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.

Slides:



Advertisements
Similar presentations
Kiwoon Choi PQ-invariant multi-singlet NMSSM
Advertisements

The minimal B-L model naturally realized at TeV scale Yuta Orikasa(SOKENDAI) Satoshi Iso(KEK,SOKENDAI) Nobuchika Okada(University of Alabama) Phys.Lett.B676(2009)81.
Exploration without Map - Lepton-Flavor Violation in LHC era - 1st Open Meeting of the SuperKEKB Collaboration KEK, Japan, December 2008 J.HISANO.
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.
P461 - particles VII1 Glashow-Weinberg-Salam Model EM and weak forces mix…or just EW force. Before mixing Bosons are massless: Group Boson Coupling Quantum.
1 SUSY and B physics observables Yasuhiro Okada (KEK) Super B Factory Workshop in Hawaii, April 20, 2005.
Yingchuan Li Weak Mixing Angle and EIC INT Workshop on Pertubative and Non-Pertubative Aspects of QCD at Collider Energies Sep. 17th 2010.
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.
The LC and the Cosmos: Connections in Supersymmetry Jonathan Feng UC Irvine American Linear Collider Physics Group Seminar 20 February 2003.
JoAnne Hewett, SLAC Scientific Opportunities at a Linear Collider: Making the Case.
Big Questions, L(H)C Answers Jonathan Feng UC Irvine LC/LHC Workshop, Fermilab 13 December 2002.
The International Linear Collider Barry Barish iThemba Cape Town 21-Oct-05.
Paris 22/4 UED Albert De Roeck (CERN) 1 Identifying Universal Extra Dimensions at CLIC  Minimal UED model  CLIC experimentation  UED signals & Measurements.
The Big Bang, the LHC and the Higgs Boson Dr Cormac O’ Raifeartaigh (WIT)
Searches for New Physics Motivations Examples Searches so far Setting scene for LHC 1/12.
SUSY Dark Matter Collider – direct – indirect search bridge. Sabine Kraml Laboratoire de Physique Subatomique et de Cosmologie Grenoble, France ● 43. Rencontres.
 Collaboration with Prof. Sin Kyu Kang and Prof. We-Fu Chang arXiv: [hep-ph] submitted to JHEP.
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
The Dark Side of the Universe What is dark matter? Who cares?
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.
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.
1 Summary talk for ILC Physics Yasuhiro Okada (KEK) November 12, 2004 ACFA LC7, Taipei.
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:
INVASIONS IN PARTICLE PHYSICS Compton Lectures Autumn 2001 Lecture 8 Dec
WHAT BREAKS ELECTROWEAK SYMMETRY ?. We shall find the answer in experiments at the LHC? Most likely it will tells us a lot about the physics beyond the.
Theoretical Issues in Astro Particle Physics J.W. van Holten April 26, 2004.
Ohio State DUSEL Theory Workshop Stuart Raby Underground Detectors Investigating Grand Unification Brookhaven National Lab October 16, 2008.
Report on New Physics Subgroup Activities Nobuchika Okada (KEK) 5th general meeting of the ILC physics working group May 31, KEK Past activities.
1 Prospect after discoveries of Higgs/SUSY Yasuhiro Okada (KEK) “Discoveries of Higgs and Supersymmetry to Pioneer Particle Physics in the 21 st Century”
Low scale gravity black holes at LHC Enikő Regős ( CERN )
1 Higgs Physics Yasuhiro Okada (KEK) November 26, 2004, at KEK.
Compelling Scientific Questions The International Linear Collider will answer key questions about matter, energy, space and time We now sample some of.
The Search For Supersymmetry Liam Malone and Matthew French.
Higgs boson pair production in new physics models at hadron, lepton, and photon colliders October Daisuke Harada (KEK) in collaboration.
The Standard Model of the elementary particles and their interactions
1 Overview of physics RDR and the next step Yasuhiro Okada (KEK/Sokendai) March 3, 2008 TILC08, Sendai, Japan.
Diquark Higgs production at LHC Nobuchika Okada Theory Division, High Energy Accelerator Research Organization (KEK) In collaboration with Rabindra Nath.
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.
Elba -- June 7, 2006 Collaboration Meeting 1 CDF Melisa Rossi -- Udine University On behalf of the Multilepton Group CDF Collaboration Meeting.
Collider Signals of Extra Dimension Scenarios
February 12, 2003ACFA LC Symposium 1 JLC Physics Yasuhiro Okada (KEK) ACFA LC Symposium February 12, 2003,Tsukuba, Japan.
Journées de Prospective
Physics Overview Yasuhiro Okada (KEK)
Shufang Su • U. of Arizona
MSSM4G: MOTIVATIONS AND ALLOWED REGIONS
Collider Phenomenology of SUSY Cosmic Connections &
Barbara Mele Sezione di Roma
Higgs and SUSY at future colliders
ILC and future high energy physics
Lepton Flavor Violation
Electroweak Baryogenesis and LC
Physics at a Linear Collider
Yasuhiro Okada (KEK) FPCP 2004, Deagu, Korea October 7, 2004
Physics Overview Yasuhiro Okada (KEK)
Yasuhiro Okada (KEK) April 17, 2003, CAT, Indore, India
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
Prospect after discoveries of Higgs/SUSY
Presentation transcript:

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

2 Fundamental questions in elementary particle physics What are the elementary constituents of matter? What are forces acting between them? How has the Universe begun and evolved?

3 How have we come to the Standard Model ? nuclear force pionquark gravity EM interaction weak interaction strong interaction Fermi theory Electroweak theory Higgs mechanism QCD general relativity

4 Why TeV scale? This is the scale of the weak interaction, in modern language, the Higgs vacuum expectation value (~246 GeV). We expect to find a Higgs boson and “New Physics” associated to the electroweak symmetry breaking. The answer to the question “what is the physics behind the electroweak symmetry breaking?” is a crucial branching point for the future of particle physics. Supersymmetry vs. Low cut-off theory (Little Higgs models, models with large extra-dimension, etc.)

5 Why do we expect physics beyond the Standard Model? We do not know how the Higgs field arises. There are evidences which require new particles and/or new interactions. Neutrino mass Dark matter Baryon-anti-baryon asymmetry of the Universe Expectation of Unification. GUT, Superstring

6 Weak Int. Standard Model Higgs Physics EM Interaction Strong Int. Gravity GUT SUSY Seesaw Neutrino Superstiring Alternative scenarios (Extra dim, Little Higgs model,etc) 100 GeV Dark Matter Baryogenesis Inflation Dark Energy TeV GeV

7 Why do we need both LHC & ILC? Two machines have different characters. Advantage of lepton colliders: e + and e - are elementary particles (well-defined kinematics). Less background than LHC experiments. Beam polarization, energy scan.  -  e- , e - e - options, Z pole option. LHC ILC

8 Goals of ILC physics Higgs physics (Electroweak symmetry breaking and mass generation mechanism of quarks, leptons, and gauge bosons.) New physics signals Direct search for new particles and interactions. Indirect search for new physics effects through the SM particle processes. Capability of precise measurements of various quantities is a key.

9 [1] Higgs physics A Higgs boson will be discovered at LHC as long as its properties (production/decay) is similar to the SM Higgs boson. In order to study the Higgs mechanism at work, Higgs couplings to various particles have to be measured precisely.

10 Higgs boson search at LHC M H (GeV) 55 SM Higgs boson branching ratio Higgs boson discovery at LHC

11 Higgs physics at ILC Production of 0(10 5 )Higgs bosons. Determination of spin and parity. Precise mass determination. Measurements of production corss sections and branching fractions TESLA TDR GLC report Higgs boson couplings to other particles Mass generation mechanism

12 Coupling measurements at ILC GLC Project m H =120 GeV, Ecm= GeV.L=500fb -1 Higgs self-coupling (Ecm>700 GeV) LHC: (10)% for ratios of coupling constants ILC: a few % determination

13 New physics effects in Higgs boson couplings In many new physics models, the Higgs sector is extended and /or involves new interactions. The Higgs boson coupling can have sizable deviation from the SM prediction. B(h->bb)/B(h->  ) LC J.Guasch, W.Hollik,S.Penaranda B(h->WW)/B(h->  ) LHC LC The heavy Higgs boson mass in the MSSMSUSY correction to Yukawa couplings ACFA report

14 Radion-Higgs mixing in extra-dim model Little Higgs model with T parity C.-R.Chen, K.Tobe, C.-P. Yuan The triple Higgs coupling in 2HDM in the electroweak baryogenesis scenario HEPAP report S.Kanemura, Y. Okada, E.Senaha Deviation to 5-10 % level can be distinguished at ILC

15 [2] Direct searches for New Physics Some type of new signals is expected around 1TeV range, if New Physics is related to a solution of the hierarchy problem. (SUSY, Large extra-dimension, etc ) The first signal of New Physics is likely to be obtained at LHC. (ex. squarks up to 2.5 TeV at LHC) ILC experiments are necessary to figure out what is New Physics, by measuring spin, quantum numbers, coupling constants of new particles, and finding lower mass particles which may escape detection at LHC. Beam polarization, energy scan, and well-defined initial kinematics play important roles in ILC studies.

16 SUSY studies at ILC SUSY is a symmetry between fermions and bosons. Spin determination is essential, ideal for ILC. W,Z,  H gluon lepton quark neutralino, chargino gluino slepton squark SM particlesSuper partners Spin 1/2Spin 0 Spin 1 Spin 1/2 Spin 1 Spin 1/2 Spin 0 neutralino mixing chargino mixing Mixing angle determination

17 SUSY relation M.M.Nojiri, K.Fujii, and T.Tsukamoto Right-handed selectron production SUSY predicts characteristic relations among superpartner’s interactions.

18 If we combine information from LHC and LC, we can test whether SUSY breaking masses satisfy GUT and/or Unification conditions Gauge coupling unification GUT relation B.C.Allanach, et al in LHC/LC report Gaugino mass relation Scalar mass relation

19 Large extra-dimensions An alternative solution to the hierarchy problem. LC physics: Size and numbers of extra-dimensions, The spin 2 property of Kaluza-Klein gravitons. G.W.Wilson Angular distribution -> Spin 2 exchange N.Delerue, K.Fujii, N.Okada graviton matter

20 [3] Dark matter and collider physics Energy composition of the Universe Dark energy 74% Dark matter 22% Baryon 4% Dark matter candidate WIMP ( weakly interacting massive particle) a stable, neutral particle WIMP candidates Neutralino (SUSY) KK-photon (UED) Heavy photon (Little Higgs with T parity)…

21 Cosmological parameter determination WMAP, Planck, … Direct and indirect ( , e+,anti-p, ) searches for dark matter Collider search for a dark matter candidate particle at LHC and ILC. ILC will play a particularly important role in distinguishing different models and determine properties of the dark matter candidate. Thermal history of the Universe Dark matter profile in our galaxy Thermal relic abundanceDetection rate See, E.A.Baltz,M.Battaglia,M.E.Peskin,and T.Wizansky, hep-ph/

22 SUSY Dark matter at ILC ALCPG cosmology subgroup SUSY mass and coupling measurements => Identification of dark matter

23 [4] Precision measurements of SM processes Improve precision of the fundamental parameters. Search for new physics in indirect ways. GLC report The threshold scan improves the top mass measurement and determines the top width. Top quark threshold scan Deviation of the top width in the Little Higgs model. C.F.Berger,M.Pelestein,F.Petriello

24 Z’ and e + e - ->ff processes Even if ILC at 500 GeV cannot produce a new Z’ particle kinematically,we can determine left-handed and right-handed couplings from ee-> ff processes. This will give important information to identify the correct theory. S.Godfrey, P.Kalyniak, A.Tomkins m z’ =2TeV,Ecm=500 GeV, L=1ab -1 with and w/o beam polarization e e f f Z’ LHC=> mass ILC => coupling Z’ coupling determination at ILC

25 [5] Physics Benchmarks for the ILC Detectors M.Battaglia, T.Barklow, M.E.Peskin, Y.Okada, S.Yamashita, and P.Zerwas, hep-ex/ The big table Benchmark processes for detector design and optimization. Selected from important physics reactions

26 The short list

27 Conclusions The LHC experiment is expected to open a new era of the high energy physics by finding a Higgs boson and other new particles. Establishing the mass generation mechanism is the urgent question. This will be achieved by precise determination of the Higgs couplings, and ILC will play essential roles. In order to explore New Physics, Higgs coupling measurements, direct study of new particles and new phenomena, and indirect searches through SM processes are all important at ILC. TeV physics explored at LHC and ILC will lead to new understanding of unification and cosmology.