Implications of a Heavy Z Gauge Boson
|
|
- Buddy Cunningham
- 5 years ago
- Views:
Transcription
1 Implications of a Heavy Z Gauge Boson Motivations A (string-motivated) model Non-standard Higgs sector, CDM, g µ 2 Electroweak baryogenesis FCNC and B s B s mixing
2 References T. Han, B. McElrath, PL, hep-ph/ (implications of Higgs sector) V. Barger, C. Kao, PL and H. S. Lee, hep-ph/ (cold dark matter). V. Barger, C. Kao, PL and H. S. Lee, in preparation (g µ 2) J. Kang, T. Li, T. Liu, and PL, hep-ph/ (electroweak baryogenesis) V. Barger, C. W. Chiang, J. Jiang and PL, hep-ph/ (B s B s mixing).
3 Beyond the MSSM Even if supersymmetry holds, MSSM may not be the full story Most of the problems of standard model remain (hierarchy of electroweak and Planck scales is stabilized but not explained) µ problem introduced Could be that all new physics is at GUT/Planck scale, but there could be remnants surviving to TeV scale Specific string constructions often have extended gauge groups, exotics Important to explore alternatives/extensions to MSSM
4 Motivations Strings, GUTs, DSB, little Higgs, LED often involve extra Z (GUTs require extra fine tuning for M Z M GUT ) String models Extra U(1) and SM singlets extremely common Radiative breaking of electroweak (SUGRA or gauge mediated) often yield EW/TeV scale Z (unless breaking along flat direction intermediate scale) Breaking due to negative mass 2 for scalar S (driven by large Yukawa) or by A term
5 S f S ~ f _ f t
6 Solution to µ problem (string-motivated extension of NMSSM) W hsh u H d, U(1) may forbid elementary µ or term in Kähler S = standard model singlet, charged under U(1) S breaks U(1), µ eff = h S Like NMSSM, but no domain walls (Alternative: nmssm) Singlets don t have W κs 3 (cf. NMSSM) in constructions studied SM-singlets usually have U(1) charges in constructions studied
7 Flat directions Two SM singlets charged under U(1). If no F terms, V (S 1, S 2 ) = m 2 1 S2 1 + m2 2 S2 2 + g 2 Q 2 ( S S2 2 )2 Break at EW scale for m m2 2 > 0, at intermediate scale for m m2 2 < 0 (stabilized by loops or HDO) Small Dirac (or other fermion) masses from ( Ŝ ) PD W Ĥ 2 ˆL Lˆν c L M Secluded sector: lift F -flatness by small ( 0.05) singlet Yukawa
8 Models SUSY-breaking scale models (Demir et al) M Z M Z, leptophobic M Z > 10M Z by modest tuning Secluded sector models (Erler, PL, Li) Approximately flat direction, broken by small ( 0.05) Yukawa Z breaking decoupled from effective µ term Four SM singlets: S, S 1,2,3, doublets H 1,2 Off-diagonal Yukawas (string-motivated) Can be consistent with minimal gauge unification
9 Superpotential : W = hsh 1 H 2 + λs 1 S 2 S 3 Potential : V = V F + V D + V soft V F = h 2 ( H 1 2 H S 2 H S 2 H 2 2) + λ 2 ( S 1 2 S S 2 2 S S 3 2 S 1 2) V D = G2 8 ( H2 2 H 1 2) g2 Z (Q S S 2 + Q H1 H Q H2 H ) 2 3 Q Si S i 2 i=1 where G 2 = g g2 2,
10 3 V soft = m 2 H 1 H m 2 H 2 H m 2 S S 2 + m 2 S i S i 2 i=1 (A h hsh 1 H 2 + A λ λs 1 S 2 S 3 + H.C.) + (m 2 SS 1 SS 1 + m 2 SS 2 SS 2 + m 2 S 1 S 2 S 1 S 2 + H.C.) S i m Si /λ large for small λ Breaking along D(U(1) ) 0 Smaller S, H i, dominated by ha h tan β 1, S H i Large doublet-singlet mixing Two sectors nearly decoupled Tree-level CP breaking in S, S i sector in general
11 Nonstandard Higgs (T. Han, PL, B. McElrath) Complex Higgs, neutralino spectrum and decays, very different from MSSM and NMSSM because of mixing and D terms
12 6 scalars and 4 pseudoscalars Can have tree level CP breaking mixing May separate into two sectors, one weakly coupled Often light scalars with significant doublet admixture, but reduced coupling due to singlet admixture; often light pseudoscalar Can have lightest Higgs up to 168 GeV with all couplings perturbative to M P because of D terms M 2 h h2 v 2 + (M 2 Z h2 v 2 ) cos 2 2β + 2g 2 Z v 2 (Q H2 cos 2 β + Q H1 sin 2 β) m 4 t v 2 π 2 log m t 1 m t 2 m 2 t. Typically, tan β 1 3
13 CP-Even MSSM fractions 1 MSSM Fraction ξ MSSM H 1 H 2 H 3 H 4 H 5 H MSSM Fraction M H (GeV)
14 LEP2 (209 GeV) Higgsstrahlung Cross Section σ(e + e - -> ZH) (fb) H 1 H 2 Standard Model MSSM NLO (tanβ=5) MSSM NLO (tanβ=10) MSSM NLO (tanβ=20) M H
15 LEP2 H A Cross Section σ(e + e - -> H A) (fb) H 1 A 1 H 1 A 2 H 2 A 1 MSSM NLO (tanβ=5) e M A (GeV)
16 M H vs. M A by MSSM fraction ξ MSSM > 0 ξ MSSM > ξ MSSM > 0.01 ξ MSSM > 0.1 ξ MSSM > M H (GeV) M A (GeV)
17 χ 0 1 χ0 1 Lightest Higgs Branching Ratios χ 0 1 χ0 i>1 χ 0 i>1 χ0 i>1 A A W + W - Z Z b b τ + τ c c 1 Branching Ratio M H1 (GeV)
18 Linear Collider (500 GeV)Higgsstrahlung Cross Section 100 σ(e + e - -> ZH)(fb) H 1 H 2 H 3 H 4 Standard Model MSSM h NLO (tanβ=5) MSSM H NLO (tanβ=5) M H (GeV)
19 Cold Dark Matter (V. Barger, C. Kao, PL, H.-S. Lee) 0.09 < Ω χ 0h 2 < 0.15 MSSM: limited parameter space for sufficient LSP (co)annihilation; mainly bino in most of parameter space. U(1) : additional Z -ino and singlino. ((n)nmssm: additional singlino) may have enhanced annihilation coupling to Z Solutions compatible with observations for most m χ 0 (only examined for large Z -ino mass)
20 1 0.1 S-model (M 2 > 0) (b) Zχ 0 χ 0 Coupling MSSM (M 2 > 0) Singlino (M 2 < 0) MSSM (M 2 < 0) S-model (M 2 < 0) 1e m 0 χ (GeV)
21 500 Ω χ h 2 < Ω χ h 2 < < Ω χ h 2 < < Ω χ h 2 < < Ω χ h 2 < < Ω χ h 2 < 1.0 (P3) (P1) (P1) s (GeV) s (GeV) LEP exclusion (m + χ1 < 104 GeV) (b) tanβ = M 2 (GeV) LEP exclusion (m + χ1 < 104 GeV) (c) tanβ = M 2 (GeV)
22 Muon g µ 2 (V. Barger, C. Kao, PL, H.-S. Lee) BNL E821: a µ (exp) = ( ± 5.8) σ deviation from its Standard Model (SM) prediction a µ a µ (exp) a µ (SM) = 23.9(7.2)(3.5)(6) 10 10, assuming e + e hadrons value for hadronic vacuum polarization MSSM: a µ (SUSY) tan β sign(µ) (M SUSY /100 GeV) 2, for common superpartner masses M SUSY, favoring large tan β and/or small M SUSY LEP2: m µ > 95 GeV
23 Z diagrams small for allowed M Z New Z -ino and singlino contributions in U(1), and different parameter range Neutralino mass matrix in { B, W 3, H 0 1, H 0 2, S, Z } basis M 1 0 g 1 v 1 /2 g 1 v 2 / M 2 g 2 v 1 /2 g 2 v 2 /2 0 0 g 1 v 1 /2 g 2 v 1 /2 0 h s s/ 2 h s v 2 / 2 g Z Q (H 0 1 )v 1 g 1 v 2 /2 g 2 v 2 /2 h s s/ 2 0 h s v 1 / 2 g Z Q (H 0 2 )v h s v 2 / 2 h s v 1 / 2 0 g Z Q (S)s 0 0 g Z Q (H 0 1 )v 1 g Z Q (H 0 2 )v 2 g Z Q (S)s M 1
24
25 Adequate g µ 2 possible, even with small tan β, consistent with m µ constraints, while also giving observed CDM aμ aμ tanβ Maximum a µ Observation: ( ) M soft GeV
26 Electroweak Baryogenesis (J. Kang, PL, T. Li, T. Liu) Baryon asymmetry n B /n γ Basic ideas worked out by Sakharov in 1967, but no concrete model Possible mechanisms Affleck-Dine baryogenesis GUT baryogenesis (wiped out by sphalerons for B L=0) Leptogenesis Electroweak baryogenesis
27 The Sakharov conditions 1. Baryon number violation 2. CP violation: to distinguish baryons from antibaryons 3. Nonequilibrium of B-violating processes
28 Electroweak baryogenesis Utilize the electroweak (B-violating) tunneling to generate the asymmetry at time of electroweak phase transition (Kuzmin, Rubakov, Shaposhnikov) Off the wall scenario (Cohen, Kaplan, Nelson) Strong first order phase transition from electroweak symmetry unbroken (massless W, Z, fermions) to broken phase (massive W, Z, fermions) proceeds by nucleation and 0 expansion of bubbles φ crit φ (Figures: W. Bernreuther, hep-ph/ ) V eff T = T 2 > T C T = T C T = T 1 < T C
29 CP violation by asymmetric reflection of quarks and leptons (or charginos/neutralinos) from the wall Electroweak B violation in unbroken phase outside wall Scenario requires strong first order transition, v(t c )/T c > and adequate CP violation in expanding bubble wall v Wall q q broken phase φ = 0 becomes our world unbroken phase q q CP Sph Γ B + L _~ 0 CP _ q _ q _ q _ q Sph Γ B + L >> H
30 Implementation of off the wall Standard model: no strong first order for M h violation too small > GeV; CP Minimal supersymmetric extension (MSSM): small parameter space for light Higgs and light stop; new sources for CP violation NMSSM (extension to include extra Higgs fields): can have strong first order for large ha h SH 1 H 2 but cosmological domain walls nmssm: strong transition without domain walls (Menon, Morrissey, Wagner)
31 Secluded sector U(1) : Symmetry breaking driven by large ha h SH 1 H 2 Tree level CP breaking in Higgs sector associated with soft SM singlet terms New contributions to electric dipole moments negligible First phase transition breaks U(1), second breaks SU(2) U(1) Phase transition strongly first order
32 Potential Value T=114.4 GeV T=119.5 GeV T=123.1 GeV T=124.6 GeV v (GeV) Transition at T c = 120 GeV, v(t c )/T c = 1.31
33 For τ lepton use thin wall approximation (justified) For reasonable parameters, can obtain adequate asymmetry, even for large t mass, from τ alone n B s = 90γ3 w (1 + v w v L )ξ Lm 2 δ θ CP h(δ, T )Γ (2π) 4 v w g T 3 s Larger contributions from neutralinos/charginos if not too heavy
34 -10 ) n B /s( v w =0.01 v w =0.02 v w = γ(π) γ = explicit CP phase. Exp: n B /s ( )
35 FCNC and rare B decays U(1) couplings often family-nonuniversal in string constructions FCNC (Z and Z from Z Z mixing) after family mixing (GIM breaking) (also from exotic mixing) Depends on V ψl and V ψr, ψ = u, d, e, ν, but only V CKM = V ul V d L and V MNS = V νl V e L known from exp K and µ decays first two families are universal (PL, Plümacher) Third family could be nonuniversal A 0b F B (Erler, PL) B s B s mixing and rare B decays, especially in competition with SM (or SUSY) loops, e.g. B φk, η K, πk or B s µ + µ (Leroux, London; Barger, Chiang, Jiang, PL, Lee) s b Z s s
36 Interaction L Z = g J µ Z µ, where J µ = i,j ψ I i γ µ [(ɛ ψl ) ij P L + (ɛ ψr ) ij P R ] ψ I j Can pick basis with ɛ ψl,r real and diagonal, but non-universal. In mass basis, couplings are B L d V d L ɛ dl V d L, B R d V d R ɛ dr V d R, which is Hermitian but non-diagonal.
37 x s = M s /Γ s > 20.8 SM box: x SM s = 26.3 ± 5.5 φ SM s Z (tree) B s B s mixing (V. Barger, C.-W. Chiang, J. Jiang,, PL) = 2 arg(v tb V ts ) = 2λ2 η 2 s b Z s b H Z eff = G ( F g2 M 2 Z B 2 g 1 M sb) L O LL (m b ) + LR + RR + RL Z G F 2 ρ 2 L e2iφ L O LL (m b ) + LR + RR + RL
38 100 x s φ L (degrees) ρ L 0.003
39 150 sin2φ s = x s =90 φ L (degrees) Consistent with SM 1σ range of x s 26.3 Exp. excluded ρ L
40 Conclusions Important to explore alternatives to MSSM Top-down string constructions very often contain extra Z and SM singlets S Elegant solution to µ problem (string-motivated extension of NMSSM) Many implications, including nonstandard Higgs spectrum/couplings, CDM, g µ 2, efficient EW baryogenesis, B s B s mixing, rare B decays, neutrino masses But, must observe Z
Implications of an extra U(1) gauge symmetry
Implications of an extra U(1) gauge symmetry Motivations 400 LEP2 (209 GeV) Higgsstrahlung Cross Section A (string-motivated) model σ(e + e - -> ZH) (fb) 350 300 250 200 150 100 50 H 1 H 2 Standard Model
More informationThe Matter-Antimatter Asymmetry and New Interactions
The Matter-Antimatter Asymmetry and New Interactions The baryon (matter) asymmetry The Sakharov conditions Possible mechanisms A new very weak interaction Recent Reviews M. Trodden, Electroweak baryogenesis,
More informationThe Physics of Heavy Z-prime Gauge Bosons
The Physics of Heavy Z-prime Gauge Bosons Tevatron LHC LHC LC LC 15fb -1 100fb -1 14TeV 1ab -1 14TeV 0.5TeV 1ab -1 P - =0.8 P + =0.6 0.8TeV 1ab -1 P - =0.8 P + =0.6 χ ψ η LR SSM 0 2 4 6 8 10 12 2σ m Z'
More informationSupersymmetric Origin of Matter (both the bright and the dark)
Supersymmetric Origin of Matter (both the bright and the dark) C.E.M. Wagner Argonne National Laboratory EFI, University of Chicago Based on following recent works: C. Balazs,, M. Carena and C.W.; Phys.
More informationarxiv:hep-ph/ v1 6 Feb 2004
arxiv:hep-ph/0402064v1 6 Feb 2004 AN NMSSM WITHOUT DOMAIN WALLS TAO HAN Department of Physics University of Wisconsin Madison, WI 53706 USA E-mail: than@pheno.physics.wisc.edu PAUL LANGACKER Department
More informationLecture 18 - Beyond the Standard Model
Lecture 18 - Beyond the Standard Model Why is the Standard Model incomplete? Grand Unification Baryon and Lepton Number Violation More Higgs Bosons? Supersymmetry (SUSY) Experimental signatures for SUSY
More informationE 6 Spectra at the TeV Scale
E 6 Spectra at the TeV Scale Instituts-Seminar Kerne und Teilchen, TU Dresden Alexander Knochel Uni Freiburg 24.06.2010 Based on: F. Braam, AK, J. Reuter, arxiv:1001.4074 [hep-ph], JHEP06(2010)013 Outline
More informationElectroweak baryogenesis in the MSSM. C. Balázs, Argonne National Laboratory EWBG in the MSSM Snowmass, August 18, /15
Electroweak baryogenesis in the MSSM C. Balázs, Argonne National Laboratory EWBG in the MSSM Snowmass, August 18, 2005 1/15 Electroweak baryogenesis in the MSSM The basics of EWBG in the MSSM Where do
More informationHiggs, neutralinos and exotics beyond the MSSM
Higgs, neutralinos and exotics beyond the MSSM N 5 (Singlino in χ ).8.6.4. nmssm N 6 in Beyond the MSSM Heavy Z Higgs Neutralinos Exotics 3 (GeV) M χ Fermilab (March, 6) References V. Barger, PL and H.
More informationLHC Signals of (MSSM) Electroweak Baryogenesis
LHC Signals of (MSSM) Electroweak Baryogenesis David Morrissey Department of Physics, University of Michigan Michigan Center for Theoretical Physics (MCTP) With: Csaba Balázs, Marcela Carena, Arjun Menon,
More informationAstroparticle Physics and the LC
Astroparticle Physics and the LC Manuel Drees Bonn University Astroparticle Physics p. 1/32 Contents 1) Introduction: A brief history of the universe Astroparticle Physics p. 2/32 Contents 1) Introduction:
More informationElectroweak Baryogenesis in the LHC era
Electroweak Baryogenesis in the LHC era Sean Tulin (Caltech) In collaboration with: Michael Ramsey-Musolf Dan Chung Christopher Lee Vincenzo Cirigliano Bjorn Gabrecht Shin ichiro ichiro Ando Stefano Profumo
More informationHiggs Signals and Implications for MSSM
Higgs Signals and Implications for MSSM Shaaban Khalil Center for Theoretical Physics Zewail City of Science and Technology SM Higgs at the LHC In the SM there is a single neutral Higgs boson, a weak isospin
More informationSupersymmetry Breaking
Supersymmetry Breaking LHC Search of SUSY: Part II Kai Wang Phenomenology Institute Department of Physics University of Wisconsin Madison Collider Phemonology Gauge Hierarchy and Low Energy SUSY Gauge
More informationCold Dark Matter beyond the MSSM
Cold Dark Matter beyond the MM Beyond the MM inglet Extended MM inglet Extended tandard Model References V. Barger, P. Langacker, M. McCaskey, M. J. Ramsey-Musolf and G. haughnessy, LHC Phenomenology of
More informationElectroweak Baryogenesis in Non-Standard Cosmology
Electroweak Baryogenesis in Non-Standard Cosmology Universität Bielefeld... KOSMOLOGIETAG 12... Related to works in colloboration with M. Carena, A. Delgado, A. De Simone, M. Quirós, A. Riotto, N. Sahu,
More informationElectroweak Baryogenesis after LHC8
Electroweak Baryogenesis after LHC8 Gláuber Carvalho Dorsch with S. Huber and J. M. No University of Sussex arxiv:135.661 JHEP 131, 29(213) What NExT? Southampton November 27, 213 G. C. Dorsch EWBG after
More informationGrand Unification. Strong, weak, electromagnetic unified at Q M X M Z Simple group SU(3) SU(2) U(1) Gravity not included
Pati-Salam, 73; Georgi-Glashow, 74 Grand Unification Strong, weak, electromagnetic unified at Q M X M Z Simple group G M X SU(3) SU() U(1) Gravity not included (perhaps not ambitious enough) α(q ) α 3
More informationDark Matter Direct Detection in the NMSSM
Dark Matter Direct Detection in the NMSSM,DSU27. Dark Matter Direct Detection in the NMSSM Daniel E. López-Fogliani Universidad Autónoma de Madrid Departamento de Física Teórica & IFT DSU27 D. Cerdeño,
More informationNew Physics from the String Vacuum
New Physics from the String Vacuum The string vacuum Extended MSSM quivers String remnants Small neutrino masses Quivers: Cvetič, Halverson, PL, JHEP 1111,058 (1108.5187) Z : Rev.Mod.Phys.81,1199 (0801.145)
More informationBeyond the MSSM. Beyond the MSSM. Heavy Z. Higgs. Neutralinos. Exotics. Neutrino Mass in Strings
Beyond the MSSM Beyond the MSSM Heavy Z Higgs Neutralinos Exotics Neutrino Mass in Strings References J. Kang, P. Langacker, T. j. Li and T. Liu, Electroweak baryogenesis in a supersymmetric U() model,
More informationPhysics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1
Physics 662 Particle Physics Phenomenology February 21, 2002 Physics 662, lecture 13 1 Physics Beyond the Standard Model Supersymmetry Grand Unified Theories: the SU(5) GUT Unification energy and weak
More informationIntroduction to Supersymmetry
Introduction to Supersymmetry I. Antoniadis Albert Einstein Center - ITP Lecture 5 Grand Unification I. Antoniadis (Supersymmetry) 1 / 22 Grand Unification Standard Model: remnant of a larger gauge symmetry
More informationNeutrinos and Fundamental Symmetries: L, CP, and CP T
Neutrinos and Fundamental Symmetries: L, CP, and CP T Outstanding issues Lepton number (L) CP violation CP T violation Outstanding issues in neutrino intrinsic properties Scale of underlying physics? (string,
More informationBeyond the MSSM (BMSSM)
Beyond the MSSM (BMSSM) Nathan Seiberg Strings 2007 SUSY 2012 Based on M. Dine, N.S., and S. Thomas, to appear Assume The LHC (or the Tevatron) will discover some of the particles in the MSSM. These include
More informationThe Constrained E 6 SSM
The Constrained E 6 SSM and its signatures at the LHC Work with Moretti and Nevzorov; Howl; Athron, Miller, Moretti, Nevzorov Related work: Demir, Kane, T.Wang; Langacker, Nelson; Morrissey, Wells; Bourjaily;
More informationPHYSICS BEYOND SM AND LHC. (Corfu 2010)
PHYSICS BEYOND SM AND LHC (Corfu 2010) We all expect physics beyond SM Fantastic success of SM (LEP!) But it has its limits reflected by the following questions: What is the origin of electroweak symmetry
More informationNeutrino masses respecting string constraints
Neutrino masses respecting string constraints Introduction Neutrino preliminaries The GUT seesaw Neutrinos in string constructions The triplet model (Work in progress, in collaboration with J. Giedt, G.
More informationarxiv:hep-ph/ v2 8 Jun 2004
hep-ph/0405244 MADPH 04 1376 UPR 1043T UCD 2004 20 arxiv:hep-ph/0405244v2 8 Jun 2004 The Higgs Sector in a U(1) Extension of the MSSM Tao Han 1,4, Paul Langacker 2, Bob McElrath 3 1 Department of Physics,
More informationSUSY and Exotics. UK HEP Forum"From the Tevatron to the LHC, Cosener s House, May /05/2009 Steve King, UK HEP Forum '09, Abingdon 1
SUSY and Exotics Standard Model and the Origin of Mass Puzzles of Standard Model and Cosmology Bottom-up and top-down motivation Extra dimensions Supersymmetry - MSSM -NMSSM -E 6 SSM and its exotics UK
More informationSplit Supersymmetry A Model Building Approach
Split Supersymmetry A Model Building Approach Kai Wang Phenomenology Institute Department of Physics the University of Wisconsin Madison UC Riverside HEP Seminar In Collaboration with Ilia Gogoladze (Notre
More informationNatural Electroweak Symmetry Breaking in NMSSM and Higgs at 100 GeV
Natural Electroweak Symmetry Breaking in NMSSM and Higgs at 100 GeV Radovan Dermíšek Institute for Advanced Study, Princeton R.D. and J. F. Gunion, hep-ph/0502105 R.D. and J. F. Gunion, hep-ph/0510322
More informationAstroparticle Physics at Colliders
Astroparticle Physics at Colliders Manuel Drees Bonn University Astroparticle Physics p. 1/29 Contents 1) Introduction: A brief history of the universe Astroparticle Physics p. 2/29 Contents 1) Introduction:
More informationBeyond the Standard Model
Beyond the Standard Model The Standard Model Problems with the Standard Model New Physics Supersymmetry Extended Electroweak Symmetry Grand Unification References: 2008 TASI lectures: arxiv:0901.0241 [hep-ph]
More informationBig Bang Nucleosynthesis
Big Bang Nucleosynthesis George Gamow (1904-1968) 5 t dec ~10 yr T dec 0.26 ev Neutrons-protons inter-converting processes At the equilibrium: Equilibrium holds until 0 t ~14 Gyr Freeze-out temperature
More informationBaryogenesis and dark matter in the nmssm
Baryogenesis and dark matter in the nmssm C.Balázs, M.Carena, A. Freitas, C.Wagner Phenomenology of the nmssm from colliders to cosmology arxiv:0705431 C. Balázs, Monash U Melbourne BG & DM in the nmssm
More informationSUPERSYMETRY FOR ASTROPHYSICISTS
Dark Matter: From the Cosmos to the Laboratory SUPERSYMETRY FOR ASTROPHYSICISTS Jonathan Feng University of California, Irvine 29 Jul 1 Aug 2007 SLAC Summer Institute 30 Jul 1 Aug 07 Feng 1 Graphic: N.
More informationHidden Sector Baryogenesis. Jason Kumar (Texas A&M University) w/ Bhaskar Dutta (hep-th/ ) and w/ B.D and Louis Leblond (hepth/ )
Hidden Sector Baryogenesis Jason Kumar (Texas A&M University) w/ Bhaskar Dutta (hep-th/0608188) and w/ B.D and Louis Leblond (hepth/0703278) Basic Issue low-energy interactions seem to preserve baryon
More informationBaryogenesis. David Morrissey. SLAC Summer Institute, July 26, 2011
Baryogenesis David Morrissey SLAC Summer Institute, July 26, 2011 Why is There More Matter than Antimatter? About 5% of the energy density of the Universe consists of ordinary (i.e. non-dark) matter. By
More informationStatus and Phenomenology of the Standard Model
Status and Phenomenology of the Standard Model The new standard model Experimental tests, unique features, anomalies, hints of new physics Precision tests Higgs Heavy quarks Neutrinos FCNC and EDMs Astrophysics
More informationHiggs Physics. Yasuhiro Okada (KEK) November 26, 2004, at KEK
Higgs Physics Yasuhiro Okada (KEK) November 26, 2004, at KEK 1 Higgs mechanism One of two principles of the Standard Model. Gauge invariance and Higgs mechanism Origin of the weak scale. Why is the weak
More informationAspetti della fisica oltre il Modello Standard all LHC
Aspetti della fisica oltre il Modello Standard all LHC (con enfasi sulla verificabilità sperimentale in gruppo I e II) Andrea Romanino SISSA e INFN TS Giornata di Seminari, INFN TS, 07.07.09 The Standard
More informationLight Pseudoscalar Higgs boson in NMSSM
K. Cheung 1 Light Pseudoscalar Higgs boson in NMSSM Kingman Cheung NTHU, December 2006 (with Abdesslam Arhrib, Tie-Jiun Hou, Kok-Wee Song, hep-ph/0606114 K. Cheung 2 Outline Motivations for NMSSM The scenario
More informationBeyond the Standard Paradigm
Beyond the Standard Paradigm The standard paradigm or a landscape? Heavy Z Extended Higgs Neutralinos Quasi-chiral exotics References J. Kang, P. Langacker, T. j. Li and T. Liu, Electroweak baryogenesis
More informationNeutralino dark matter in the NMSSM
Neutralino dark matter in the NMSSM Ana M. Teixeira (LPT - Orsay) XLII Rencontres de Moriond La Thuile, Italy, 4 March 27 In collaboration with Cerdeño, Gabrielli, Hugonie, López-Fogliani and Muñoz Discussion
More informationThe first one second of the early universe and physics beyond the Standard Model
The first one second of the early universe and physics beyond the Standard Model Koichi Hamaguchi (University of Tokyo) @ Colloquium at Yonsei University, November 9th, 2016. Credit: X-ray: NASA/CXC/CfA/M.Markevitch
More informationSplit SUSY and the LHC
Split SUSY and the LHC Pietro Slavich LAPTH Annecy IFAE 2006, Pavia, April 19-21 Why Split Supersymmetry SUSY with light (scalar and fermionic) superpartners provides a technical solution to the electroweak
More informationDark Matter Implications for SUSY
Dark Matter Implications for SUSY Sven Heinemeyer, IFCA (CSIC, Santander) Madrid, /. Introduction and motivation. The main idea 3. Some results 4. Future plans Sven Heinemeyer, First MultiDark workshop,
More informationModels of Neutrino Masses
Models of Neutrino Masses Fernando Romero López 13.05.2016 1 Introduction and Motivation 3 2 Dirac and Majorana Spinors 4 3 SU(2) L U(1) Y Extensions 11 4 Neutrino masses in R-Parity Violating Supersymmetry
More informationInverse See-saw in Supersymmetry
Inverse See-saw in Supersymmetry Kai Wang IPMU, the University of Tokyo Cornell Particle Theory Seminar September 15, 2010 hep-ph/10xx.xxxx with Seong-Chan Park See-saw is perhaps the most elegant mechanism
More informationYukawa and Gauge-Yukawa Unification
Miami 2010, Florida Bartol Research Institute Department Physics and Astronomy University of Delaware, USA in collaboration with Ilia Gogoladze, Rizwan Khalid, Shabbar Raza, Adeel Ajaib, Tong Li and Kai
More informationCP Violation, Baryon violation, RPV in SUSY, Mesino Oscillations, and Baryogenesis
CP Violation, Baryon violation, RPV in SUSY, Mesino Oscillations, and Baryogenesis David McKeen and AEN, arxiv:1512.05359 Akshay Ghalsasi, David McKeen, AEN., arxiv:1508.05392 (Thursday: Kyle Aitken, David
More informationSupersymmetry, Dark Matter, and Neutrinos
Supersymmetry, Dark Matter, and Neutrinos The Standard Model and Supersymmetry Dark Matter Neutrino Physics and Astrophysics The Physics of Supersymmetry Gauge Theories Gauge symmetry requires existence
More informationElectroweak baryogenesis as a probe of new physics
Electroweak baryogenesis as a probe of new physics Eibun Senaha (Nagoya U) HPNP25@Toyama U. February 3, 25 Outline Introduction Overview of electroweak baryogenesis (EWBG) Current status EWBG in SUSY models
More informationThe Standard Model and Beyond
The Standard Model and Beyond Nobuchika Okada Department of Physics and Astronomy The University of Alabama 2011 BCVSPIN ADVANCED STUDY INSTITUTE IN PARTICLE PHYSICS AND COSMOLOGY Huê, Vietnam, 25-30,
More informationStatus Report on Electroweak Baryogenesis
Outline Status Report on Electroweak Baryogenesis Thomas Konstandin KTH Stockholm hep-ph/0410135, hep-ph/0505103, hep-ph/0606298 Outline Outline 1 Introduction Electroweak Baryogenesis Approaches to Transport
More informationProperties of the Higgs Boson, and its interpretation in Supersymmetry
Properties of the Higgs Boson, and its interpretation in Supersymmetry U. Ellwanger, LPT Orsay The quartic Higgs self coupling and Supersymmetry The Next-to-Minimal Supersymmetric Standard Model Higgs
More informationMaria Dimou In collaboration with: C. Hagedorn, S.F. King, C. Luhn. Tuesday group seminar 17/03/15 University of Liverpool
Maria Dimou In collaboration with: C. Hagedorn, S.F. King, C. Luhn Tuesday group seminar 17/03/15 University of Liverpool 1 Introduction Outline The SM & SUSY Flavour Problem. Solving it by imposing a
More informationUnification without Doublet-Triplet Splitting SUSY Exotics at the LHC
Unification without Doublet-Triplet Splitting SUSY Exotics at the LHC Jürgen Reuter Albert-Ludwigs-Universität Freiburg W. Kilian, JR, PLB B642 (2006), 81; and work in progress (with F. Deppisch, W. Kilian)
More informationStatus of low energy SUSY models confronted with the 125 GeV Higgs data
Status of low energy SUSY models confronted with the 5 GeV Higgs data Junjie Cao On behalf of my collaborators J. M. Yang, et al Based on our works arxiv: 7.3698, 6.3865, 3.3694,.58,.439 junjiec@itp.ac.cn
More informationModels of New Physics for Dark Matter
Models of New Physics for Dark Matter Carlos Muñoz instituto de física teórica ift-uam/csic departamento de física teórica dft-uam 1 PPC 2010, Torino, July 12-16 Crucial Moment for SUSY in next few years:
More informationThe SCTM Phase Transition
The SCTM Phase Transition ICTP / SAIFR 2015 Mateo García Pepin In collaboration with: Mariano Quirós Motivation The Model The phase transition Summary EW Baryogenesis A mechanism to explain the observed
More informationSupersymmetry at the LHC
Supersymmetry at the LHC What is supersymmetry? Present data & SUSY SUSY at the LHC C. Balázs, L. Cooper, D. Carter, D. Kahawala C. Balázs, Monash U. Melbourne SUSY@LHC.nb Seattle, 23 Sep 2008 page 1/25
More informationF. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King. arxiv:
F. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King S FLASY 2015 arxiv:1503.03306 Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y SM:
More informationNeutrinos: status, models, string theory expectations
Neutrinos: status, models, string theory expectations Introduction Neutrino preliminaries and status Models String embeddings Intersecting brane The Z 3 heterotic orbifold Embedding the Higgs triplet Outlook
More informationA model of the basic interactions between elementary particles is defined by the following three ingredients:
I. THE STANDARD MODEL A model of the basic interactions between elementary particles is defined by the following three ingredients:. The symmetries of the Lagrangian; 2. The representations of fermions
More informationLittle Higgs Models Theory & Phenomenology
Little Higgs Models Theory Phenomenology Wolfgang Kilian (Karlsruhe) Karlsruhe January 2003 How to make a light Higgs (without SUSY) Minimal models The Littlest Higgs and the Minimal Moose Phenomenology
More informationThe Standard Model of particle physics and beyond
The Standard Model of particle physics and beyond - Lecture 3: Beyond the Standard Model Avelino Vicente IFIC CSIC / U. Valencia Physics and astrophysics of cosmic rays in space Milano September 2016 1
More informationHigher dimensional operators. in supersymmetry
I. Antoniadis CERN Higher dimensional operators in supersymmetry with E. Dudas, D. Ghilencea, P. Tziveloglou Planck 2008, Barcelona Outline Effective operators from new physics integrating out heavy states
More informationDynamical Solution to the µ/b µ Problem in Gauge Mediated Supersymmetry Breaking
Dynamical Solution to the µ/b µ Problem in Gauge Mediated Supersymmetry Breaking Carlos E.M. Wagner EFI and KICP, University of Chicago HEP Division, Argonne National Lab. Work done in collaboration with
More informationDecember 10, :42 World Scientific Review Volume - 9in x 6in zpr 09. Chapter 1
Chapter 1 Z Physics and Supersymmetry M. Cvetič Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104-6396 P. Langacker School of Natural Sciences, Institute for Advanced
More informationAlternatives to the GUT Seesaw
Alternatives to the GUT Seesaw Motivations Higher-dimensional operators String instantons Other (higher dimensions, Higgs triplets) Motivations Many mechanisms for small neutrino mass, both Majorana and
More informationLeptogenesis with type II see-saw in SO(10)
Leptogenesis wit type II see-saw in SO(10) Andrea Romanino SISSA/ISAS Frigerio Hosteins Lavignac R, arxiv:0804.0801 Te baryon asymmetry η B n B n B n γ = n B n γ Generated dynamically if = (6.15 ± 0.5)
More informationExceptional Supersymmetry. at the Large Hadron Collider
Exceptional Supersymmetry at the Large Hadron Collider E 6 SSM model and motivation Contents Why go beyond the Standard Model? Why consider non-minimal SUSY? Exceptional SUSY Structure, particle content
More informationarxiv:hep-ph/ v1 24 Jun 2003
hep-ph/0306240 FTPI MINN 03/14 UMN TH 2203/04 CERN TH/2003 121 CP Violation in Supersymmetric U1) Models arxiv:hep-ph/0306240v1 24 Jun 2003 Durmuş A. Demir 1 and Lisa L. Everett 2 1 William I. Fine Theoretical
More informationThe first year of the LHC and Theory. G.G.Ross, Krakow, December 09
The first year of the LHC and Theory G.G.Ross, Krakow, December 09 The LHC a discovery machine The gauge sector : new gauge bosons? The maber sector : new quarks and leptons? The scalar sector : the hierarchy
More informationgeneration Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion Nejc Košnik
th Discovery Discovery of of the the 4 4th generation generation Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion 1 Introduction Introduction
More informationPseudo-Dirac Bino as Dark Matter and Signatures of D-Type G
and Signatures of D-Type Gauge Mediation Ken Hsieh Michigan State Univeristy KH, Ph. D. Thesis (2007) ArXiv:0708.3970 [hep-ph] Other works with M. Luty and Y. Cai (to appear) MSU HEP Seminar November 6,
More information+ µ 2 ) H (m 2 H 2
I. THE HIGGS POTENTIAL AND THE LIGHT HIGGS BOSON In the previous chapter, it was demonstrated that a negative mass squared in the Higgs potential is generated radiatively for a large range of boundary
More informationKaluza-Klein Theories - basic idea. Fig. from B. Greene, 00
Kaluza-Klein Theories - basic idea Fig. from B. Greene, 00 Kaluza-Klein Theories - basic idea mued mass spectrum Figure 3.2: (Taken from [46]). The full spectrum of the UED model at the first KK level,
More informationU(1) Gauge Extensions of the Standard Model
U(1) Gauge Extensions of the Standard Model Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA U(1) Gauge Extensions of the Standard Model (int08) back to start
More informationPati-Salam GUT-Flavour Models with Three Higgs Generations
Pati-Salam GUT-Flavour Models with Three Higgs Generations Florian Hartmann in collaboration with Wolfgang Kilian and Karsten Schnitter based on: JHEP 1405 (2014) 064 and arxiv:1405.1901 Universität Siegen
More informationBaryogenesis and Particle Antiparticle Oscillations
Baryogenesis and Particle Antiparticle Oscillations Seyda Ipek UC Irvine SI, John March-Russell, arxiv:1604.00009 Sneak peek There is more matter than antimatter - baryogenesis SM cannot explain this There
More informationStau Pair Production At The ILC Tohoku University Senior Presentation Tran Vuong Tung
e + Z*/γ τ + e - τ Stau Pair Production At The ILC Tohoku University Senior Presentation Tran Vuong Tung 1 Outline Introduction of the International Linear Collider (ILC) Introduction of (g μ -2) in the
More informationBeyond the SM: SUSY. Marina Cobal University of Udine
Beyond the SM: SUSY Marina Cobal University of Udine Why the SM is not enough The gauge hierarchy problem Characteristic energy of the SM: M W ~100 GeV Characteristic energy scale of gravity: M P ~ 10
More informationWhither SUSY? G. Ross, Birmingham, January 2013
Whither SUSY? G. Ross, Birmingham, January 2013 whither Archaic or poetic adv 1. to what place? 2. to what end or purpose? conj to whatever place, purpose, etc. [Old English hwider, hwæder; related to
More informationSupersymmetry Basics. J. Hewett SSI J. Hewett
Supersymmetry Basics J. Hewett SSI 2012 J. Hewett Basic SUSY References A Supersymmetry Primer, Steve Martin hep-ph/9709356 Theory and Phenomenology of Sparticles, Manual Drees, Rohini Godbole, Probir
More informationMaking Neutrinos Massive with an Axion in Supersymmetry
UCRHEP-T300 February 2001 arxiv:hep-ph/0102008v1 1 Feb 2001 Making Neutrinos Massive with an Axion in Supersymmetry Ernest Ma Physics Department, University of California, Riverside, California 92521 Abstract
More informationHiggs Physics and Cosmology
Higgs Physics and Cosmology Koichi Funakubo Department of Physics, Saga University 1 This year will be the year of Higgs particle. The discovery of Higgs-like boson will be reported with higher statistics
More informationCrosschecks for Unification
Crosschecks for Unification Hans Peter Nilles Physikalisches Institut Universität Bonn Crosschecks for Unification, Planck09, Padova, May 2009 p. 1/39 Questions Do present observations give us hints for
More informationPhysics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002
Physics at e + e - Linear Colliders 4. Supersymmetric particles M. E. Peskin March, 2002 In this final lecture, I would like to discuss supersymmetry at the LC. Supersymmetry is not a part of the Standard
More informationLecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model
Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,
More informationRelating the Baryon Asymmetry to WIMP Miracle Dark Matter
Brussels 20/4/12 Relating the Baryon Asymmetry to WIMP Miracle Dark Matter PRD 84 (2011) 103514 (arxiv:1108.4653) + PRD 83 (2011) 083509 (arxiv:1009.3227) John McDonald, LMS Consortium for Fundamental
More informationHeterotic Supersymmetry
Heterotic Supersymmetry Hans Peter Nilles Physikalisches Institut Universität Bonn Heterotic Supersymmetry, Planck2012, Warsaw, May 2012 p. 1/35 Messages from the heterotic string Localization properties
More informationSupersymmetry at the LHC
Supersymmetry at the LHC What is supersymmetry? Present data & SUSY SUSY at the LHC C. Balázs L. Cooper D. Carter D. Kahawala C. Balázs, Monash U. Melbourne SUSY@LHC.nb Beijing, 8 Oct 2008 page 1/25 What
More informationLHC Phenomenology of SUSY multi-step GUTs
0/14 J. Reuter LHC Phenomenology of SUSY multi-step GUTs PHENO 09, Madison, 1.5.009 LHC Phenomenology of SUSY multi-step GUTs Jürgen Reuter Albert-Ludwigs-Universität Freiburg W. Kilian, JR, PL B64 (006),
More informationHidden two-higgs doublet model
Hidden two-higgs doublet model C, Uppsala and Lund University SUSY10, Bonn, 2010-08-26 1 Two Higgs doublet models () 2 3 4 Phenomenological consequences 5 Two Higgs doublet models () Work together with
More informationFoundations of Physics III Quantum and Particle Physics Lecture 13
Foundations of Physics III Quantum and Particle Physics Lecture 13 Frank Krauss February 27, 2012 1 Construction of the Standard Model 2 The Standard Model: Tests and status 3 Beyond the Standard Model?
More informationSUSY PHENOMENOLOGY. A Dissertation BO HU
SUSY PHENOMENOLOGY A Dissertation by BO HU Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY August 2004
More informationWho is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential)
Who is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential) Satoshi Iso (KEK, Sokendai) Based on collaborations with H.Aoki (Saga) arxiv:1201.0857
More information