issues in hidden sector dark matter

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Issues in hidden sector dark matter Seungwon Baek (KIAS) Summer Institute 2013 Jirisan National Park, Aug. 17-23, 2013 based on JHEP1202; JHEP1211; JHEP1305 in collaboration with Pyungwon Ko, Wan-Il Park, Eibun Senaha 2013-08-18 Baek, Seungwon

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Issues in hidden sector dark matter . Seungwon Baek (KIAS) Summer Institute 2013 Jirisan National Park, Aug . 17-23, 2013 based on JHEP1202; JHEP1211; JHEP1305 in collaboration with Pyungwon Ko , Wan-Il Park, Eibun Senaha. Outline. - PowerPoint PPT Presentation

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Page 1: Issues in  hidden sector  dark  matter

Baek, Seungwon

Issues in hidden sector dark matter

Seungwon Baek (KIAS)Summer Institute 2013

Jirisan National Park, Aug. 17-23, 2013

based on JHEP1202; JHEP1211; JHEP1305 in collaboration with Pyungwon Ko, Wan-Il Park, Eibun Senaha

2013-08-18

Page 2: Issues in  hidden sector  dark  matter

Baek, Seungwon

Outline

2013-08-18

Hidden sector dark matter with Higgs portal interaction Relic density and direct detection Higgs phenomenology EW precision test Vacuum stability, perturbativity, unitarity bound LHC searches

Conclusions

Page 3: Issues in  hidden sector  dark  matter

Baek, Seungwon

Dark Matter

2013-08-18

27% of the universe is DM We do not know the na-ture of DM

WIMP allows the parti-cle physics explanation of DM and its creation and detection at LHC

One possible WIMP DM scenario is the frame-work of “Hidden Sec-tor” DM

Dark Matter;

26.8

Ordinary Matter;

4.9

Dark Energy;

68.3

Page 4: Issues in  hidden sector  dark  matter

Baek, Seungwon

Hidden Sector DM and Higgs Portal

2013-08-18

DM is singlet under the SM gauge group hidden

Higgs and a singlet scalar can mediate be-tween the SM and hidden sector through renormalizable interaction

SM HS(DM)

Page 5: Issues in  hidden sector  dark  matter

Baek, Seungwon

Other portals

2013-08-18

-portal Babu, Kolda, March-Russel, hep-ph/9710441

-portal Adam Falkowski , Joshua T. Ruderman , Tomer Volansky, arXiv:1101.4936

fermion-portal Yang Bai, Joshua Berger, arXiv:1308.0612

Page 6: Issues in  hidden sector  dark  matter

Baek, Seungwon

Hidden sector DM models with Higgs por-tal

2013-08-18

Singlet Fermionic DM

Vector DM

Page 7: Issues in  hidden sector  dark  matter

Baek, Seungwon

Direct detection

2013-08-18

XENON100(2012)

Page 8: Issues in  hidden sector  dark  matter

Baek, Seungwon

Direct detection

2013-08-18

GIM-type cancellation occurs in direct detection cross section

0 for degenerate Higgs

Page 9: Issues in  hidden sector  dark  matter

Baek, Seungwon

Direct detection

2013-08-18

Exclusion plot by XENON100

gx: DM- coupling Cancellation mecha-

nism works quite ef -ficiently and larger region is allowed by direct detection ex-periments

SB, P. Ko, W.I. Park(2011)

𝑀 𝑋=70𝐺𝑒𝑉

𝑚2=150𝐺𝑒𝑉

Page 10: Issues in  hidden sector  dark  matter

Baek, Seungwon

Comparison with the EFT approach

2013-08-18

SB, P. Ko, W-I. Park, E. Senaha, JHEP(2013)

𝑟1<0.7

Page 11: Issues in  hidden sector  dark  matter

Baek, Seungwon

Higgs Phenomenology

2013-08-18

Higgs sector is extendedHiggs phenomenol-ogy is different from the SM one

SM HS(DM)

Page 12: Issues in  hidden sector  dark  matter

Baek, Seungwon

Higgs Phenomenology

2013-08-18

Invisible decay of Higgs at tree is allowed

Reduction of Higgs signal strength

Hi

X

X

Page 13: Issues in  hidden sector  dark  matter

Baek, Seungwon

Higgs Phenomenology

2013-08-18

Signal strength

If some , our scenario will be excluded

Page 14: Issues in  hidden sector  dark  matter

Baek, Seungwon

EW precision tests

2013-08-18

New contribution to the EW precision obs. Barger, et.al. 2008

Page 15: Issues in  hidden sector  dark  matter

Baek, Seungwon

EW precision tests

2013-08-18

𝛼=20°

𝛼=45°

𝑚2=25𝐺𝑒𝑉

𝑚2=750𝐺𝑒𝑉 𝑚𝐻=720𝐺𝑒𝑉

SB, P. Ko, W-I. Park, E. Senaha, JHEP(2013)

Page 16: Issues in  hidden sector  dark  matter

Baek, Seungwon

Vacuum stability (EW)

2013-08-18

Requiring the global min. of the Higgs poten-tial is at the EW vacuua constrains the param-eters of the Higgs portal

Page 17: Issues in  hidden sector  dark  matter

Baek, Seungwon 2013-08-18

Page 18: Issues in  hidden sector  dark  matter

Baek, Seungwon

Triviality and vacuum stability bound on mH

2013-08-18

The Higgs potential may become unstable before Mpl.

125GeV

Page 19: Issues in  hidden sector  dark  matter

Baek, Seungwon 2013-08-18

Higgs portal model can provide negative con-tribution to the SM-like Higgs.

Lebedev 2012, Joan Elias-Miro, Jose R. Espinosa, Gian F. Giu-dice, Hyun Min Lee, Alessandro Strumia, 2012

Page 20: Issues in  hidden sector  dark  matter

Baek, Seungwon

Triviality and vacuum stability bound

2013-08-18

Page 21: Issues in  hidden sector  dark  matter

Baek, Seungwon

Unitarity bound

2013-08-18

Sin Kyu Kang, Jubin Park, arXiv:1306.6713

Page 22: Issues in  hidden sector  dark  matter

Baek, Seungwon

LHC tests

2013-08-18

𝑟1<0.7

Page 23: Issues in  hidden sector  dark  matter

Baek, Seungwon

LHC tests

2013-08-18

𝑟1>0.7

It will be difficult to produce the 2nd Higgs at the LHC.

Page 24: Issues in  hidden sector  dark  matter

Baek, Seungwon

Conclusions

2013-08-18

DM with Higgs portal provides cancellation to the direct search bound improves the stability of Higgs potential changes the Higgs search at colliders is constrained by EWPT and the discovery of SM-

Higgs boson It will be difficult to produce the 2nd Higgs.

Page 25: Issues in  hidden sector  dark  matter

Baek, Seungwon

Backups

2013-08-18

Page 26: Issues in  hidden sector  dark  matter

Physics of Higgs Portal DM

2013-08-18Baek, Seungwon

Dark matter relic density, direct & indirect detection scalar: C.P. Burgess, Maxim Pospelov, Tonnis ter Veldhuis, hep-ph/0011335 fermion:Yeong Gyun Kim, Kang Young Lee, Seodong Shin, arXiv:0809.2745 vector: Yasaman Farzan, Amin Rezaei Akbarieh, arXiv:1207.4272 Collider phenomenology SB, P. Ko, W-I. Park, E. Senaha, 1112.1847, 1209.4163, 1212.2131 EW precision tests Vacuum stability Perturbativity Unitarity

Page 27: Issues in  hidden sector  dark  matter

Comparison with the EFT approach

2013-08-18Baek, Seungwon

For heavy EFT is a good approximation.S. Kanemura et.al 2010, A. Djouadi, et.al. 2011, O. Lebedev, H. M. Lee, Y. Mambrini, 2011, L. Lopez-Hororez, Schwetz, Zupan 2012

Page 28: Issues in  hidden sector  dark  matter

Comparison with the EFT approach

2013-08-18Baek, Seungwon

SFDM scenario is ruled out in the EFT

A. Djouadi, et.al. 2011

Page 29: Issues in  hidden sector  dark  matter

Baek, Seungwon

EW precision tests

2013-08-18

The S,T,U parameters give strong constraints on the mixing angle α