Higgs and SUSY at future colliders

Slides:



Advertisements
Similar presentations
Exploration without Map - Lepton-Flavor Violation in LHC era - 1st Open Meeting of the SuperKEKB Collaboration KEK, Japan, December 2008 J.HISANO.
Advertisements

Higgs Boson Mass In Gauge-Mediated Supersymmetry Breaking Abdelhamid Albaid In collaboration with Prof. K. S. Babu Spring 2012 Physics Seminar Wichita.
Comprehensive Analysis on the Light Higgs Scenario in the Framework of Non-Universal Higgs Mass Model M. Asano (Tohoku Univ.) M. Senami (Kyoto Univ.) H.
1 SUSY and B physics observables Yasuhiro Okada (KEK) Super B Factory Workshop in Hawaii, April 20, 2005.
Minimal Supersymmetric Standard Model (MSSM) SM: 28 bosonic d.o.f. & 90 (96) fermionic d.o.f. SUSY: # of fermions = # of bosonsN=1 SUSY: There are no particles.
.. Particle Physics at a Crossroads Meenakshi Narain Brown University.
Big Questions, L(H)C Answers Jonathan Feng UC Irvine LC/LHC Workshop, Fermilab 13 December 2002.
Paris 22/4 UED Albert De Roeck (CERN) 1 Identifying Universal Extra Dimensions at CLIC  Minimal UED model  CLIC experimentation  UED signals & Measurements.
Mitsuru Kakizaki (University of Toyama)
SUSY Dark Matter Collider – direct – indirect search bridge. Sabine Kraml Laboratoire de Physique Subatomique et de Cosmologie Grenoble, France ● 43. Rencontres.
Physics Session Summary Nobuchika Okada Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK) TILC09, Tsukuba,
Center for theoretical Physics at BUE
1 Electroweak Baryogenesis and LC Yasuhiro Okada (KEK) 8 th ACFA LC workshop July 12, 2005, Daegu, Korea.
Low scale gravity mediation in warped extra dimensions and collider phenomenology on sector hidden sector LCWS 06, March 10, Bangalore Nobuchika.
Takehiro Nabeshima University of Toyama ILC physics general meeting 9 jun Phenomenology at a linear collider in a radiative seesaw model from TeV.
Wednesday, Apr. 23, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #24 Wednesday, Apr. 23, 2003 Dr. Jae Yu Issues with SM picture Introduction.
Supersymmetric Models with 125 GeV Higgs Masahiro Yamaguchi (Tohoku University) 17 th Lomonosov Conference on Elementary Particle Physics Moscow State.
DARK MATTER CANDIDATES Cody Carr, Minh Nguyen December 9 th, 2014.
1 Summary talk for ILC Physics Yasuhiro Okada (KEK) November 12, 2004 ACFA LC7, Taipei.
Dark matter in split extended supersymmetry in collaboration with M. Quiros (IFAE) and P. Ullio (SISSA/ISAS) Alessio Provenza (SISSA/ISAS) Newport Beach.
ILC Physics a theorist’s perspective Koji TSUMURA (Kyoto from Dec 1 st ) Toku-sui annual workshop 2013 KEK, Dec , 2013.
1 Supersymmetry Yasuhiro Okada (KEK) January 14, 2005, at KEK.
Low scale supergravity mediation in brane world scenario and hidden sector phenomenology Phys.Rev.D74:055005,2006 ( arXiv: hep-ph/ ) ACFA07 in Beijing:
1 ILC の物理 岡田安弘 (KEK) ILC 測定器学術創成会議 2006年6月28日 KEK.
22 December 2006Masters Defense Texas A&M University1 Adam Aurisano In Collaboration with Richard Arnowitt, Bhaskar Dutta, Teruki Kamon, Nikolay Kolev*,
1 Prospect after discoveries of Higgs/SUSY Yasuhiro Okada (KEK) “Discoveries of Higgs and Supersymmetry to Pioneer Particle Physics in the 21 st Century”
1 Higgs Physics Yasuhiro Okada (KEK) November 26, 2004, at KEK.
The Search For Supersymmetry Liam Malone and Matthew French.
1 Overview of physics RDR and the next step Yasuhiro Okada (KEK/Sokendai) March 3, 2008 TILC08, Sendai, Japan.
1 ILC Physics DCR Yasuhiro Okada (KEK) on behalf of the editors for DCR Physics Part, Abdelhak Djouadi, Joe Lykken, Klaus Moenig,Yasuhiro Okada, Mark Oreglia,
DIS2003 A.Tilquin Searches for Physics Beyond the Standard Model at LEP What is the Standard Model Why to go beyond and how Supersymmetry Higgs sector.
Report on model separation Masaki Asano (Tohoku U.) The 12th general meeting of the ILC physics working group.
February 12, 2003ACFA LC Symposium 1 JLC Physics Yasuhiro Okada (KEK) ACFA LC Symposium February 12, 2003,Tsukuba, Japan.
新学術領域研究 先端加速器LHCが切り拓くテラスケールの素粒子物理学 ~真空と時空への新たな挑戦~ 研究会 2013年5月23日〜25日
Charged Higgs boson decay in supersymmetric TeV scale seesaw model
Origin of large At in the MSSM with extra vector-like matters
Phenomenology of Three-Loop Neutrino Masses Models
Journées de Prospective
Physics Overview Yasuhiro Okada (KEK)
Grand Unified Theories and Higgs Physics
MSSM4G: MOTIVATIONS AND ALLOWED REGIONS
Cosmology study at CEPC/SppC on behalf of the TeV cosmology working group Bi Xiao-Jun (IHEP)
Collider Phenomenology of SUSY Cosmic Connections &
Exploring SUSY models through quark and lepton flavor physics
Some Implications Of The Recent LHC Higgs Search Results Xiao-Gang He (SJTU&NTU) Xiao-Gang He and German Valencia, arXiv: Xiao-Gang He and.
ILC and future high energy physics
Lepton Flavor Violation
Searching for SUSY in B Decays
New Physics from B decays
Electroweak Baryogenesis and LC
Exploring SUSY breaking mechanism with B decays
Phenomenology of SUSY Models with Non-universal Sfermions
mSUGRA SUSY Searches at the LHC
Yasuhiro Okada (KEK/Sokendai) October 18, 2007
Physics at a Linear Collider
非最小超对称唯象研究: 工作汇报 杨 金 民 中科院 理论物理所 南开大学.
CEPC-Physics Workshop
Yasuhiro Okada (KEK) FPCP 2004, Deagu, Korea October 7, 2004
Physics beyond the SM in Kaon decays --Theory--
Physics Overview Yasuhiro Okada (KEK)
Yasuhiro Okada (KEK) April 17, 2003, CAT, Indore, India
Searching for New Physics in muon lepton flavor violating processes
Lepton Flavor Violation
Physics Overview Yasuhiro Okada (KEK)
SUSY SEARCHES WITH ATLAS
ILC Physics DCR Yasuhiro Okada (KEK)
SUSY and B physics observables
Theoretical Status of LFV and Rare Tau decays
Can new Higgs boson be Dark Matter Candidate in the Economical Model
Prospect after discoveries of Higgs/SUSY
Presentation transcript:

Higgs and SUSY at future colliders Yasuhiro Okada (KEK) Hiroshima Univ. January 17, 2006

Why TeV?, Why New Physics? LHC will start in the next year, which will explore TeV scale physics. Main objectives are Higgs physics and search for New physics. These two are closely related because the dynamics behind the electroweak symmetry breaking is “New Physics”.

Other reasons to believe physics beyond the Standard Model Neutrino masses Dark Matter Baryon number in the Universe. Solutions to these questions may or may not lie in the TeV region.

Contents of this talk (1) Higgs Physics (2) Supersymmetry (3) Dark Matter and collider physics.

(1) Higgs Physics Finding the mass-generation mechanism for gauge bosons, quarks and leptons the most urgent question of the present particle physics. Discovery of the Higgs boson is the first step (1) Discovery of a Higgs boson (2) Higgs coupling measurements. (3) Physics behind the EW symmetry breaking

Higgs mass Large Higgs mass  Large self-coupling  Strong dynamics If we require that the SM is valid up to 10^19 GeV,

Higgs mass in SUSY models SUSY models include at least two Higgs doublets. In the minimal SUSY Standard Model (MSSM), the lightest CP-even Higgs boson mass has theoretical upper bound. Possible vacuum instability is saved by supersymmetry.

Possible range of the lightest Higgs boson mass for the Planck scale cutoff As long as theory behaves weakly-coupled up to the Planck scale, the Higgs bosom mass is les than ~200 geV.

Precision EW test and the Higgs Mass In the SM, the global fit suggests a light Higgs boson. M.Peskin and J.Wells mt=174.3+-5.1GeV mh=100,200,300,500,1000 GeV Additional new physics is needed to accommodate a heavy Higgs boson.

Higgs search at LHC LHC: 2007 14 TeV pp collider Discovery of the Higgs boson is a main target. Higgs boson search depends on the Higgs boson mass Production: gluon fusion, WW fusion Decay: decay to heavier particles if kinematically allowed. p p W gluon Higgs boson Higgs boson W p gluon p

SM Higgs boson decay branching ratios Higgs discovery at ATLAS At LHC, a SM-like Higgs boson can be discovered independent of its mass.

ILC (International Linear Collider) Highest energy e^+e^- collider   500 GeV (1st stage) -> ~ 1 TeV (2nd stage) High luminosity, 10^34/cm^2/s     (~10^5 light Higgs boson =Higgs factory Startin mid-2010’s 

Higgs physics at ILC Determination of spin and parity. Precise mass determination . Detection of the Higgs boson independent of its decay property. (Recoil mass distribution in the HZ mode) Coupling measurement -> Mass generation mechanism of elementary particles. TESLA TDR GLC report

Higgs coupling LHC 0(10)% for ratio of the coupling constants ILC A few % for absolute values of various coupling

Indirect constraint on the heavy Higgs boson mass in MSSM Direct search at LHC Direct search at 1TeV LC ACFA Higgs WG S. Kiyoura, et al ACFA report

SUSY loop contributions to the hbb Yukawa coupling B(h->bb)/B(h->tt) is sensitive to the SUSY loop correction to the bottom Yukawa coupling for a large tanb region. B(h->bb)/B(h->tt) nomalized by SM value LC LHC K.S.Babu, C.Kolda: M.Carena, D.Garcia, U.Nierste, C.E.M.Wagner J.Guasch, W.Hollik,S.Penaranda

Higgs self-coupling measurement Access to the Higgs potential. Precision at 1/ab for 120 GeV Higgs boson ~20% for 500GeV ILC ~10% for 1 TeV ILC Y.Yasui, et al, LCWS 02

Electroweak baryogenesis and Higgs potential First order phase transition Extension of the Higgs sector The Higgs potential at zero temperature is also modified. => Self coupling measurement Model with dim 6 potential 2HDM S.Kaenmura, Y. Okada, E.Senaha C.Grojean,G.Servant, J.D.Wells

Higgs and physics beyond the SM Even if one Higgs doublet model is a good description, What is f? What physics determines –m^2? What physics determines l? Different scenarios provides different answers. SUSY, String Theory Composite model, Little Higgs model TeV scale extra dimension

Composite model ~10 TeV a SUSY GUT Gravity Gauge force Extra dimension Various new physics signals are expected in the TeV region, depending on different signals.

(2) Supersymmetry Symmetry between bosons and fermions Discovery of SUSY is a revolution of physics similar to relativity. (extension of relativity, generalization of the space-time concept) A solution to the hierarchy problem. The coupling unification in SUSY GUT

Hierarchy problem and SUSY String and GUT unification -> A cutoff scale ~ Planck scale (10^19 GeV). SUSY is the only known symmetry to avoid the fine tuning in the renormalization of the Higgs boson mass at the level of O(10^34). Three possibilities: Some new dynamics associated with the electroweak symmetry breaking exists just above the TeV scale. SUSY exists. Fine-tuning is realized by unknown reason. => LHC will provide a hint on which is the correct direction.

SUSY models A SUSY model is not a single model, rather collection of models. The number of free parameters of the minimal supersymmetric standard model (MSSM) is about 100. Low energy SUSY models = SUSY extensions of the SM R-parity conserving model R-parity violation MSSM NMSSM, Extra U(1), etc. SUSY Breaking scenarios (mSUGRA, AMSB, GMSB, etc.) SUSY GUT, See-saw neutrino, String unification No strong motivations to consider beyond the MSSM.

MSSM The particle content of MSSM = Two Higgs doublet SM + scalar SUSY partners and fermionic SUSY partners Two Higgs doublets are necessary for fermion Yukawa couplings. H1: down-type-quark and lepton Yukawa couplings H2: up-type-quark Yukawa couplings

SUSY phenomenology Discover SUSY particles Establish the symmetry property. Determine SUSY breaking mechanism. Clarify the meaning in unification and the cosmological connection.

SUSY at LHC LHC experiments will provide a crucial test for SUSY. Mass reach of squark and gluino search is about 2 TeV. A light Higgs boson below 135 GeV must exist for MSSM. Higgs search: At least one Higgs boson can be found. SUSY search: Cascade decay. ~gluino 2 TeV m1/2(GeV) mSUGRA MSSM

LC studies on SUSY Determine mass, spin and quantum numbers of SUSY particles. Beam polarization and energy scan are very useful tools. Determine chargino and neutralino mixings. Test SUSY coupling relations. Test the gaugino GUT relation. Determine properties of the dark matter candidate. Search for lepton flavor violation in slepton production and decays.

Smuon production and decay Test of a SUSY relation Smuon production and decay  Selectron production Dark matter candidate? M.M.Nojiri, K. Fujii and T. Tsukamoto

SUSY breaking scenario Combined analysis of LHC and LC provide a hint on a SUSY breaking scenario. LHC: Squark and gluino production and cascade decay LC: Slepton, neutlarino, and chargino pair-production SUSY particle masses Combined analysis Energy scale SUSY breaking scenario G.A.Blair, W.Porod,and P.M.Zerwas

SUSY Seesaw model Large Lepton flavor violation processes are expected. m->eg in SU(5) SUSY GUT with seesaw neutrino Slepton flavor mixing J.Hisano, M.M.Nojiri, Y.Shimizu, M.Tanaka MEG experiment T.Goto,Y.Shimizu,T.Shindo,M.Tanaka and Y.Okada.

(3) Dark matter and collider physics Energy composition of the Universe Dark energy 73%   Dark matter 23%   Baryon     4% Dark matter candidate WINP (weakly interacting massive particle)  Stable, neutral

Relic abundance of dark matter A larger pair annihilation cross section -> Smaller relic abundance Candidates of dark matter   SUSY neutralino, gravitino   KK-photon in the universal extra dimension model, Heavy photon in the little Higgs model with a T parity Collider physics (1) Discovery of the dark matter candidate (2) Identify a correct model. (3) Determine the mass and couplings and compare the relic abundance.

Identification of the dark matter at LC  Even if a dark matter candidate is found at LHC by missing energy signals, many possibilities can exist. Ex. SUSY and KK model can be distinguished at LC. Threshold behaviors for smuon and KK muon productions neutralino sneutrino KK photon M.Peskin

SUSY Dark matter at LC SUSY mass and coupling measurements ALCPG cosmology subgroup SUSY mass and coupling measurements => Identification of dark matter PLANCK WMAP

Conclusions Discovery of the Higgs boson is the first step to understand the dynamics of the electroweak symmetry breaking. In order to confirm the mass generation mechanism of elementary particles, coupling constants related to the Higgs boson have to be measured precisely. SUSY, if it exists, has far-reaching consequences in particle physics and cosmology.