Upload
silvia-fisher
View
218
Download
4
Embed Size (px)
Citation preview
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 1
Satyaki
Bhattacharya
Beyond Standard Beyond Standard Model Higgs Model Higgs
Search at LHCSearch at LHC
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 2
* numbers are for barrel
data taking starts 2007
Startup Luminosity 1033 cm-2/s
that is: 10 fb-1 per year
Silicon Tracker15 ( )%T
TT
p p TeVp
2.7% 0.150.5% E
E EE
PbWO4 ECAL
sampling brass HCAL 120
5%E
E E
solenoid4Tesla field
1.0 1.5%@100T
T
pglobal GeV
p
MUON Chambers
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 3
Higgs in Higgs in MSSM MSSM
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 4
MSSM Higgs sector MSSM Higgs sector
01
1
H
H
02
2
H
H
Two Higgs doublets
8 real Higgs fields( 4 complex fields)
3 fields are
gauged away
01
0
0 02
cos sin
sin cos
H
h
0 01 2
0 , ,, , A H H
All masses, and mixing angle are determined by two independent parameters, generally taken as
tan – ratio of vacuum expectation values of the two doubletsMA – mass of pseudoscalar Higgs A
pseudoscalar Higgs
charged Higgs
heavy Higgs
light Higgs
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 5
MSSM Higgs Production MSSM Higgs Production
h production x-sections similar to SM higgs in decoupling regionggh largest
ggH/A most important at low tan
at high tangg/qqHbb dominant for H/A
for H± tttH-bis most important
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 6
CMS Detector: schematic X-sectional view
HCAL
ECAL
TRACKER
h h Two clean electromagnetic clusters(For unconverted photons)
Backgrounds: gg,qq,qgq @low luminosityjet-jet 105 events/sjet+photon 102 events/s2 photon 1 event/12.5sHiggs 1 event/25sh2photon 1 event/10,000s
@low luminosityjet-jet 105 events/sjet+photon 102 events/s2 photon 1 event/12.5sHiggs 1 event/25sh2photon 1 event/10,000s
two photon background
gamma+jet background
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 7
hh mass resolutionmass resolution
=646MeVe
ven
ts/5
0M
eV
mfor 130 GeV Higgs
CMS full detector simulation. Ref: CMS Note 2003/033
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 8
A/HA/H jets + X jets + X
backgrounds: Z/2multijets faking tt and W+jet with W
reduce background by requiring: high pt narrow jet, isolation, b-tag, impact parameter
NLO x-section used
Signal:Production: ggbbH/A and ggH/ADecay: H/A+
MA 500GeV: .Br=0.188pbMA 200GeV: .Br=9.53pb
~15% mass resolution
Higgs signal over total backgroundPythia simulation
Ref: CMS Note 2003/006
Mass can be reonstructed assuming ||
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 9
h discovery @ 30fbh discovery @ 30fb-1-1
Decay branching ratios and searches for h are like SM Higgs
Ref: CMS Note 2003/033
5 discovery with 30 fb-1 possible in this region using h decay
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 10
A/H and HA/H and H± ± Discovery RegionsDiscovery Regions
At large tanAt large tan A/H coupling to A/H coupling to down type fermion is strong and down type fermion is strong and H production with bH production with bb b and H and H decay to decay to become important become important
For charged Higgs associated For charged Higgs associated production with top is dominantproduction with top is dominant
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 11
SummarySummary
• At LHC Higgs mass range between LEP bounds and ~1 TeV can be probed
• Atleast one MSSM Higgs will be found in entire MA-tan plane
• All MSSM Higgs should be visible in large region of the parameter space
• 5 discovery possible with 30 fb-1 in large region of the parameter space
• Few hundred MeV mass resolution for light Higgs from h
cmsdoc.cern.ch/~anikiten/cms-higgs/Higgs Working Group Summary, Les Houches 2004,hep-ph0406152
for more information
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 12
The EndThe End
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 13
Higgs Production in MSSM(details)Higgs Production in MSSM(details)
• H/A production– ggH/A, gg/qqbbH/A– g(AVV)=0 no VBF– At large tanβ
• VBF suppressed for H• g(A/Hbb) enhanced
~90% bbH/A for tanβ>10 and MA>300 GeV
– H SM-like near lower mass limit ( high tanβ, small
MA)VBF significant
• h production– h SM-like for MA>mh
max
• H± productionFor MH±<Mt : tttH±b
For MH±>Mt:
– ggtbH±,H+H-,W±H±
– gbtH±
– qqH±
Higgs couplings with up(u) down(d) fermions and vector bosons (v)
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 14
MSSM Higgs Production (updated from M. Spira)MSSM Higgs Production (updated from M. Spira)
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 15
MSSM Higgs Production (ii)MSSM Higgs Production (ii)
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 16
channels considered for a SUSY Higgschannels considered for a SUSY Higgs• H/h , bb
– H->bb in WH,ttH– h-> in Wh, tth->l
• H/hZZ*/ZZ4l • h/H/A(e/jETeET, jjET
– Including qqH,ttH,WH
• H+from tt• H+, H+tb for MH+
>Mt
• AZh with hbb• A• H/A ij• H±+
~ ~ ~ ~ ~
~
~
~
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 17
A/HA/H jets + X (detailed efficiency) jets + X (detailed efficiency)
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 18
H/A H/A
• ppbbH/A + X with H/A
2soft(ET< 50GeV) b jets
– Use b-tag against Z/* background
– Use central jet veto against tt
Mass resolution 1%, |mH-mA| ~ 2 GeVH/A peaks superimposed
(mass difference can be upto ~ 5.5 GeV)
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 19
CMS Trigger RatesCMS Trigger Rates
CMS total level1 rate is 16 kHz at startupTotal High Level Trigger (HLT) is 100 Hz.
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 20
Extra Slides on Extra Slides on Standard Model Standard Model
HiggsHiggs
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 21
Higgs production at LHCHiggs production at LHCggH
High gluon flux – dominant although loop process
Vector Boson Fusion (VBF)
10% at MH=100GeV
Comparable to gg->H at MH=1 TeV
ttH, bbH,HW,HZ
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 22
Decays and Search StrategyDecays and Search StrategyMH < ~140 GeV
Hbb dominantggHbb : background too large
ttHttbb possible
H–small BR but very clean
MH < ~500 GeV 120-200 GeV
HWW*/WWll(serious t,Wtb background)
200-500 GeVHZZ4l gives highest sensitivity
between 200-500 GeV
MH > ~500 GeVH large, use channels with large BR,
HZZ/WW
VBF x-sec large and can be used
sear
chch
anne
ls
17 April. 2005,APS meeting, Tampa,Florida S. Bhattacharya 23
Discovery reach of CMSDiscovery reach of CMS
• CMS can probe the entire “allowed” mass range
• 5 discovery possible in few months in many channels
Total
HHZZl+l-l+l-HWWll