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Extra Dimensions: From Colliders to Cosmology
• Large Extra Dimensions (Primordial Black Holes)
• Universal Extra Dimensions (KK Bino)
• Warped Extra Dimensions (KK R )
Michell Symposium 2007J. Hewett
Collider signals & DM properties*
* Thanks to T. Tait!
Kaluza-Klein tower of particles
E2 = (pxc)2 + (pyc)2 + (pzc)2 + (pextrac)2 + (mc2)2
In 4 dimensions, looks like a mass!
pextra is quantized = n/R
Small radius Large radius
Small radius gives well separated Kaluza-Klein particles
Large radius gives finely separated Kaluza-Klein particles
Tower of massive particles
Large Extra Dimensions
Motivation: solve the hierarchy problem by removing it!
SM fields confined to 3-brane
Gravity becomes strong in the bulk
Arkani-Hamed, Dimopoulos, Dvali, SLAC-PUB-7801
Gauss’ Law: MPl2 = V MD
2+ , V = Rc
MD = Fundamental scale in the bulk ~ TeV
Kaluza-Klein Modes in a Detector Indirect Signature
Missing Energy Signature pp g + GnJLH Vacavant, Hinchliffe
Graviton Exchange Modified with Running Gravitational Coupling
Insert Form Factor in coupling to
parameterizerunning
M*D-2 [1+q2/t2M*
2 ]-1
Could reduce signal!D=3+4M* = 4 TeV
SM
t=
1
0.5
JLH, Rizzo, to appear
Constraints from Astrophysics/Cosmology
• Supernova CoolingNN NN + Gn can cool supernova too rapidly
• Cosmic Diffuse RaysNN NN + Gn
Gn
• Matter Dominated Universetoo many KK states
• Neutron Star Heat ExcessNN NN + Gn
becomes trapped in neutron star halo
and heats it
-
Cullen, PerelsteinBarger etal, Savage etal
Hannestad, RaffeltHall, Smith
Fairbairn
Hannestad, Raffelt
Astrophysical Constaints*: MD in TeV
= 2 3 4 5
Supernova Cooling 9 0.66 0.01
Cosmic Diffuse -rays Sne 28 1.65 0.02 Sne Cas A 14 1.2 0.02 Neutron Star 39 2.6 0.4
Matter Dominated Universe 85 7 1.5
Neutron Star Heat Excess 700 25 2.8 0.57
Low MD disfavored for ≤ 3
* Can be evaded with hyperbolic manifolds
- Starkman, Stojkovic, Trodden
Hannestad, Raffelt
Black Hole Production @ LHC:
Black Holes produced when s > M*
Classical Approximation: [space curvature << E]
E/2
E/2b
b < Rs(E) BH forms
Geometric Considerations:
Naïve = Rs2(E), details show this holds up to a
factor of a few
Dimopoulos, LandsbergGiddings, Thomas
Black Hole event simulation @ LHC
Decay Properties of Black Holes (after Balding):Decay proceeds by thermal emission of Hawking
radiation
At fixed MBH, higher dimensional BH’s are hotter: N ~ 1/T
higher dimensional BH’s emit fewer quanta, with each quanta having higher energy
Harris etal hep-ph/0411022
Multiplicity for n = 2 to n = 6
n determined to n = 0.75 @ 68% CL for n=2-6 from TH and This procedure doesn’t work for large n
pT distributions of Black Hole decays
Provide good discriminating power for value of n
Generated using modified CHARYBDIS linked to PYTHIA with M* = 1 TeV
Production rate is enormous!
1 per sec at LHC!
JLH, Lillie, Rizzo
Determination of Number of Large Extra Dimensions
Primordial Microscopic Black Holes
• Produced in high-energy collisions in early universe
• Rapid growth by absorption of matter from surrounding plasma
Demand:1.Black Holes not
overclose the universe2.Must not dominate
energy density during BBN
Mass density determined by TI
Conley, Wizansky
Excluded
Empty Bulk
Thermalized Bulk
Universal Extra Dimensions
• All SM fields in TeV-1, 5d, S1/Z2 bulk• No branes! translational invariance is
preserved tree-level conservation of p5
• KK number conserved at tree-level broken at higher order by boundary terms
• KK parity conserved to all orders, (-1)n
Consequences:1. KK excitations only produced in pairs
Relaxation of collider & precision EW constraints Rc
-1 ≥ 300 GeV!
2. Lightest KK particle is stable (LKP) and is Dark Matter candidate
3. Boundary terms separate masses and give SUSY-like spectrum
Appelquist, Cheng, Dobrescu
Universal Extra Dimensions: Bosonic SUSY
Phenomenology looks like Supersymmetry:
Heavier KK particles cascade down to LKP
LKP: Photon KK state appears as missing
ET
SUSY-like Spectroscopy
Confusion with SUSY if discovered @ LHC !
Chang, Matchev,Schmaltz
Spectrum looks like SUSY !
How to distinguish SUSY from UED I:
Observe KK states in e+e- annihilation
Measure their spin via:
•Threshold production, s-wave vs p-wave•Distribution of decay products
•However, could require CLIC energies...
JLH, Rizzo, TaitDatta, Kong, Matchev
How to distinguish SUSY from UED II:
Observe higher level (n = 2) KK states:
– Pair production of q2q2,
q2g2, V2 V2
– Single production of V2 via (1) small KK number breaking couplings and (2) from cascade decays of q2
Discovery reach @ LHC
Datta, Kong, Matchev
How to distinguish SUSY from UED III:
Measure the spins of the KK states @ LHC – Difficult!
Decay chains in SUSY and UED:
Form charge asymmetry:
Works for some, but not all, regions of parameter space
Smillie, Webber
Identity of the LKP
• Boundary terms (similar to SUSY soft-masses) – Induced @ loop-level (vanish @ cut-off)– Determine masses & couplings of entire KK tower
1 ≪ 2 ≪ 3
– Smallest corrections to U(1) KK state
– NLKP is eR(1)
M ~ 1/R > v– LKP is almost pure Bino KK B
(1)
Bino-Wino mass matrix, n=1
Thermal Production and Freeze Out
• Assume LKP in thermal equilibrium in early universe
• Falls out of equilibrium as universe expands
• Below freeze-out, density of LKP WIMPS per co-moving volume is fixed
For 1 TeV KK, Tf = 40 TeV
Co-annihilation
• eR(1) may substantially affect relic density if
it is close in mass to B(1)
• eR(1) has same interaction efficiency
– freeze-out temp is unaffected
• eR(1) left after freeze-out
– Eventually eR(1) e(0) + B(1)
• Net relic density of B(1) is increased
Relic Density
= scaled mass splitting between eR
(1) and B(1)
= 0.05 = 0.01
h2 = 0.11 0.006 yields for R:
Tait, Servant
… 1 flavor
… 5 flavors
5d range of 600-900 GeV
6d range of 425-625 GeV
B(1) alone
More Complete Calculations
WMAP
Kong, Matchev Burnell, Kribs
Quasi-degenerate KK eL
(1)
Quasi-degenerate KK quarks and gluons
= 0.01 solid 0.05 dashed
Add Gravity in the Bulk
mG1 > mB1 mG1 < mB1
KK graviton decays into B(1)
(mWG = KK scale from relic density
without graviton) Shah, Wagner
Super-WIMPS!
Feng, Rajaraman, Takayama
Direct Detection of LKP
• LKP – nucleon scattering:
Tait, Servant
Localized Gravity: Warped Extra Dimensions
Randall, Sundrum
Bulk = Slice of AdS5
5 = -24M53k2
k = curvature scale
Naturally stablized via Goldberger-Wise
Hierarchy is generated by exponential!
Number of Events in Drell-Yan @ LHC
For this same model embedded in a string theory: AdS5 x S
Kaluza-Klein Modes in a Detector: SM on the brane
Davoudiasl, JLH, Rizzo
Unequal spacing signals curved space
Kaluza-Klein Modes in a Detector: SM off the brane
Fermion wavefunctions in the bulk: decreased couplings to light fermions for gauge & graviton KK states
gg Gn ZZ @ LHC
gg gn tt @ LHC
Agashe, Davoudiasl, Perez, Soni
-
Lillie, Randall, Wang
Issue: Top Collimation
Lillie, Randall, Wang
gg gn tt-
g1 = 2 TeV g1 = 4 TeV
Warped Extra Dimension with SO(10) in the bulk
• Splits families amongst 16 of SO(10) with different Z3 charges: Baryon symmetry in bulk
• Lightest Z-odd particle, R’ KK state, is stable
Agashe, Servant
Gives correct relic density for wide range of masses
Bold-face particles have zero-modes
Cosmic Ray Sensitivity to Black Hole Production
Ringwald, TuAnchordoqui etal
No suppression
Summary of Exp’t Constraints on MD
Anchordoqui, FengGoldberg, Shapere