collider constraints on low mass wimp
DESCRIPTION
Collider Constraints On Low Mass WIMP. Haipeng An, University of Maryland Shanghai Jiao Tong University In collaboration with Xiangdong Ji, Lian-Tao Wang. 中国科学院理论物理研究所冬季研讨会 -- 暗物质与重子物质起源 2010.12.13-15. Outlines. Experiments; - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/1.jpg)
Collider Constraints On Low Mass WIMP
Haipeng An, University of Maryland
Shanghai Jiao Tong UniversityIn collaboration with Xiangdong Ji, Lian-Tao Wang
中国科学院理论物理研究所冬季研讨会-- 暗物质与重子物质起源 2010.12.13-15
![Page 2: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/2.jpg)
Outlines
Experiments;
Possible Interactions Between WIMP and SM particles;
Tevatron Constraints on the parameter space;
Tevatron Constraints on direct detection cross section;
Relic abundance;
Flavor changing neutral currents.
![Page 3: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/3.jpg)
Direct Detection Experiments
CoGeNT
Observed excess could be explained by WIMP signal with mass in the range of 6~11 GeV. Cross section 10-41~10-40 cm2.
CRESST-II
CaWO4 32 events cannot be explained by known background. Can be explained by WIMP with mass around smaller than 15 GeV. And the cross section is about a few times 10-41 cm2 .
XENON100
Poisson smearing, null-result. New XENON100 result with a detecting power ten times larger will be published soon.
![Page 4: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/4.jpg)
Direct Detection Experiments
15 GeV
5 GeV
![Page 5: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/5.jpg)
Relic abundance
Thermal freezing-out
Thermal freezing-in (Multi-components)
SuperWIMP
Asymmetric dark matter
... ...
Using relic abundance as a lower bound
![Page 6: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/6.jpg)
Tevatron Constraints
Leading jet ET > 80 GeV; pT of second jet < 30 GeV; Vetoing any third jet with ET > 20 GeV; Missing ET > 80 GeV. 1 fb-1 of data from Tevatron, 8449 events observed. SM background 8663±332;
Hard process is good enough.
Goodman, Ibe, Rajaraman, Shepherd, Tait, Yu (1005.1286, 1008.1783);
Bai, Fox, Harnik (1005.3797).
Aaltonen et al. [CDF Collaboration], PRL 101, 181602, 2008.Study the properties of large extra dimension
models
![Page 7: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/7.jpg)
Contact Operator
In the work by Irvine group, effective four particle interaction is used to study the Tevatron constraint and LHC prediction.
However, in Tevatron the center-of-mass energy of the proton-anti-proton pair is 1.96 TeV, therefore if the mass of the intermediate particle is around a few hundred GeV, the interaction cannot be considered as a contact interaction.
Furthermore, if the result of CoGeNT is induced by elastic SI, MI collision between dark matter and nuclei, the effective coupling can be written as
![Page 8: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/8.jpg)
Z-boson mediator
MDM << MZ.
Coupling between MZ and DM should be smaller than 0.02.
Relic abundance is too large.
![Page 9: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/9.jpg)
Standard Model Higgs
If dark matter is a fermion, since the Yukawa couplings to light quarks are small. The relic abundance is too large.
However, if dark matter is a scalar, the relic abundance constraint can be avoided. (Xiao-gang’s talk)
![Page 10: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/10.jpg)
Possible Interactions
SM Higgs + Scalar dark matter is still possible.
Dark matter: Complex Scalar (Φ), Dirac Fermion (χ).
Mediator: Scalar (H’), Vector (Z’).
T-channel annihilation, colored particle. (Will be study elsewhere).
More complicated cases …
![Page 11: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/11.jpg)
Vector Mediator with Fermion WIMP
M*
gD=0.5, 1, 2, 3, 5
MZ’ = 5 GeV
![Page 12: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/12.jpg)
Vector Mediator with Fermion WIMP
gD=0.5, 1, 2, 3, 5
430 GeV
450 GeV
480 GeV
500 GeV
Contact operator case
Tevatron constraint
Cannot saturate Tevatron bound in
perturbative region
![Page 13: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/13.jpg)
Vector mediator fermion dark matter
Scalar mediator fermion dark matter
Vector mediator Scalar dark matter
Vector Mediator with Fermion WIMP
5 GeV
15 GeV
![Page 14: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/14.jpg)
Dipole Interaction
Perturbatively
Non-perturbatively
![Page 15: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/15.jpg)
Dipole Interaction
![Page 16: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/16.jpg)
Direct detection cross section
Hadronic matrix elements
Electric Dipole coupling
Belanger, Boudjema, Pukhov, Semenov “MicrOMEGAs2.2” (0803.2360).
Fan, Reece, Wang (1008.1591).
Quark EDM
(QCD sum rules)
Pospelov, Ritz PRD 63, 073015
![Page 17: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/17.jpg)
Power counting
Direct detection cross section
SI: Spin-independent ~ O(1)
SD: Spin-dependent ~ O(10-3~10-4)
MI: Momentum-indenpent ~ O(1)
MD: Momentum-dependent ~ O(10-6)
![Page 18: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/18.jpg)
Magnetic Interaction
![Page 19: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/19.jpg)
Tevatron Constraints on Direct Detection Cross Section
gD=1
gD=0.5
MZ’ < M* constraint on gZ’ does not depend on gD.
σ g∝ D- 2
![Page 20: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/20.jpg)
Tevatron Constraints on Direct Detection Cross Section
MDM=5 GeV
MDM=15 GeV
![Page 21: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/21.jpg)
Relic Abundance
Ωh2 ≈ 0.1pb / σ.
We choose gD=1 as a benchmark scenario to study the relic abundance.
During the thermal annihilation MDM/T ≈ 20, during this era, dark matter particles are non-relativistic.
For some operators the annihilation cross section are suppressed by v2.
JPC Group state of spin-1/2 fermion anti-fermion pair can only be 0-+ and 1--
![Page 22: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/22.jpg)
Tevatron Constraints on Relic Abundance (MZ’>80 GeV)
5 GeV, 7 GeV, 10 GeV, 12 GeV, 15 GeV
![Page 23: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/23.jpg)
Tevatron Constraints on Relic Abundance (MZ’>80 GeV)
NR suppression
Factor of 10
σ M∝ DM2
![Page 24: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/24.jpg)
Dipole coupling (MZ’>80 GeV) Factor of 102
σ M∝ DM4
![Page 25: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/25.jpg)
Scalar Mediator with Fermion DM
![Page 26: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/26.jpg)
Vector Mediator and Scalar DM
![Page 27: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/27.jpg)
Scalar Mediator with Scalar Dark Matter (MZ’>80 GeV)
![Page 28: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/28.jpg)
Different Energy Scales
Collider:
In the case of Mmediator < M*, the mediator is produced on-shell and then decay to DM-anti-DM pair, the energy flowing into the DM anti-DM pair is just Mmediator.
Thermal annihilation:
The energy flowing into Z’ is 2MDM. Therefore, if the coupling is dimensional -1, like the dipole interaction case, the collider constraint on the thermal annihilation cross section is enhanced by a factor of (MDM/MZ’)2. Whereas, if the coupling is dimension 1, like the scalar mediator with scalar dark matter case, the constraint on thermal annihilation cross section is weakened by a factor of (MDM/MH’)2.
![Page 29: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/29.jpg)
LEP II constraints on Z’ coupling to leptons If the MZ’ > 209 GeV, in the case of B-xL model, the constraint on x
is that MZ’/gZ’ > 6.2x TeV.
If MZ’ < 209 GeV, the coupling between Z’ and leptons should be smaller than 10-2.
In the case of gD=1, MZ’=80 GeV, MD=15 GeV, ge=gmu=gtau=0.01, the relic abundance is Ωh2 = 0.58, which is about 5 times larger than the observed one. Since Ωh2 ~ 0.1pb / σ, the contribution of the annihilation cross section from hadronic sector needs to be at least 5 time larger than from the lepton sector.
If gD gets larger, the constraint from thermal relic abundance is weakened.
![Page 30: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/30.jpg)
Possible Interactions at gD=1, Mmediator>80 GeV
Other interactions are either suppressed by velocity or suppressed by MD / MZ’.
Except for the case of scalar mediator and scalar DM, the allowed cases are also stringently constrained.
![Page 31: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/31.jpg)
Flavor Changing Neutral Current Quark rotation matrices can induce tree-level FCNC. In the case of
new scalar mediator.
If the vector mediator is non-universally coupled to quarks, it also suffers from tree-level FCNC constraints.
![Page 32: Collider Constraints On Low Mass WIMP](https://reader033.vdocuments.mx/reader033/viewer/2022061608/568151c8550346895dbffe11/html5/thumbnails/32.jpg)
Summary
We consider elastic, single component, dark matter, specifically, complex scalar and Dirac fermion. The mediator we can considered are vector and real scalar.
In our study, the interaction is conducting by a propagating particle instead of a contact operator.
Collider constraints on the direct detection and relic abundance is studied especially for heavy mediator cases (M>80 GeV, gD=1).