Transcript
Page 1: Randall- Sundrum Gravitons and Black Holes at the LHC

Randall- Sundrum Gravitons and Black Holes

at the LHC

Kevin Black

Harvard University

For the ATLAS and CMS Collaborations

Page 2: Randall- Sundrum Gravitons and Black Holes at the LHC

Outline

TeV Scale Gravity Gravitons Black Holes Summary

Landsberg

Page 3: Randall- Sundrum Gravitons and Black Holes at the LHC

State of the Standard Model

Effective model which describes data well

Accommodates but does not explain Fermion masses CP-Violation

Well known fine-tuning, hierarchy, triviality problems

LEP EWWG – Winter 2007

mH2 ~ ~

MPl2

Page 4: Randall- Sundrum Gravitons and Black Holes at the LHC

Why Gravity at the LHC View Standard Model as

effective theory as a low energy approximation

New theory takes over at energy scale comparable to the Higgs mass 1 TeV SUSY, Technicolor, Little

Higgs, .. Perhaps there is no other

scale , GUT scale is ~ TeV Gravity made strong by extra

dimensions where gravity propagates

Page 5: Randall- Sundrum Gravitons and Black Holes at the LHC

Randall – Sundrum Model SM fields on one of two

4-dimensional brane in a 5-D space time

Graviton can propagate in the bulk

Kaluza-Klein States on the order of TeV

Main parameters: Mass of Graviton Curvature parameter

( c = k/Mpl) Signatures in dilepton,

diboson, dijet final states

wk = MPl e-kr

q

q

l

l

Page 6: Randall- Sundrum Gravitons and Black Holes at the LHC

Current Direct Limits

CDF Conference note 9160 PRL 100, 091802 (2008)

Mass limits from 300 – 900 GeV depending on coupling

Page 7: Randall- Sundrum Gravitons and Black Holes at the LHC

Dimuon Signature Two reconstructed muons

One || < 2.1 One with PT > 24 GeV

Use angular distribution to discriminate spin

Main background SM Drell-Yan

c = 0.01c = 0.02c = 0.05c = 0.10

10 fb-1

100 fb-1

300 fb-1

See Dilepton Talk Later this session

Page 8: Randall- Sundrum Gravitons and Black Holes at the LHC

Diphotons

Branching ratio twice as large as dilepton

Z’ doesn’t decay into diphotons Backgrounds

Direct Diphoton Production Photon + Jet Dijets (photon misidentification) Drell-Yan (missing tracks)

Two isolated photons with ET > 150 GeV Isolated both by calorimeter and

tracker

Page 9: Randall- Sundrum Gravitons and Black Holes at the LHC

Dijets

Two jets | Fit invariant mass (leading 2 jets) Compare observed/predicted Including Systematics

Jet Energy Scale Jet Resolution Trigger Prescales Radiation

See Dijets talk later this session…

Page 10: Randall- Sundrum Gravitons and Black Holes at the LHC

Black Holes

Dimopolous, Landsberg Black holes could form if

two colliding partons have impact parameter smaller than RS

Partonic Cross-Section given by geometry, total cross-section convoluted with PDFS

Decay by Hawking Radiation Demographic Decay Spherically Symmetric

E/2

E/2b

b < Rs(E) BH forms

RS2

Page 11: Randall- Sundrum Gravitons and Black Holes at the LHC

Black Holes – Generator Studies

CATFISH Collider

grAviTational FIeld Simulator for black Holes

Comput.Phys.Commun.177:506-517,2007

Page 12: Randall- Sundrum Gravitons and Black Holes at the LHC

Black Hole – CMS I Parameters

Plank Scale 2 TeV Black Holes 4 – 10 TeV

Signature high sphericity high ΣpT high multiplicity

Backgrounds tt, W/Z + jets, Diboson,

multijets Selection

MBH(reco) > 2 TeV Multiplicity > 4 Sphericity < 0.28

Page 13: Randall- Sundrum Gravitons and Black Holes at the LHC

Black Hole – CMS II

Page 14: Randall- Sundrum Gravitons and Black Holes at the LHC

ATLAS Black Holes Event Selection

Electron or muon with ||pT > 50 GeV Two approaches (almost identical results)

|pT| > 2.5 TeV (jets + leptons) At least 4 jets and lepton pT > 200 GeV

A n=2,m = 5-14 TeV

C n=2,m = 8-14 TeV

B n=4,m = 5-14 TeV

D n=7,m = 8-14 TeV

ABCD

Page 15: Randall- Sundrum Gravitons and Black Holes at the LHC

ATLAS Black Holes 2

Reconstruct the visible mass of the black hole from all objects and MET

Very dramatic signature + large signal cross-sections

Page 16: Randall- Sundrum Gravitons and Black Holes at the LHC

ATLAS Black Holes 3

Investigated Event Shapes Do give separation with

background Very different for different

parameters

Page 17: Randall- Sundrum Gravitons and Black Holes at the LHC

ATLAS Black Holes 4

Discovery potential S/B > 5 S > 10

Discovery possible ranging from Few pb for 5 TeV ~1 fb for 9 TeV

Page 18: Randall- Sundrum Gravitons and Black Holes at the LHC

Summary

Signatures from Gravitons and Black Holes would be dramatic compelling signatures

RS Gravitons should be observable ~5 TeV range and quickly observable for ~1 TeV masses

Black holes could be seen to very high masses (8-9 TeV) with a few to ~ 30 fb-1 of data (depending on parameters)

For older results go to ATLAS and CMS exotics pages

New ATLAS results expected to be made public ~few months…

Page 19: Randall- Sundrum Gravitons and Black Holes at the LHC

Backup

Page 20: Randall- Sundrum Gravitons and Black Holes at the LHC

Graviton Signatures at the LHC

Gravitons couple to momentum tensor (contribute to most SM processes)

Monojets Single Vector Boson

production Dilepton/Dijet/Diboson

production As resonance As non-resonant

modification to SM cross-section

q

q

g

g

g

G

g

G

q

q G

V q

q G

V

q

q

l

l

q

q

V

V

Page 21: Randall- Sundrum Gravitons and Black Holes at the LHC

Backup Dimuon I

Signal Cross-Sections

Drell-Yan Backgrounds – others on ~ 10 to 40 times smaller

Page 22: Randall- Sundrum Gravitons and Black Holes at the LHC

Dimuon Backup II

Page 23: Randall- Sundrum Gravitons and Black Holes at the LHC

Dimuon Backup III

Page 24: Randall- Sundrum Gravitons and Black Holes at the LHC

Dimuon backup 4

Systematics Theory QCD and EW Scale – 13-17% PDF – 7%

Systematics Experiment Misalignment Pileup - negligible Background Shape – 10-15% shift in signficance Trigger –negligible (normalizations float in fit) Magnetic Field – negligable

Page 25: Randall- Sundrum Gravitons and Black Holes at the LHC

Dimuon Backup 5

C = 0.01

C= 0.1

Solid line – idealDotted – long term alignmentDashed – “first alignment”

Page 26: Randall- Sundrum Gravitons and Black Holes at the LHC

Diphoton Backup IDiphoton production

Photon + Jet

Dijet

Drell-Yan

Page 27: Randall- Sundrum Gravitons and Black Holes at the LHC

Diphoton Backup II

Page 28: Randall- Sundrum Gravitons and Black Holes at the LHC

Diphoton Backup III

Page 29: Randall- Sundrum Gravitons and Black Holes at the LHC

Diphoton Backup 4Hard Process Scale PDF Uncertainties

Page 30: Randall- Sundrum Gravitons and Black Holes at the LHC

Dijet Backup

Page 31: Randall- Sundrum Gravitons and Black Holes at the LHC

Sezen Sekmen SUSY 07

Page 32: Randall- Sundrum Gravitons and Black Holes at the LHC

Sezen Sekmen SUSY 07

Page 33: Randall- Sundrum Gravitons and Black Holes at the LHC

CMS Black Hole Backup

Sphericity

PDF Uncertainties :

Uncertainty on Signficance ~ 12%

Page 34: Randall- Sundrum Gravitons and Black Holes at the LHC

Black Hole Backup

CMS TDR -2006

Page 35: Randall- Sundrum Gravitons and Black Holes at the LHC

Atlas Black Hole backup

As a function of black hole threshold


Recommended