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May 12, 2004 1 Invisible Higgs at ATLAS Brian Cox, Jeff Forshaw, Rohini Godbole, Irina Nasteva ATLAS UK Physics meeting

Invisible Higgs at ATLAS

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Invisible Higgs at ATLAS. Brian Cox, Jeff Forshaw, Rohini Godbole, Irina Nasteva. ATLAS UK Physics meeting. In some extensions to the Standard Model, the Higgs can decay into invisible final states: SUSY models H χ 0 χ 0 - PowerPoint PPT Presentation

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Page 1: Invisible Higgs at ATLAS

May 12, 2004 1

Invisible Higgs at ATLAS

Brian Cox, Jeff Forshaw, Rohini Godbole, Irina Nasteva

ATLAS UK Physics meeting

Page 2: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 2

MotivationIn some extensions to the Standard Model, the Higgs can decay into invisible final states:• SUSY models H χ0χ0

• models with enlarged symmetry breaking sector (Majoron models) H JJ• Extra dimension models- H mixes with scalar fields arising from gravity propagating in the extra dimensions.

It is possible that H is produced at SM rates, but decays predominantly in its invisible modes:

in some regions of parameter space BR(invisible) ~ 100%

Page 3: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 3

Invisible Higgs signalProduction via vector boson fusion:qq qqVV qqH (where V = W,Z)

• the vector bosons have PT~ mW/2 => H is produced with transverse momentum ~ mW

• jets from quarks have a small scattering angle and are emitted in the high rapidity regions• W,Z have an energy of ~ mH/2 => the tag jets energy is ~ O(TeV)• no colour connection between the quarks – lack of hadronic activity in the central region (rapidity gaps)

The signatures of this process are: Two far forward and backward tagging jets of moderate PT Considerable missing PT in the central region Rapidity gaps

jet

jet

Page 4: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 4

Main backgrounds*• Z + jets associated production (Zjj) where Z νν

• W + jets associated production (Wjj) where W lν and the lepton is undetected

• QCD multi-jet production: QCDjj, QCDjjj + fake missing PT due to particles escaping detection or to semileptonic decays.

* from a study by L. Neukermans and B. Di Girolamo [ATL-PHYS-2003-006]

Page 5: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 5

Analysis[ATL-PHYS-2003-006]

Selection cuts:1) Two tag jets with PT > 40 GeV and |η| < 5.0, separated in

rapidity: |η1 – η2 | > 4.4 , η1.η2 < 02) Invariant mass of the two jets Mjj > 1200 GeV3) Missing PT > 100 GeV4) Lepton veto and jet veto (no jets with PT > 20 GeV between

the tag jets)

The discriminating variable is the azimuthal angle separation of the tag jets ΔΦjj:

• signal – flat azimuthal dependence• background – jets are back-to-back

azimuthal angle cut ΔΦjj < 1 rad

Page 6: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 6

[ATL-PHYS-2003-006]

cut (1) – jet PT and |Δη|

cut (2) – Mjj

cut (3) – missing PT

azimuthal angle cut – ΔΦjj

Page 7: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 7

BFKL pomeron background

rapidity gap

• colour singlet exchange – gluon radiation is suppressed (rapidity gaps)• mimics the invisible Higgs signal when there is large missing PT: from jets lost down the beam pipe, when only some radiation is detected• BFKL pomeron background is potentially larger than QCD background (single gluon exchange):

where y is the rapidity separation and ω is the pomeron intercept ω ~ 1.4

Two jets, back-to-back in Φ, with rapidity gaps

yedt

d ~

t

sy

ˆln

Page 8: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 8

BFKL pomeron measurementsHard colour singlet exchange was measured at the TeVatron and found to agree with BFKL theory: B. Cox, J. Forshaw, L. Lönnblad [hep-ph/9908464]

Gap fraction compared to D0 data:

• gap fractions were calculated from BFKL pomeron exchange• leading logarithmic calculation of BFKL at fixed αs = 0.17• using HERWIG 6.4

Page 9: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 9

Missing PT distribution after cuts (1) - (4)

The BFKL and QCD backgrounds are eliminated by the azimuthal angle cut ΔΦjj < 1 rad (at leading order)

Invisible HiggsBFKLQCDjj

BFKL background in plots is a factor of 2 – 5 smaller than the full LO calculation

Page 10: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 10

NLO contributions to BFKL• Monte Carlos can’t simulate reliably the high-PT and large-angle gluon radiation• this is important for both BFKL and QCD backgrounds – large-angle radiation is detected while the quark jet is lost down the beam pipe

need the next-to-leading order (NLO) contribution to the 2 3 parton scattering process.

NLO will increase backgrounds because of:

• higher cross-sections for hard gluon emission• de-correlated azimuthal angle of the jets (if one jet is lost) => ΔΦjj cut becomes less effective

Page 11: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 11

NLO calculations• gluon radiation in BFKL pomeron exchange is not calculated at next-to-leading order• it is expected to be similar to the NLO contribution to QCD three-jet production (2 3 scattering) • we can look at the NLO contribution to QCD three-jet production and estimate the BFKL background by this

• use NLOJET++ QCD event generator to calculate three-jet cross sections at next-to-leading order with the KT algorithm

Work in progressNo results yet

Page 12: Invisible Higgs at ATLAS

May 12, 2004 Invisible Higgs, I. Nasteva, Manchester 12

Summary and outlook

• a first estimate of leading order BFKL background to the invisible Higgs

• need further analysis to include NLO contributions