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14 April, 2009 C. Dallapiccola, MIT Seminar
Mini Black Holes at the LHC as a Signature of Extra Dimensions
Mini Black Holes at the LHC as a Signature of Extra Dimensions
Carlo DallapiccolaUniversity of Massachusetts,
Amherst
14 April, 2009 C. Dallapiccola, MIT Seminar
OutlineOutline
• Introduction - TeV scale gravity and black holes Motivation Theoretical background
• Black Hole signature
• Analysis at LHC - ATLAS Event selection Observation and Limits
14 April, 2009 C. Dallapiccola, MIT Seminar
Why the interest in gravitational interactions in high energy physics?
Why the interest in gravitational interactions in high energy physics?
14 April, 2009 C. Dallapiccola, MIT Seminar
Motivation I: Hierarchy ProblemMotivation I: Hierarchy Problem
• Conventional paradigm: two very disparate fundamental scales in physics
Electroweak Scale (EEW) ≈ 1000 GeV Gravitational Scale ( ) = 1.21019 GeV
16 orders of magnitude difference!
• Striking hierarchy problem that must be some day be addressed -- what is stabilizing this large difference in fundamental scales?
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MPl = hc GN
14 April, 2009 C. Dallapiccola, MIT Seminar
Motivation II: EmpiricalMotivation II: Empirical
• Electroweak interactions have already been probed at length scales 1/EEW we know it’s truly a fundamental scale.
• Gravity has not remotely been probed at length scales 1/MPl = 10-33 cm 31 orders of magnitude smaller than scales at which gravity has been tested (0.01 cm).
• Presumptuous to assume extrapolation of Newton’s Law over these 31 orders of magnitude?
14 April, 2009 C. Dallapiccola, MIT Seminar
A Proposal: TeV Scale GravityA Proposal: TeV Scale Gravity
• Perhaps EEW is the only fundamental scale in physics
Fundamental scale even for gravity: MPl = EEW = 1 TeV At this energy scale, gravitational interactions comparable to weak interactions strong gravity
Radiative stability of electroweak scale is resolved without SUSY, etc. ultraviolet cut-off for the theory is at 1 TeV, where quantum gravity is the new physics
• But then how do we explain where observed Planck Scale comes from (ie. Why is gravity so weak at large distance scales = low energies)? = effective scale, not in fundamental laws
14 April, 2009 C. Dallapiccola, MIT Seminar
Theoretical Framework Theoretical Framework
Geometry of extra spatial dimensions is responsible for this apparent hierarchy
• Observed 3-space = 3-brane on which SM charges and fields are confined/localized.
• Embedded in a D-dimensional bulk = 3+n+1 spacetime dimensions
• Only graviton propagates in the extra dimensions
String theory branes on which some fields (open strings) are confined and others (closed strings) are not prefers n = 7
• Observed 3-space = 3-brane on which SM charges and fields are confined/localized.
• Embedded in a D-dimensional bulk = 3+n+1 spacetime dimensions
• Only graviton propagates in the extra dimensions
String theory branes on which some fields (open strings) are confined and others (closed strings) are not prefers n = 7
14 April, 2009 C. Dallapiccola, MIT Seminar
Theoretical Framework Theoretical Framework
Two popular scenarios:
• Arkani-Hamed, Dimopoulos, Dvali (ADD)*
Large volume of compact (flat) extra dimensions generates the hierarchy gravitational field lines spread through bulk.
• Randall, Sundrum (RS)†
Strong curvature (warping) of small AdS single extra dimension generates the hierarchy gravity localized on a second brane bounding the extra dimension.
* Phys. Lett. B 429, 263 (1998)† Phys. Rev. Lett. 83, 3370 (1999)
Focus on this at ATLAS
14 April, 2009 C. Dallapiccola, MIT Seminar
Compact Extra Dimensions (ADD)Compact Extra Dimensions (ADD)
Matter (SM fields) are localized on a 4-d submanifold (SM brane) of a higher dimensional spacetime (bulk)
Gravitational field not localized propagates in the bulk
The n extra spatial dimensions are compactified at submillimeter length scales R explains why not observed yet
Newton’s Law ( ) becomes:
Looks just like usual (tested) Newton’s Law, with an effective Planck Scale:
€
V r( ) =−m1m2
MDn +2
⋅1
rn +1r << R( )
V r( ) =−m1m2
MDn +2Rn
⋅1
rr >> R( )
€
V r( ) =−m1m2
MDn +2
⋅1
rn +1r << R( )
V r( ) =−m1m2
MDn +2Rn
⋅1
rr >> R( )
€
MPl2 = MD
n +2Rn€
MD =1 TeV€
V = −m1m2 MPl2 r
14 April, 2009 C. Dallapiccola, MIT Seminar
Compact Extra Dimensions: SignaturesCompact Extra Dimensions: Signatures
Gravity “strong” at TeV (MD) scale
• Deviations from Newton’s Law at short distance (torsion-balance “Cavendish” expts.)
• Direct or virtual emission of gravitons by SM particles in accelerator experiments
• Enhanced production of gravitons in early universe and in certain astrophysical processes
• Large cross section for black hole production at TeV collision energies
€
MPl2 = MD
n +2Rn
14 April, 2009 C. Dallapiccola, MIT Seminar
Deviations from Newton’s LawDeviations from Newton’s Law
• Direct tests of deviations from Newton’s Law (torsion-balance “Cavendish” expts.)
n = 1 already ruled out (R = solar system scale!)
n = 2 still viable (R ≈ 10m - 1mm) R < 30m, MD > 4 TeV
n > 2 unconstrained Ex.: MD > 4 GeV for n = 3
14 April, 2009 C. Dallapiccola, MIT Seminar
Astrophysical/Cosmological SignaturesAstrophysical/Cosmological Signatures
• Gravitons compete with other processes in carrying away energy in astrophysical phenomena
• Gravitons decay slowly (~109 yrs. or more) preferentially 2-photon state Gravisstrahlung accelerates supernovae cooling Photons from decays of gravitons produced from supernovae contributes to diffuse cosmic gamma ray background
“Halo” of trapped gravitons around neutron stars source of gamma rays long after supernova
Contribution of gravitons produced early in universe to critical density
Stringent constraints (many assumptions):n > 3 , MD > ~5 TeV
14 April, 2009 C. Dallapiccola, MIT Seminar
Accelerator Signatures: GravitonsAccelerator Signatures: Gravitons
• Graviton momentum in the bulk = Kaluza-Klein (KK) tower of graviton states ~continuum of states due to large size of extra dimensions
• Direct graviton production: Photon + missing E at LEP Photon + missing Et at Tevatron (LHC) Jet + missing Et at Tevatron (LHC)
• Virtual graviton exchange enhancing SM processes Ex.: Sensitive to unknown coupling and ultra-violet cutoff
€
e+e− qq → γG
€
qg → qG
€
e+e− → e+e−
€
qq → γγ l +l −
Reliable constraints (few assumptions):n > 1 , MD > ~1-2 TeV
14 April, 2009 C. Dallapiccola, MIT Seminar
Accelerator Signatures: Black HolesAccelerator Signatures: Black Holes
• At CM energies above Planck scale MD black holes can be produced in particle collisions particles passing within distance smaller than event horizon
• Naively, cross section for partons a and b to form a black hole is “geometric”:
RS is the horizon size, or Schwarzschild radius Depends on which fraction of available parton energy goes into forming the black hole (trapped behind horizon).
Convolute with parton distribution functions to get
• Range of BH masses depends on eff. impact param.
€
σ ab →BH ≈ πRS2
€
ˆ s
€
σ pp →BH
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Holes at the LHCBlack Holes at the LHC
• At LHC (ECM = 14 TeV), cross section may be quite large
• Assume some min. BH mass, below which unknown quantum gravity effects are important and classical BH production is lost
• Use MD = 1 TeV as reference point
• Perspective: Zl+l- + jets = 26 pb
n Min. MBH (TeV) σ (pb)
2 5 40.7
2 8 0.34
4 5 24.3
7 5 22.3
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Hole Search at ATLASBlack Hole Search at ATLAS
• LHC and the ATLAS experiment• ATLAS Black Hole event simulation• Search strategy and predicted discovery thresholds
14 April, 2009 C. Dallapiccola, MIT Seminar
The Large Hadron ColliderThe Large Hadron Collider
Lake Geneva
14 TeV
CMSATLAS
CERN Main Site
• Proton-proton collider circumference = 27 km
• Energy = 7 TeV / beam√s = 14 TeV
• Stored energy / beam = 350 MJ (!)
• Bunch spacing = 25 ns 40 MHz crossing rate
• Design luminosity= 1034 cm-2 s-1
• 100 fb-1 / year
• Number of interactionsper crossing ~23
14 April, 2009 C. Dallapiccola, MIT Seminar
The ATLAS DetectorThe ATLAS Detector
Inner Tracker
EM Calorimeter
Hadronic Calorimeter
Muon Detectors
Diameter 25 mBarrel toroid length 26 mEnd-cap end-wall chamber span 46 mOverall weight 7000 Tons
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Hole ProductionBlack Hole Production
• Collision: gravitational shock waves of ultrarelativistic particles collide complex horizon forms
• Balding: collapse to a more regular “Kerr-Newman” stationary solution asymmetries and moments (hair) shed by emitting bulk gravitons (energy lost)
• Spin down: angular momentum lost via emission of high-spin state particles
• Hawking evaporation: thermal grey-body radiation High temperature: many high pT particles
democratic: rate of SM particle emission according to degrees of freedom no couplings
Isotropic: no preferred direction n dependence: higher T for higher n
Mini black hole
14 April, 2009 C. Dallapiccola, MIT Seminar
BH Evaporation PropertiesBH Evaporation PropertiesParticle multiplicities and missing ET ( and G) for BH events
Particle pT and
LARGE
n = 7
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Hole BackgroundsBlack Hole Backgrounds
• Primary bkgds. are states with high multiplicity and high pT jets, such as ttbar
• Requiring a very high pT charged lepton can greatly reduce bkgd.
14 April, 2009 C. Dallapiccola, MIT Seminar
BH - Bkgd CharacteristicsBH - Bkgd Characteristics
BHs
Bkgd
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Hole Event SelectionBlack Hole Event Selection
• Single jet trigger with 400 GeV threshold: > 99% eff.
• Uniquely identify objects in the event as muon, electron, photon or hadronic jet
• Select events with large scalar sum pT
• Further require at least one lepton with pT > 50 GeV (QCD dijet reduced by additional 103)
€
pT∑ > 2.5 TeV
14 April, 2009 C. Dallapiccola, MIT Seminar
Black Hole SelectionBlack Hole Selection
Missing ET also characteristic (larger than, say, SUSY)
€
pT∑ > 2.5 TeV
14 April, 2009 C. Dallapiccola, MIT Seminar
BH Signal DeterminationBH Signal Determination
Reconstruct BH Mass: Discovery:
€
S B > 5
€
S >10
fb-1
14 April, 2009 C. Dallapiccola, MIT Seminar
Classical BHs: ConclusionClassical BHs: Conclusion
• ATLAS capable of discovering BHs up to kinematic limit of LHC
• 5σ discovery: few pb-1 data if Mthresh = 5 TeV
few fb-1 data if Mthresh = 8-10 TeV• Could be accompanied by bulk graviton signals of
jet/photon + missing energy• Exciting prospect of resolving difficult hierarchy
problem and perhaps even probing quantum gravity!• Determining fundamental params. (MD and n) difficult
But…Relies on:• Large predicted cross-section (many caveats)
• Extrapolations of QCD dijet backgrounds at high pT from TeV scale to 14 TeV scale (could be off by orders of magnitude)
14 April, 2009 C. Dallapiccola, MIT Seminar
Classical BHs: Recent StudiesClassical BHs: Recent Studies
• Better simulation of mass lost during balding phase: as much as 30% of mass could be lost lowers cross section by factor of 5-10.
• Better simulation of effects of BH with spin: effectively higher temp. BH fewer, but higher pT emissions (more jet-like). Also, vector emission enhanced by factor 2-3, at expense of fermions fewer leptons produced.
Will increase amount of integrated luminosity needed for discovery and degrade S/B, but will not significantly diminish ability to observe classical BHs at the LHC
14 April, 2009 C. Dallapiccola, MIT Seminar
Non-Classical RegimeNon-Classical Regime
• Recently argued* that classical BHs at the LHC are unlikely: only valid for MBH >> MD (Mmin introduced) Quantum gravity effects important (and largely unknown) for MBH near the Planck mass
Reasonable criteria is that Compton wavelength of colliding partons are within their Schwarzschild radius or that entropy is sufficiently large: Mmin = 3-4 * MD
• Steeply falling parton distribution functions make it exceedingly difficult to satisify this relation at LHC energies
• Instead, we may see mostly phenomena at quantum gravity regime eg. string balls* P. Meade and L. Randall, J. High Energy Physics 5, 003 (2008)
14 April, 2009 C. Dallapiccola, MIT Seminar
String BallsString Balls
• String theory is one candidate for partial description of quantum gravity Highly-excited string states (string balls) could be produced at the LHC decay thermally (but more jet-like than BHs)
New mass scale introduced string scale (MS < MD) Thus, string ball cross-section higher than that of BHs
Select using cuts on |pT| and jet pT ratios (at least 4 jets)
14 April, 2009 C. Dallapiccola, MIT Seminar
String Balls: Cross Section LimitsString Balls: Cross Section Limits
• Studies: set limits on string-ball cross section for given mass threshold and 100 pb-1 int. luminosity.
At 95% C.L. MS > 4.8 TeV
MS > 1.6 TeV
MD > 2.4 TeV
14 April, 2009 C. Dallapiccola, MIT Seminar
ConclusionConclusion
• The “big” hierarchy problem, addressing the gigantic disparity of the electroweak and gravitational scales, is one of the biggest in fundamental physics
• Extra dimensional theories provide a framework in which the hierarchy problem is replaced by the more tractable problem of how to naturally stabilize the large sizes of the extra dimensions
• The LHC is well-positioned to observe or set stringent limits on the most striking phenomena: mini black hole production, string balls, etc.