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Some model-independent phenomenological consequences
of flexible brane-worlds
IRGAC 2006
Barcelona, July 11-15 2006
J.A.R. CembranosA. Dobado
A. L. Maroto
IRGAC 2006 Antonio L. Maroto 2
• Brane worlds: branons vs. KK gravitons • Phenomenology in colliders
• Branons as dark matter
• Virtual branon effects
Summary
IRGAC 2006 Antonio L. Maroto 3
• Brane worlds: branons vs. KK gravitons
IRGAC 2006 Antonio L. Maroto 4
Introduction: brane worlds
Rfundamental scale
of gravity in D = 4 + dimensions
brane tension
Brane universe
Brane hierarchy
MD f4
ADD, 98Antoniadis, et al. 98
IRGAC 2006 Antonio L. Maroto 5
Kaluza-Klein gravitons
3+1 coordinates extra-dimensional coordinates
KK gravitontower
Linearizing the bulkgravitational field
KK gravitonmass
(torus compactif.)
IRGAC 2006 Antonio L. Maroto 6
Coset space
Isometry group of GMN
Brane ground state
Branons (brane fluctuations)
Branons (x) GB fields Spontaneous isometry
breaking
Brane position
Sundrum, ‘99Dobado, A.L.M. ‘01
IRGAC 2006 Antonio L. Maroto 7
• Bulk metric:
• Branon mass related to bulk curvature:
• Induced metric on the brane:
Branons
IRGAC 2006 Antonio L. Maroto 8
Branon dynamics
Dirac-Nambu-GotoInduced metric
IRGAC 2006 Antonio L. Maroto 9
KK gravitons vs. branons
KK-production Branon production
KK-SM coupling suppression
Bando et al. ‘99
IRGAC 2006 Antonio L. Maroto 10
- Rigid branes ( f >> MD)
Kaluza-Klein modes Brane-world
scenario
- Flexible branes (f << MD)
Branon fields
(KK modes decouple from SM)
KK gravitons vs. branons
IRGAC 2006 Antonio L. Maroto 11
• Phenomenology in colliders
IRGAC 2006 Antonio L. Maroto 12
• Induced metric on the brane:
• Dirac - Nambu - Goto action:
Branon action
Limits from colliders
LEP-II ... TEVATRON-I
+ ...
hep-ex/0407017
Cembranos, Dobado, A.L.M, ’03
IRGAC 2006 Antonio L. Maroto 13
Prospects for future colliders
Single photon-Z Monojet (quark production)
Monojet(gluon prod.)
IRGAC 2006 Antonio L. Maroto 14
Prospects for future colliders
TEVATRON-II LHC
ILC
Cembranos, Dobado, A.L.M, ’04
IRGAC 2006 Antonio L. Maroto 15
• Branons as dark matter
IRGAC 2006 Antonio L. Maroto 16
• Brane orientation branons are pseudoscalar particles
• Parity on the brane branons couple by pairs to SM . (stable particles)
Branons are stable, massive and weakly interacting particles
NATURAL DARK MATTER CANDIDATES
A new dark matter candidate
Cembranos, Dobado, A.L.M, ’03
IRGAC 2006 Antonio L. Maroto 17
+e1
-
ê1
+e1
e2
+
ê2
ê1
Parity on the brane
Odd-dimensional branes: pseudoscalar branons
Even-dimensional branes: scalar branons
P
P
IRGAC 2006 Antonio L. Maroto 18
Branon cosmic abundance Freeze-out in an expanding universe:
Annihilation into all SM pairs X : ,
e.g. annihilation into photons, :
Cold branons (M >> T) Hot branons (M << T)
IRGAC 2006 Antonio L. Maroto 19
Branon cosmic abundance
Cold branons
WMAP limits
IRGAC 2006 Antonio L. Maroto 20
Branon cosmic abundance
Hot branons
WMAP WMAP-CBI-ACBAR-2dF-Ly-
BBN limits (light branons): for
IRGAC 2006 Antonio L. Maroto 21
Combined limits
IRGAC 2006 Antonio L. Maroto 22
Direct detection
Elastic branon-nucleon
cross section
(spin independent)
IRGAC 2006 Antonio L. Maroto 23
Non-thermal branon production
(M f2 RB)1/2explicit symmetry breaking scale).
Branons are very light particles and decoupled from SM.
Brane initial position: Y0 = O (RB) and f 2 RB
Dark matter as coherent brane oscillations (similar to axions)
If H(T) > (T) for T < TRH brane oscillations only diluted by
Hubble expansion.
Non-thermal branon abundance:
A.L.M, ’04
If << TRH << Tf
IRGAC 2006 Antonio L. Maroto 24
Non-thermal branon production
Tf < (M MP)1/2
IRGAC 2006 Antonio L. Maroto 25
• Virtual branon effects
IRGAC 2006 Antonio L. Maroto 26
Radiative corrections
Cembranos, Dobado, A.L.M, ’06
One-loop SM effective action
SM masses renormalization
New SM vertices
IRGAC 2006 Antonio L. Maroto 27
Muon anomalous magnetic moment
Cembranos, Dobado, A.L.M, ’06
Brookaven (g-2) coll. (2004) 2.7above SM
IRGAC 2006 Antonio L. Maroto 28
Conclusions and future perspectives
Low-energy branon dynamics universally described by effective action depending on 3 parameters (M,f,N) For f << MD only branons and SM particles relevant
degrees of freedom.
Limits on (M,f) from present and future colliders
Loop effects contribute to the muon anomalous magnetic moment
Branons are natural dark matter candidates (thermal or non- thermal production)
Future detection in direct or indirect experiments?