Implication of 126 GeV Higgs for Planck scale physics 1 Satoshi Iso (KEK, Sokendai) with Y.Orikasa (Osaka) 1210.2848 to appear in PTEP Higgs was discovered.

Slides:



Advertisements
Similar presentations
Higgs physics theory aspects experimental approaches Monika Jurcovicova Department of Nuclear Physics, Comenius University Bratislava H f ~ m f.
Advertisements

Fine Tuning Standard Model and Beyond Peter Athron Dr David Miller In collaboration with.
THE FINE-TUNING PROBLEM IN SUSY AND LITTLE HIGGS
Kiwoon Choi PQ-invariant multi-singlet NMSSM
Peter Athron David Miller In collaboration with Fine Tuning In Supersymmetric Models.
What do we know about the Standard Model? Sally Dawson Lecture 4 TASI, 2006.
THE STATUS OF THE BSM SCENARIOS (AFTER THE FIRST LHC PHASE) STEFAN POKORSKI, UNIVERSITY OF WARSAW.
Chiral freedom and the scale of weak interactions.
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.
The classically conformal B-L extended standard model Yuta Orikasa Satoshi Iso(KEK,SOKENDAI) Nobuchika Okada(University of Alabama) Phys.Lett.B676(2009)81.
Phenomenological Aspects of SUSY B-L Extension of the SM 1 Shaaban Khalil Centre for Theoretical Physics British University in Egypt.
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.
Chiral freedom and the scale of weak interactions.
Richard Howl The Minimal Exceptional Supersymmetric Standard Model University of Southampton UK BSM 2007.
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 Top Quark and Precision Measurements S. Dawson BNL April, 2005 M.-C. Chen, S. Dawson, and T. Krupovnikas, in preparation M.-C. Chen and S. Dawson,
Chiral freedom and the scale of weak interactions.
CUSTODIAL SYMMETRY IN THE STANDARD MODEL AND BEYOND V. Pleitez Instituto de Física Teórica/UNESP Modern Trends in Field Theory João Pessoa ─ Setembro 2006.
Jose E. Garcia presented by: Jose E. Garcia (IFIC-Valencia) on behalf of ATLAS Collaboration XXXIXth Rencontres de Moriond.
Chiral freedom and the scale of weak interactions.
.. Particle Physics at a Crossroads Meenakshi Narain Brown University.
The Higgs boson and its mass. LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12.
 Collaboration with Prof. Sin Kyu Kang and Prof. We-Fu Chang arXiv: [hep-ph] submitted to JHEP.
Kaluza-Klein gluon production at the LHC
Fermion Masses and Unification Steve King University of Southampton.
Two Higgs doublets model in gauge-Higgs unification framework Yonsei University Jubin Park (SNUT)  Collaboration with Prof. We-Fu Chang,
Geneva, October 2010 Dark Energy at Colliders? Philippe Brax, IPhT Saclay Published papers :
Associated production of the Higgs boson and a single top quark in the littlest Higgs model at Large Hadron Collier Shuo Yang.
What do we know about the Standard Model? Sally Dawson Lecture 2 SLAC Summer Institute.
Center for theoretical Physics at BUE
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.
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.
1 THEORETICAL PREDICTIONS FOR COLLIDER SEARCHES “Big” and “little” hierarchy problems Supersymmetry Little Higgs Extra dimensions G.F. Giudice CERN.
Low scale supergravity mediation in brane world scenario and hidden sector phenomenology Phys.Rev.D74:055005,2006 ( arXiv: hep-ph/ ) ACFA07 in Beijing:
Twin Higgs Theories Z. Chacko, University of Arizona H.S Goh & R. Harnik; Y. Nomura, M. Papucci & G. Perez.
The mass of the Higgs boson and the great desert to the Planck scale.
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.
Low-scale Gaugino Mediation in Warped Spacetime Toshifumi Yamada Sokendai, KEK in collaboration with Nobuchika Okada (Univ. of Alabama ) arXiv: May 11,
Thoughts on Higgs naturalness problem
Scale invariance and the electroweak symmetry breaking Archil Kobakhidze with R. Foot, K.L. McDonald and R. R. Volkas: Phys. Lett. B655 (2007) Phys.
Neutrino mass and DM direct detection Daijiro Suematsu (Kanazawa Univ.) Erice Sept., 2013 Based on the collaboration with S.Kashiwase PRD86 (2012)
Electroweak Symmetry Breaking without Higgs Bosons in ATLAS Ryuichi Takashima Kyoto University of Education For the ATLAS Collaboration.
Dynamical EWSB and Fourth Generation Michio Hashimoto (KEK) Mt. Tsukuba M.H., Miransky, M.H., Miransky, in preparation.
SUSY and Superstrings Masahiro Yamaguchi Tohoku University Asian School Particles, Strings and Cosmology (NasuLec) September 25-28, Japan.
1 Prospect after discoveries of Higgs/SUSY Yasuhiro Okada (KEK) “Discoveries of Higgs and Supersymmetry to Pioneer Particle Physics in the 21 st Century”
H. Quarks – “the building blocks of the Universe” The number of quarks increased with discoveries of new particles and have reached 6 For unknown reasons.
1 Higgs Physics Yasuhiro Okada (KEK) November 26, 2004, at KEK.
Nobuchika Okada The University of Alabama Miami 2015, Fort Lauderdale, Dec , GeV Higgs Boson mass from 5D gauge-Higgs unification In collaboration.
The Search For Supersymmetry Liam Malone and Matthew French.
Supersymmetric B-L Extended Standard Model with Right-Handed Neutrino Dark Matter Nobuchika Okada Miami Fort Lauderdale, Dec , 2010 University.
Monday, Apr. 7, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #20 Monday, Apr. 7, 2003 Dr. Jae Yu Super Symmetry Breaking MSSM Higgs and Their.
The Importance of the TeV Scale Sally Dawson Lecture 3 FNAL LHC Workshop, 2006.
Renormalization of the Higgs Triplet Model Mariko Kikuchi ( Univ. of Toyama ) Collaborators M. Aoki ( Kanazawa Univ. ), S. Kanemura ( Univ. of Toyama ),
Diquark Higgs production at LHC Nobuchika Okada Theory Division, High Energy Accelerator Research Organization (KEK) In collaboration with Rabindra Nath.
Lecture 7. Tuesday… Superfield content of the MSSM Gauge group is that of SM: StrongWeakhypercharge Vector superfields of the MSSM.
Profound Implications of the Higgs Boson Christopher T. Hill Fermilab ATLAS Collaboration meeting Argonne Nat’l. Lab July 15, 2013.
New Physics effect on Higgs boson pair production processes at LHC and ILC Daisuke Harada (KEK, Graduate University for Advanced Studies) in collaboration.
Charged Higgs boson decay in supersymmetric TeV scale seesaw model
Unified Modes and Collider Experiments
Dynamical Fine-Tuning of Initial Conditions
Classically conformal B-L extended Standard Model
Fine Tuning In Supersymmetric Models
The MESSM The Minimal Exceptional Supersymmetric Standard Model
Shuo Yang Associated production of the Higgs boson and
Prospect after discoveries of Higgs/SUSY
Presentation transcript:

Implication of 126 GeV Higgs for Planck scale physics 1 Satoshi Iso (KEK, Sokendai) with Y.Orikasa (Osaka) to appear in PTEP Higgs was discovered at M H =126 GeV 26 Jan 京産大 No evidence of “new” ATLAS,CMS & LHCb What is the implication of these two? together with some phenomena beyond SM (ν oscillation, Baryon asymmetry, Dark matter)

Discovery of Higgs(-like particle) was reported by CMS and ATLAS groups: 7 TeV L= 5.2 /fb (2011) + 8 TeV with L= 5.1 /fb for 3 months in 2012 Mh = ± 0.4 GeV (stat)± 0.4 GeV (sys) CMS ± 0.4 GeV (stat)± 0.4 GeV (sys) ATLAS ATLAS H  2 gamma CMS H  2 gamma Brief summary of July 4 th  Now 12.2 /fb

Production of SM Higgs 3

Decay modes of SM Higgs 3 major channels for low mass Higgs 1% mass resolution Another useful decay modes 4

CS is low (50 fb), but relatively clean bkg  around 250 events are 5 /fb  170 efficiency 40 % (ATLAS) in 6340 backgrounds SM ATLAS CMS Both of CMS and ATLAS reported slightly larger events than SM expected but not inconsistent with SM result. New particles may contribute to the loop. 5

CMS 6 Gold plated mode

CMS combining all decay modes SM ATLAS SM 7 M h = ± 0.4 ± 0.4 GeV (CMS) ± 0.4 ± 0.4 GeV (ATLAS)

125-6 GeV Higgs Almost consistent with Standard Model Higgs But slightly larger events of H  2 photon than SM prediction LHC will run until this winter before upgrade to TeV 3 times data will be collected new physics search They will give new data analysis at Moriond Stay tuned. 8

9 What can we learn from the current data? Higgs mass 126 GeV No evidence beyond SM Higgs decay Flavor physics: LHCb, B-factory, MEG (e.g. Br(Bs  μμ) = ×10 -9 ) consistent with SM (3.2±0.2)× It is a good time to reconsider “the central dogma” of particle physics GUT  hierarchy problem  TeV SUSY

10 Hierarchy problem

Naturalness (Hierarchy problem) Quadratic divergence Quadratic divergence in Higgs mass term Cancellation of Quadratic divergence (supersymmetry etc.)

Bardeen Ontake summer school) Standard model is classically scale invariant if Higgs mass term is absent. Quantum anomaly breaks the invariance (if not conformal ) The common wisdom is that the breaking is not soft and we have Bardeen argued that it should be

13 Hierarchy problem Is quadratic divergence the issue of hierarchy problem? NO Bardeen(1995) There are 3 different types of divergences 1.Quadratic divergences Λ 2 2.Logarithmic divergences m 2 log Λ 3.Logarithmic but looks like quadratic M 2 log Λ H Aoki, SI PRD(2012)

(2) No Higgs mass term is generated in SM through RGE (multiplicatively renormalized) (1)Quadratic divergence can be simply subtracted, so it gives a boundary condition at UV cut off Λ.  If massless at Λ, it continues to be so in the IR theory. (3) If SM is coupled with a massive particle with mass M, logarithmic divergences give a correction to m as 14

FP * * With quadratic div.No quadratic div. Fine - tuning of the distance from the critical line = Low energy mass scale The difference is the choice of the coordinates of the parameter space. Critical line Hierarchy problem in Wilsonian RG H Aoki, SI PRD(2012)]

16 In order to solve the “hierarchy problem” without a special cancellation like supersymmetry, we need to control (a) “quadratic divergence”  correct boundary condition at Planck The most natural b.c. is NO MASS TERMS at Planck ( = classical conformal invariance) (b) “radiative corrections” by mixing with other relevant operators No intermediate scales between EW (or TeV) and Planck “Classical conformal theory with no intermediate scale” can be an alternative solution to hierarchy problem. Bardeen (95) Shaposhnikov (07) Meissner Nicolai (07) SI, Okada,Orikasa (09)

17 Stability of Vacuum

18 Another Hint of 126 GeV Higgs mass is Stability bound of the Higgs quartic coupling

Higgs potential RGE improved effective potential for large field (h >> v) Already known It is related to Higgs mass as Higgs mass controls the behavior of Higgs potential at large values of h. This gives two bounds for Higgs mass (1) The quartic coupling does not blow up until UV cut-off. M < 180 GeV (triviality bound) (2) The quartic coupling does not become negative until UV cut-off. (Stability bound) M = 125 GeV Higgs is very close to the stability bound

New physics at GeV is necessary to stabilize the vacuum Flat Higgs potential at Planck scale 20 Why stability bound is important for Planck scale physics? very sensitive to top quark mass Elias-Miro et.al.(12) Shaposhnikov et.al. (12)

If this is the case ? 21 Direct window to Planck scale M.Shaposhnikov (07)

22 Emergence of Higgs potential

23 Hierarchy (classical conformality) Stability Vanishing at Planck LHC experiment implies that Higgs has a flat potential V(H)=0 at Planck. Indication of LHC on Higgs potential

24 Higgs particle Potential minimum Spontaneous Symmetry Breaking Higgs potential 加速器科学研究奨励会 2012/10/5

25 How can we realize EW symmetry breaking from V(H)=0 potential at Planck? Everything should be radiatively generated.

Two mechanisms of symmetry breaking (2) Coleman-Weinberg mechanism (radiative breaking) (1) SSB by negative mass term tree1-loop 26 Higgs mass is given by

27 Coleman-Weinberg radiative breaking Symmetry is broken near the scale where the coupling crosses zero. Dimensional transmutation ( 2’ ) RG improved CW mechanisms cf. Dimensional transmutation in QCD

But CW does not work in SM. the large top Yukawa coupling invalidates the CW mechanism Extension of SM is necessary ! 28 “Occam’s razor” scenario that can explain ・ 126 GeV Higgs ・ hierarchy problem ・ ν oscillation, baryon asymmetry (B-L) extension of SM with flat Higgs potential at Planck SM B-L sector ・ U(1)B-L gauge ・ SM singlet scalar φ ・ Right-handed ν N Okada, Y Orikasa, & SI (PLB) (PRD) (PRD) (PTEP) Meissner Nicolai (07)

Model: (B-L) extension of SM with Right Handed Neutrinos ・ B-L is the only anomaly free global symmetry in SM. ・ [U(1) B-L ] 3 is anomaly free if we have right handed fermion. ・ B-L gauge symmetry is broken by vev of an additional scalar. See-saw mechanism H Higgs doublet B-L sector scalar field N Okada, Y Orikasa, SI PLB676(09)81, PRD80(09) PRD83(11)

30 Flat Higgs potential at Planck scale classically conformal 126 GeV key to relate EW and TeV CW mechanism in B-L sector PlanckTeV B-L can be broken by CW mechanism at TeV.

31 How about EWSB ? Can the small scalar mixing be realized naturally? Radiatively generated scalar mixing λ mix in V(H) triggers EWSB YES

32 ******** Why is small negative λ mix generated? U(1)_YU(1)_(B-L)

33 Running of Scalar mixing small negative

Prediction of the model In order to realize EWSB at 246 GeV, B-L scale must be around TeV (for a typical value of α B-L ). ILC 34 LHC reach 14 TeV 100 fb -1

Stability bound in TeV scale B-L model An extra positive term is added 35 Lower the stability bound Stability bound In SM

36 Summary ・ 126 GeV Higgs = border of the stability bound of SM vacuum.  Direct window to Planck scale  Flat Higgs Hint for the origin of Higgs in string theory ・ Occam’s razor scenario beyond SM “Classically conformal B-L model” is proposed (1) it can solve hierarchy problem (2) it can explain why B-L breaking scale is around TeV. (3) Stability bound can be lowered about 1 GeV M H ~ 128 GeV (4) phenomenologically viable Neutrino oscillation, resonant leptogenesis (5) Highly predictive (or excludable) Prediction Z’ around a few TeV, M φ < M Z’, Leptogenesis at TeV

37 Future perspectives ・ Origin of flat Higgs potential at Planck Hierarchy problem & M H =126 GeV  PNGB ? Moduli ? Gauge/Higgs ? ….. Non-susy vacua of superstring with flat V(H) ・ Resonant leptogenesis Kadanoff-Baym equation (quantum Boltzman) ・ Non-susy GUT at Planck SO(10) or E6 type Gravity or string threshold correction to RGE Garny, Kartavsev, Hohenegger (11)