searching for dark matter at the lhc - uci particle...
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Searching for Dark Matterat the LHC
Searching for Dark Matterat the LHC
Tongyan LinKICP/UChicago
UCIrvine SeminarFebruary 19, 2014
Tongyan LinKICP/UChicago
UCIrvine SeminarFebruary 19, 2014
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Dark matter, 2014Dark matter, 2014
WIMP MiracleWIMP Miracle
Weak-scale annihilation cross section gets you in the right ballpark to get the right thermal relic abundance
Weak-scale annihilation cross section gets you in the right ballpark to get the right thermal relic abundance
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Dark matter, 2014Dark matter, 2014 Direct detectionDirect detection
Indirect detectionIndirect detection
LUXLUX
FermiFermi
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The LHCThe LHC
● LHC Run 1, 2011-2012– 7 and 8 TeV, combined 25/fb– Higgs discovery!
● 2015-202?– 13-14 TeV, expected 50-100/fb per year– SUSY? Dark matter? Something else?
● LHC Run 1, 2011-2012– 7 and 8 TeV, combined 25/fb– Higgs discovery!
● 2015-202?– 13-14 TeV, expected 50-100/fb per year– SUSY? Dark matter? Something else?
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Why dark matter at LHC?Why dark matter at LHC?
● WIMP miracle?– WIMP miracle suggestive of M ~ 100 GeV – 1 TeV
● Connection with new weak scale physics?– e.g. natural candidate from SUSY
● Complementarity– Cosmic dark matter needs to be
detected more than one way!
● WIMP miracle?– WIMP miracle suggestive of M ~ 100 GeV – 1 TeV
● Connection with new weak scale physics?– e.g. natural candidate from SUSY
● Complementarity– Cosmic dark matter needs to be
detected more than one way!
Indirect detectionIndirect detection
Direct d etectio n
Direct d etectio n
Collider productionCollider production
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Looking for dark matter at the LHC: new directions
Looking for dark matter at the LHC: new directions
● Contact operator, monojets– Assume DM is only new particle relevant at LHC
● Simplified models– Study DM plus
additional mediatorparticles
● Contact operator, monojets– Assume DM is only new particle relevant at LHC
● Simplified models– Study DM plus
additional mediatorparticles
CMS TrackerCMS Tracker
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“Monojet” searches“Monojet” searches
Contact operator limit: all new physics at high scale (related to
M*), not accessible
Contact operator limit: all new physics at high scale (related to
M*), not accessible
● Simple relation between collider, direct detection, and relic abundance
● Systematic study of contact operators coupled to quarks, gluons, etc.
● Simple relation between collider, direct detection, and relic abundance
● Systematic study of contact operators coupled to quarks, gluons, etc.
Assume also that DM is a SM gauge singletAssume also that DM is a SM gauge singlet
e.g. Goodman et al., Beltran et al.Fox, Harnik, Kopp, Tsai
e.g. Goodman et al., Beltran et al.Fox, Harnik, Kopp, Tsai
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MonojetsMonojets
MET > 350, 500 GeVMET > 350, 500 GeV
ATLAS monojet eventATLAS monojet event
Z+jetsZ+jets
Note: 8 TeV / CMS searches allow more than one hard jet.
Note: 8 TeV / CMS searches allow more than one hard jet.
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ChoicesChoices● Fermion/Scalar,
Real/Complex
● Lorentz structure
● Quarks, gluons
● Fermion/Scalar,Real/Complex
● Lorentz structure
● Quarks, gluons
Goodman, Ibe, Rajaraman, Shepherd, Tait, YuGoodman, Ibe, Rajaraman, Shepherd, Tait, Yu
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LimitsLimits
Constraints for operators are not very sensitive to specific tensor structureConstraints for operators are not very sensitive to specific tensor structure
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Only some are relevant fordirect detection →
Spin-independent
Spin-dependent
Only some are relevant fordirect detection →
Spin-independent
Spin-dependent
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The LHC vs. direct detectionThe LHC vs. direct detection
Cost: ~$10 billion vs. ~$10 million (LUX)Cost: ~$10 billion vs. ~$10 million (LUX)Effective for low massEffective for low mass
Effective vs. spin-dependentEffective vs. spin-dependent
BUT, there will be important modifications to this story...BUT, there will be important modifications to this story...
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The mono-something fieldThe mono-something field
● Mono-photon● Mono-W/Z● Mono-quark vs. mono-gluon● Mono-b, mono-top● Mono-higgs
● Razor analysis
● NLO corrections
● Mono-photon● Mono-W/Z● Mono-quark vs. mono-gluon● Mono-b, mono-top● Mono-higgs
● Razor analysis
● NLO corrections
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Mono-bMono-b
Production mechanisms for b-quarks plus MET:Production mechanisms for b-quarks plus MET:
Small b-quark pdf/production is made up by large couplings to b-quarks.Small b-quark pdf/production is made up by large couplings to b-quarks.
Scalar operator with MFV form of coupling to quarks
Scalar operator with MFV form of coupling to quarks
TL, Kolb, Wang, 1303.6638TL, Kolb, Wang, 1303.6638
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LHC “mono-b” searchLHC “mono-b” search
W/Z + jetsW/Z + jets
topstops
b-enriched final state: improve on monojet analysis by requiring a b-tag (~60-70% efficiency). Also cuts backgrounds significantly.
b-enriched final state: improve on monojet analysis by requiring a b-tag (~60-70% efficiency). Also cuts backgrounds significantly.
ATLAS analysis of 8 TeV data in progress.
ATLAS analysis of 8 TeV data in progress.
This is a new signal region!This is a new signal region!
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Projected limits for 8 TeV runProjected limits for 8 TeV run
Spin-independent scattering:Spin-independent scattering:
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tops + MET searchtops + MET search
● Factor of ~10 larger than b production● Unlike monojets, tt+XX signal not from ISR● Projection – recast limits from SUSY stop search
● Factor of ~10 larger than b production● Unlike monojets, tt+XX signal not from ISR● Projection – recast limits from SUSY stop search
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14 TeV projections14 TeV projectionsFor MFV couplings of DM to quarks, DM+heavy quark searches have sensitivity for CDMS/CoGeNT preferred region
For MFV couplings of DM to quarks, DM+heavy quark searches have sensitivity for CDMS/CoGeNT preferred region
Cotta, Rajaraman, Tait, WijangcoCotta, Rajaraman, Tait, Wijangco
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mono-Higgs (Higgs + MET)mono-Higgs (Higgs + MET)
Petrov and Shepherd 2013Carpenter, DiFranzo, Mulhearn, Shimmin, Tulin, Whiteson 2013Berlin, TL, Wang, to appear
Petrov and Shepherd 2013Carpenter, DiFranzo, Mulhearn, Shimmin, Tulin, Whiteson 2013Berlin, TL, Wang, to appear
Graphic from William ShepherdGraphic from William Shepherd
Found SM-like Higgs!
Potential for a new signal channel for probing dark matter couplings?
See also: Higgs invisible decay
Found SM-like Higgs!
Potential for a new signal channel for probing dark matter couplings?
See also: Higgs invisible decay
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mono-Higgs channelsmono-Higgs channels
LHC Run 1, Combined 7+8 TeV, 25/fbLHC Run 1, Combined 7+8 TeV, 25/fb
V+H searchV+H search
Carpenter et al. 1312.2592Carpenter et al. 1312.2592
Limit setting with 8 TeV data:Limit setting with 8 TeV data: A new, clean signal channel for 14 TeV?A new, clean signal channel for 14 TeV?
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mono-Higgs in EFTmono-Higgs in EFT
See also: Chen, Kolb, Wang; Fedderke, Kolb, TL, WangSee also: Chen, Kolb, Wang; Fedderke, Kolb, TL, Wang
Dimension 7, fermion DMDimension 7, fermion DM
Dimension 8, scalar or fermion DM
Dimension 8, scalar or fermion DM
Operators where dominant production is through mono-Higgs?
Operators where dominant production is through mono-Higgs?
Dimension 6, fermion DMDimension 6, fermion DM
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mono-Higgs in EFTmono-Higgs in EFT
Dimension 7, fermion DMDimension 7, fermion DM
Dimension 8, scalar or fermion DM
Dimension 8, scalar or fermion DM
Operators where dominant production is through mono-Higgs?
Operators where dominant production is through mono-Higgs?
Dimension 6, fermion DMDimension 6, fermion DM
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Naive limit >200 GeV!?Naive limit >200 GeV!?
8 TeV, bb8 TeV, bb
8 TeV, diphoton8 TeV, diphoton
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Distribution of momentum transfer Qtr skewed towards very large values
Distribution of momentum transfer Qtr skewed towards very large values
Imposing “unitarity” conditions on QtrImposing “unitarity” conditions on Qtr
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Validity of EFTValidity of EFT
Busoni, de Simone, Morgante, Riotto + Gramling et al.Busoni, de Simone, Morgante, Riotto + Gramling et al.
EFT limits conservative, in some sense
EFT limits conservative, in some sense
● Putting cuts on Qtr doesn't fully address the question.● Putting cuts on Qtr doesn't fully address the question.
In general, many events violate unitarity
In general, many events violate unitarity
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Limitations of MonojetsLimitations of Monojets
Slide from Haipeng AnSlide from Haipeng An
Light mediators Light mediators
On-shellproductionof Z'
On-shellproductionof Z'
XX
XX
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Simplified Models: s-channelSimplified Models: s-channel
An, Ji, Wang; Cotta et al,Goodman and Shepherd, etcAn, Ji, Wang; Cotta et al,Goodman and Shepherd, etc
● s-channel mediator, SM singlet
● Basic data:
● s-channel mediator, SM singlet
● Basic data:
coupling to quarkscoupling to quarks
mediator massmediator mass
dark matter massdark matter mass
coupling to dark mattercoupling to dark matter
Away from the contact operator limit, there may be a new “mediator” particle accessible at colliders.
Away from the contact operator limit, there may be a new “mediator” particle accessible at colliders.
XX
XX
For EFT limit, coupling needs to be large.For EFT limit, coupling needs to be large.
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Lessons from Z' studiesLessons from Z' studies
Dijet resonance searchesDijet resonance searches
Alves, Profumo, Queiroz Alves, Profumo, Queiroz
Relative strength of dijet vs. monojet depends on Z' branching to visible or invisible final states
Relative strength of dijet vs. monojet depends on Z' branching to visible or invisible final states Monojet limitsMonojet limits
CouplingZ' m
ass
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Simplified Models: t-channel (flavored dark matter)
Simplified Models: t-channel (flavored dark matter)
● t-channel mediator, charged underSM gauge group
● Basic data:
● t-channel mediator, charged underSM gauge group
● Basic data:
An et al., Chang et al., Bai and Berger, DiFranzo et al.,
An et al., Chang et al., Bai and Berger, DiFranzo et al.,
couplingcoupling
mediator massmediator mass
dark matter massdark matter mass
top-flavored dark mattertop-flavored dark matter
XX
XX
Batell, TL, Wang, 1309.4462Batell, TL, Wang, 1309.4462
Stability from flavor, UV completion in MFV SUSYStability from flavor, UV completion in MFV SUSY
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There are many more examplesThere are many more examples
LHC constraints more important for Majorana DM
LHC constraints more important for Majorana DM
Pair production, associated production of mediator.
Kinematics not exactly the same as squarks.
Pair production, associated production of mediator.
Kinematics not exactly the same as squarks.
Slide from Spencer ChangSlide from Spencer ChangSee also: Papucci, Vichi, ZurekSee also: Papucci, Vichi, Zurek
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mono-Higgs – a simplified model?mono-Higgs – a simplified model?
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mono-Higgs – a simplified model?mono-Higgs – a simplified model?
Pseudoscalar of Type II two-Higgs doublet modelPseudoscalar of Type II two-Higgs doublet model
Model with resonant production of Z':Model with resonant production of Z':
Avoid dilepton resonance constraintsAvoid dilepton resonance constraints Z – Z' mass mixingZ – Z' mass mixing
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Constraints on modelConstraints on model● Z-Z' mass mixing
● Limits on dijet resonances
- Important at lowtanβ, large MZ'
● Z-Z' mass mixing
● Limits on dijet resonances
- Important at lowtanβ, large MZ'
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Higgs + METHiggs + MET
Z' → hZZ' → hZ
Z' → hAZ' → hA
● Two sources:
– Z' → hA, A → XX(with 100% BR)
– Z' → hZ, Z → vv
● mA, mH > 300 GeV
● Alignment limit (h has SM couplings to fermions)
● Two sources:
– Z' → hA, A → XX(with 100% BR)
– Z' → hZ, Z → vv
● mA, mH > 300 GeV
● Alignment limit (h has SM couplings to fermions)
AssumptionsAssumptions
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Higgs + MET(Subject to constraints on coupling)
Higgs + MET(Subject to constraints on coupling)
Allowed coupling increases with large MZ', small tanß
Allowed coupling increases with large MZ', small tanß
Z' → hZZ' → hZ
Z' → hAZ' → hA
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Higgs + MET(Subject to constraints on coupling)
Higgs + MET(Subject to constraints on coupling)
Allowed coupling increases with large MZ', small tanß
Allowed coupling increases with large MZ', small tanß
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Coupling to dark matterCoupling to dark matter
● Singlet-doublet model
has fermion DM coupling to pseudoscalar A
- A → XX dominates- Can satisfy LUX
● Singlet-doublet model
has fermion DM coupling to pseudoscalar A
- A → XX dominates- Can satisfy LUX
Preliminary
Study in progress. Model may also be interesting beyond mono-Higgs.
Study in progress. Model may also be interesting beyond mono-Higgs.
Bino-Higgsino in the MSSM, but parameter space more narrowly defined.
Bino-Higgsino in the MSSM, but parameter space more narrowly defined.
See also: Cohen et al.Cheung and Sanford.
See also: Cohen et al.Cheung and Sanford.
MD
MS
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theorists & experimentalists wanted!
theorists & experimentalists wanted!
The road from monojetsThe road from monojets
● EFT framework● Many operators!
– Mono-something
● Simplified models with mediators– Z', t-channel– Need to develop
dedicated analyses
● More to do...
● EFT framework● Many operators!
– Mono-something
● Simplified models with mediators– Z', t-channel– Need to develop
dedicated analyses
● More to do...
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39
Conclusions and OutlookConclusions and Outlook
● New signal regions– Mono-b– Mono-h (diphoton) plus MET– Different kinematic regions
● New models– Not just SUSY-like, though SUSY models/searches
are a good place to start
● Many opportunities with next LHC run● We need to keep looking!
● New signal regions– Mono-b– Mono-h (diphoton) plus MET– Different kinematic regions
● New models– Not just SUSY-like, though SUSY models/searches
are a good place to start
● Many opportunities with next LHC run● We need to keep looking!