nucleus scattering is sensitive to light quark Yukawa couplings
DM decay through soft C-breaking terms
Guo, Wu, YFZ, PRD81,075014 (2010)
Including soft C-breaking term
dominant part: C- and P-even tiny part: C-odd
Decay through left-handed triplet can well explain the PAMELA/Fermi data Triplets with nonzero B-L number do not couple to quarks through Yukawa interactions Indirect channels WW, WZ, and ZZ suppressed by tiny triplet VEV required by neutrino masses.
mass parameters Guo, Wu, YFZ, PRD81,075014 (2010) Consider 3 cases with final states dominated by different lepton flavor PAMELA
Explain PAMELA data well. for all type of lepton final states.
mu/tau final states favored by Fermi tau-lepton final states predict High neutrino-induced muon flux
Predictions for up-going muon flux
Triplets couple to neutrinos and charged-leptons with the same strength
Guo, Wu, YFZ, PRD81,075014 (2010)
up-going muon flux can reach the current SK bound
Inverse Compton scattering ( ICS ) ICS FSI VIB Final state radiation ( FSI )
ICS FSI VIB Virtual internal bremsstrahlung ( VIB ) ICS FSI VIB ICS FSI VIB Guo, Wu, YFZ, PRD81,075014 (2010)
Summary of part I
We have proposed a LR model with scalar DM candidate stabilized by C and CP-symmetries. Tiny DM particle decay is induced through adding tiny soft C-violation interactions.
the DM particle can decay trough SU(2)_L triplet scalars which couple mostly to leptons.
The model predicts large neutrino-induced muon flux for certain leptonic final states. The model also predict new sources for very high energy gamma-rays, favorably in the ~ TeV region.
Part-II Boot factor from DM conversions
Liu, YFZ, Wu, work in progress
The boost factor problem
The std. WIMP annihilation cross section is too small to account for the PAMELA/Fermi data Positron flux
Bergstrom, Edsjo, Zaharijas, PRL103,031103,09’
Possible origins of boost factor
Boot factor for DM annihilation Local clumps Via Lactea II: in subhalo? B~ 4-15,
Diemand, et al, 0805.1244, Nature
Temperature-dependent ann. cross section Sommerfeld enhancement
Sommerfeld, Ann. Phy 403, 257 (1931).
Resonance enhancement Non-thermal origin of DM DM may decay rather than annihilate
The Sommerfeld effect
A. Sommerfeld, Annalen der Physik 403, 257 (1931).
J. Hisano, S. Matsumoto and M. M. Nojiri, Phys. Rev. D 67 (2003) Phys. Rev. Lett. 92, 031303 (2004 )
Constraints from relic density
J. L. Feng, M. Kaplinghat and H. B. Yu, Phys. Rev. Lett. 104, 151301 (2010)
Constraints from relic density J. L. Feng, M. Kaplinghat and H. B. Yu, Phys. Rev. Lett. 104, 151301 (2010) arXiv:1005.4678
Refined analysis at freeze-out
• • Cut-off of resonance, recoupling • Force-carrier production & decay rates Kinetic decoupling • Self-interaction efficiency, non-thermality
•Halo shape •CMB, protohalo J. Zavala, M. Vogelsberger and S. D. M. White, Phys. Rev. D 81, 083502 (2010) M. Kamionkowski and S. Profumo, Phys. Rev. Lett. 101,261301 (2008)
Multi-component DM and the boost factor Multi-component DM Models with hidden sectors naturally have multi-DM DM may have SUSY partners Neutrinos are already (tiny) part of DM No boost from simply mixed thermal DM For thermal relic
Large boost requires
Large annihilation cross section 2. Still the correct relic density Impossible for thermal DM ?
Correlated thermal evolution In the case of interacting multi-component DM
Thermal evolution for interacting DM
Two component case (s-wave)
( Kinetic equilibrium assumed
The conversion term The role of Keep the DM in chemical equilibrium Convert the heavy DM into the light
Stages of the thermal evolution 1.
Thermal equilibrium 2.
Departure from thermal equilibrium 3.
Late time DM conversion when z is large Slow conversion characterized by r(z) Crossing point 4.
The boost factor Evolution of the total density Late time evolution
Large boost factor if mass diff. is small
B~150 With conversion no conversion B~1000
B vs mass difference B vs relative cross sections
A simple model
Add to the SM
Cross sections & boost factor Internal degree of freedom Parameter set cross sections Cross sections Boost factors For near resonance case, all couplings can be smaller
Summary of part II
In multi-DM models, DM conversion can significantly modify the thermal evolution of each DM component.
The relic density of the DM component may not always inversely proportional to it ’ s annihilation cross section. Through conversions from heavier DM components, the relic density of light DM can be enhanced, leading to large boost factors.
The boost is mostly temperature independent. For generic models with large conversion rate the boost fact can reach ~100-1000. Thank You !
Sources from DM decay Background
The Sommerfeld enhancement
N. Arkani-Hamed, et al, Phys. Rev. D 79, 015014(2009) Sommerfeld enhancement factor S:
KITPC 2011 program
Dark matter and new physics
Sept. 21-Nov. 06, 2011 (7-week)
Shafi, Qaisar Aprile, Elena (Delaware), (Columbia U.) Wang, Tsz-king Henry(IOP, ) Wefel, John (Louisiana State U.) Matsumoto, Shigeki Su, Shu-Fang (IPMU), (Arizona U.) Geng, Chao-Qiang ( NCTS ),
Bi, Xiao-Jun (IHEP) Ni, Kai-Xuan (SJTU) Yang, Chang-Geng Yue, Qian (IHEP) (Tsinghua U.) Zhou, Yu-Feng (ITP )