significant effects of second kk particles on lkp dark matter physics
DESCRIPTION
Collaborated with Mitsuru Kakizaki (ICRR) Shigeki Matsumoto (ICRR) Yoshio Sato (Saitama U.). Significant effects of second KK particles on LKP dark matter physics. Masato Senami (ICRR, University of Tokyo) [email protected]. hep-ph/0502059. Kaluza-Klein dark matter. - PowerPoint PPT PresentationTRANSCRIPT
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Significant effects of second KK Significant effects of second KK particles on LKP dark matter physicsparticles on LKP dark matter physics
Collaborated withCollaborated with
Mitsuru Kakizaki (ICRR)Mitsuru Kakizaki (ICRR)
Shigeki Matsumoto (ICRR)Shigeki Matsumoto (ICRR)
Yoshio Sato (Saitama U.)Yoshio Sato (Saitama U.)
hep-ph/0502059
Masato SenamiMasato Senami(ICRR, University of Tokyo)(ICRR, University of Tokyo)
[email protected]@icrr.u-tokyo.ac.jp
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Kaluza-Klein dark matterKaluza-Klein dark matter
WMAP result establish the existence of non-baryonic cold dark matter
Weakly Interacting Massive Particle (WIMP) is excellent candidate Lightest supersymmetric particle Lightest Kaluza-Klein particle (LKP)
in universal extra dimension (UED) models
…
http://lambda.gsfc.nasa.gov
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Universal Extra Dimension modelUniversal Extra Dimension modelUniversal means all SM particles propagate in spatial extra dimensions
Momentum conservation in higher dim.= KK number conservation
KK parity conservation
To obtain chiral fermion at zero mode, the extra dimension is compactified by S1/Z2
LKP is stable
Mass spectrum
In 4 dim. viewpoint
LKP is a good candidate of DMLKP is a good candidate of DM
Eq. of motion
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1/R=500 GeV, ΛR=20, mh=120 GeV
Mass of KK particleMass of KK particle Each KK mode has degenerate mass
Radiative corrections remove the degeneracy
Lightest KK particle
Mass spectrum
Cheng, Matchev and Schmaltz
(SM massless particles are exactly degenerate)
m = mass of LKP
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Dark matter relic abundanceDark matter relic abundance After annihilation rate dropped
below the Hubble parameter, LKP can not annihilate and the density per comoving volume is fixed.
Large cross section
⇒ small relic abundance
Servant and Tait
Tree level annihilation diagrams
DM relic abundance
⇒Large mass of DM particle
They consider only the first KK modes
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Second KK s-channelSecond KK s-channel
Since DM is non-relativistic,
the incident energy of two LKPs is almost degenerate with the mass of second KK modes
In particular, s-channel LKP annihilation process mediated by competes with tree level diagrams because of the resonance
does not couple withSM particle at tree level
One of the resonant diagrams We calculatethese type of diagrams
We find
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Cross sectionCross section Parameters
For δ ~ 0.01, incident energy matches the pole and averaged cross section is significantly enhanced (10% ~ 100%)
δ ~ 0.01 is realized for
after the inclusion of the radiative corrections in the minimal UED
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Dark matter abundanceDark matter abundance
The mass of the KK dark matter consistent with the WMAP data is around 950 GeV
This result is about 100 GeV above compared to the tree-level result
The resonant annihilation process mediated by causes this increase
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Second KK resonanceSecond KK resonance The s-channel annihilation
First KK mass ~ m
Second KK mass ~ 2m Energy of two first KK mode
second KK mass second KK particle ⇒ s-channel
resonance`natural resonance’
This resonance is natural!
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ConclusionConclusion
Second KK particle effect : `natural resonance’ Relic abundance of the LKP,
s-channel resonanceKK dark matter mass consistent with WMAP
~950 GeV (about 100 GeV above the tree result)
`Natural resonance’ affects coannihilation indirect detection collider signature
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Second KK resonanceSecond KK resonance Coannihilation
If degenerate with in mass, coannihilates with
tree level coannihilation rate is small s-channel :
dipole type interaction
Indirect detection DM is almost at rest : good accuracy s-channel second KK B-boson
Collider signature Future linear e+e- collider s-channel second KK W-boson M. Battaglia et al. hep-ph/0502041
missing
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Second KK Higgs mass differenceSecond KK Higgs mass difference
100 150 200 250 300
600
800
1000
1200
1400
1 % 0 %0.5 %
2 %1.5 %
-0.5 %
m
mh
(GeV)
(GeV)
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Cross sectionsCross sections
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Some diagramsSome diagrams
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Radiative correctionsRadiative corrections
Weak mixing anglesTree level mass spectrum
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AbstractAbstract
SUSY UED similarity
LHC で new physics を発見しても区別できない
superparticle, soft mass
stable LSPfirst KK mode, 1/R mass
stable LKP
superpartner : single different spin
KK mode : tower identical spin
angular distributionenergy spectrumtotal cross-section
Lepton collider! Compact Linear Collider (CLIC)
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1/R=500 GeV, ΛR=20, mh=120 GeV
Radiative correctionsRadiative corrections Radiative corrections remove the
degeneracyLightest KK particle
Second KK particles couple to SM particles(KK number violating interaction
is forbidden by the momentum conservation)
n=20
0
11
1
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Comparison of UED and SUSYComparison of UED and SUSY
UED parameter is chosen naturally
MSSM parameter is adjusted to UED parameter
Back ground
Events
~ 20fb
small polar angle
missing energy > 2.5 TeVtransverse energy < 150 GeVevent sphericity > 0.05
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Angular distribution and spin measurementsAngular distribution and spin measurements
UED
SUSY
UED SUSY
14.4 fb
2.76 fb
Background free!!
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Threshold scansThreshold scans
cross section
includebeamstrahlung
confirm に利用New particle の質量決定
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Muon energy spectrumMuon energy spectrum
UED SUSY
UED
SUSY
For UED,
UED,SUSY の区別には使えない
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ResonanceResonance SUSY Z,γ s-channel UED Z2,γ2 s-channel Resonance!!
is kinematically forbidden.
is kinematically allowed.
is mostly -likeand predominantly couple to
1/R = 1350 GeVWeak mixing angle for second KK mode is very small