Electroweak Baryogenesis
|
|
- Kristian Fisher
- 5 years ago
- Views:
Transcription
1 Electroweak Baryogenesis Eibun Senaha (KIAS) Feb. 13, 2013 of Toyama
2 Outline Motivation Electroweak baryogenesis (EWBG) sphaleron decoupling condition strong 1 st order EW phase transition (PT) Triple Higgs bosons coupling as a probe of EWBG 2HDM, MSSM Summary
3 Baryon Asymmetry of the Universe (BAU) Our Universe is baryon-asymmetric. /0(+ /0(* /0//) ' "# ( /0/. /0/( /0/! /0() η n B n γ = n b n b n γ =( ) (95% CL) D & BBB A " /0(' /0(!./!./ ' A$"% & If the BAU is generated before T O(1) MeV, the light element abundances (D, 3 He, 4 He, 7 Li) can be explained by the standard Big-Bang cosmology. + C=$"%&./ )./ - )! "#$"% & Baryogenesis = generate right η (././. (! ' ) * +, -./ :;8:&<8;89%65;=8%η././ gure 20.1: The abundances of He, D, He, and Li as predicted by the standa [PDG 2012]
4 Sakharov s criteria To get the BAU from initially baryon symmetric Universe, the following conditions must be satisfied. [Sakharov, 67] (1) Baryon number (B) violation (2) C and CP violation (3) Out of equilibrium BAU must arise After inflation (scale is model-dependent) Before Big-Bang Nucleosynthesis (T 1 MeV). What kind of model can satisfy these conditions?
5 Many possibilities [Shaposhnikov, J.Phys.Conf.Ser.171:012005,2009.] 1. GUT baryogenesis. 2. GUT baryogenesis after preheating. 3. Baryogenesis from primordial black holes. 4. String scale baryogenesis. 5. Affleck-Dine (AD) baryogenesis. 6. Hybridized AD baryogenesis. 7. No-scale AD baryogenesis. 8. Single field baryogenesis. 9. Electroweak (EW) baryogenesis. 10. Local EW baryogenesis. 11. Non-local EW baryogenesis. 12. EW baryogenesis at preheating. 13. SUSY EW baryogenesis. 14. String mediated EW baryogenesis. 15. Baryogenesis via leptogenesis. 16. Inflationary baryogenesis. 17. Resonant leptogenesis. 18. Spontaneous baryogenesis. 19. Coherent baryogenesis. 20. Gravitational baryogenesis. 21. Defect mediated baryogenesis. 22. Baryogenesis from long cosmic strings. 23. Baryogenesis from short cosmic strings. 24. Baryogenesis from collapsing loops. 25. Baryogenesis through collapse of vortons. 26. Baryogenesis through axion domain walls. 27. Baryogenesis through QCD domain walls. 28. Baryogenesis through unstable domain walls. 29. Baryogenesis from classical force. 30. Baryogenesis from electrogenesis. 31. B-ball baryogenesis. 32. Baryogenesis from CPT breaking. 33. Baryogenesis through quantum gravity. 34. Baryogenesis via neutrino oscillations. 35. Monopole baryogenesis. 36. Axino induced baryogenesis. 37. Gravitino induced baryogenesis. 38. Radion induced baryogenesis. 39. Baryogenesis in large extra dimensions. 40. Baryogenesis by brane collision. 41. Baryogenesis via density fluctuations. 42. Baryogenesis from hadronic jets. 43. Thermal leptogenesis. 44. Nonthermal leptogenesis. Electroweak baryogenesis (EWBG) is testable. directly linked to the low energy observables, e.g. Higgs physics.
6 Electroweak baryogenesis B violation: anomalous process (sphaleron) C violation: chiral gauge interaction [Kuzmin, Rubakov, Shaposhnikov, PLB155,36 ( 85) ] Sakharov s conditions CP violation: Kobayashi-Maskawa (KM) phase and other complex phases in the beyond the SM Out of equilibrium: 1 st order EW phase transition (EWPT) with expanding bubble walls symmetric phase broken phase BAU can arise by the growing bubbles.
7 Esph Energy sphaleron rates (/time/volume): (B+L) transition (B+L) current is violated by the quantum anomaly. But (B-L) is conserved. N CS (t) = 1 32π 2 sphaleron instanton Tunneling probability: Γ instanton e 2S instanton = e 16π2 /g sphaleron = static saddle point solution with finite energy of the gauge-higgs system. broken phase : thermal activation tunneling Ncs d 3 x ijk g 2Tr F 2 ij A k 23 g 2A i A j A k g 21B ij B k Γ (b) sph T 4 e E sph/t, symmetric phase : Γ (s) sph κ(α W T ) 4, 1 gen., 0 u L d L d L ν el N g N g gen., 0 (3qL i + ll) i unobservable! [N.S. Manton, PRD28 ( 83) 2019] α W = g 2 2/(4π), κ= O(1) (B+L)-violating process is active at finite T but is suppressed at T=0. e.g. Δ(B+L) 0 low T: tunneling high T: thermal activation i=1 left-handed fermion only
8 Baryogenesis mechanism (3) (1) (2) H:Hubble constant n B 0 start with zero baryon number. n B =0 n B (1) (2) (3) Φ =0 CP n B Φ =0 B+L n B Φ =0 n R b n R b n R b n R b n B =0 n B = n L b n L b =0 n L b n L b + n R b n R b =0 =0 n B = n L b n L b n L b n L b by Γ (s) B (>H) + n R b n R b n B =0 changed B =+1 e.g.,1 gen. ū L d L d L ν el L =+1 Γ (b) B <H is needed. If Γ (b) B >H n B 0
9 Γ (b) B <H B-changing rate in the broken phase is E sph is a sphaleron energy which is proportional to Higgs VEV Γ (b) B (T ) (prefactor)γ(b) sph T 3 (prefactor)e E sph/t, E sph v what we need: large Higgs VEV after the EWPT -> EWPT should be strongly 1 st order. sphaleron decoupling condition gives strong constraints on Higgs sector. In most cases, collider signals of EWBG is consequence of this condition.
10 More on Γ (b) B <H After the EWPT, the sphaleron process must be decoupled. Γ (b) B (T ) (prefactor)e E sph/t <H(T ) 1.66 g T 2 /m P g massless dof, (SM) m P Planck mass 1.22x10 19 GeV E sph =4πvE/g 2 (g 2 : SU(2) gauge coupling), v T > g log corrections 4πE sphaleron energy gives the dominant effect. log corrections are subleading. Commonly, the sphaleron decoupling condition is evaluated at a critical temperature (Tc.).
11 Sphaleron energy For simplicity, we evaluate sphaleron energy at T=0. We take SM as an example. (U(1) Y is neglected) L = 1 4 F a µνf aµν +(D µ Φ) D µ Φ V 0 (Φ) V 0 (Φ) = λ Φ Φ v2 sphaleron energy: 2 2 E sph = 4πv g 2 E [Klinkhammer and Manton, PRD30, ( 84) 2212] Higgs mass (λ) -> E sph For m h = 126 GeV (λ =0.13), E1.92 v T > 1.16
12 SM EWBG It turned out that the SM EWBG was ruled out. KM phase is too small to generate the observed BAU. [Gavela et al, NPB430,382 ( 94); Huet and Sather, PRD51,379 ( 95).] 130 The Standard Model crossover i EWPT is a crossover for m H >73 GeV. 120 symmetric phase f..." [Kajantie at al, PRL77,2887 ( 96); Rummukainen et al, NPB532,283 ( 98); Csikor et al, PRL82, 21 ( 99); Aoki et al, PRD60, ( 99), Laine et al, NPB73,180( 99)] (LHC exp., m H =126GeV) > [.~ ll st order... 2nd order endpoint 2 nd order end point -> New Physics is required i L i mh/gev Many directions to go: SUSY models or non-susy models etc.
13 1 st and 2 nd order EWPTs This is what the 1 st and 2 nd order PTs look like. order parameter = Higgs VEV EWBG requires 1 st order PT [From K. Funakubo s slide]
14 1 st and 2 nd order EWPTs This is what the 1 st and 2 nd order PTs look like. order parameter = Higgs VEV EWBG requires 1 st order PT A negative contributions is necessary. [From K. Funakubo s slide]
15 1 st and 2 nd order EWPTs This is what the 1 st and 2 nd order PTs look like. order parameter = Higgs VEV EWBG requires 1 st order PT A negative contributions is necessary. e.g. Bosonic thermal loop [From K. Funakubo s slide] V (boson) 1 const m(v) 3/2 T
16 SM EWPT at 1-loop order Veff V eff D(T 2 T 2 0 )ϕ 2 ET ϕ 3 + λ T 4 ϕ4 T =TC λ TC 4 ϕ2 (ϕ v C ) 2 0 T>Tc T=Tc T<Tc (GeV) sphaleron decoupling condition T C is defined at which V eff has two degerate minima. 1 st order EWPT is realized by the boson loops E SM 1 4πv 3 (2m3 W + m 3 Z) 0.01 v C = 2ET C λ TC v C T C = 2E λ TC λ TC λ = m 2 h SM /(2v 2 ) Γ (b) B <H v C T C > 1 = m h SM < 48 GeV excluded by LEP way out: enhance E by adding new bosons. = cubic coeff. quartic coeff.
17 SM EWPT at 1-loop order Veff V eff D(T 2 T 2 0 )ϕ 2 ET ϕ 3 + λ T 4 ϕ4 T =TC λ TC 4 ϕ2 (ϕ v C ) 2 0 T>Tc T=Tc T<Tc (GeV) sphaleron decoupling condition T C is defined at which V eff has two degerate minima. 1 st order EWPT is realized by the boson loops E SM 1 4πv 3 (2m3 W + m 3 Z) 0.01 v C = 2ET C λ TC v C T C = 2E λ TC λ TC λ = m 2 h SM /(2v 2 ) Γ (b) B <H v C T C > 1 = m h SM < 48 GeV excluded by LEP way out: enhance E by adding new bosons. = cubic coeff. quartic coeff.
18 SM EWPT at 1-loop order Veff V eff D(T 2 T 2 0 )ϕ 2 ET ϕ 3 + λ T 4 ϕ4 T =TC λ TC 4 ϕ2 (ϕ v C ) 2 0 T>Tc T=Tc T<Tc (GeV) sphaleron decoupling condition T C is defined at which V eff has two degerate minima. 1 st order EWPT is realized by the boson loops E SM 1 4πv 3 (2m3 W + m 3 Z) 0.01 v C = 2ET C λ TC v C T C = 2E λ TC λ TC λ = m 2 h SM /(2v 2 ) Γ (b) B <H v C T C > 1 = m h SM < 48 GeV excluded by LEP way out: enhance E by adding new bosons. = cubic coeff. quartic coeff.
19 SM EWPT at 1-loop order Veff V eff D(T 2 T 2 0 )ϕ 2 ET ϕ 3 + λ T 4 ϕ4 T =TC λ TC 4 ϕ2 (ϕ v C ) 2 0 T>Tc T=Tc T<Tc (GeV) sphaleron decoupling condition T C is defined at which V eff has two degerate minima. 1 st order EWPT is realized by the boson loops E SM 1 4πv 3 (2m3 W + m 3 Z) 0.01 v C = 2ET C λ TC v C T C = 2E λ TC λ TC λ = m 2 h SM /(2v 2 ) Γ (b) B <H v C T C > 1 = m h SM < 48 GeV excluded by LEP way out: enhance E by adding new bosons. = cubic coeff. quartic coeff.
20 Caveat Scalar does not always play a roll. Suppose the scalar mass is given by m 2 = M 2 + λv 2 M : M 2 λv 2 nondecoupling decoupling λ : V eff λ 3/2 T v 3 M 2 λv 2 V eff M 3 T mass parameter in the Lagrangian coupling between Higgs and a scalar 3/2 1+ M 2 λv 2 1+ λv2 M 2 3/2 contribute does not requirements: 1. large coupling λ, 2. small M nondecoupling scalar E = E SM + E v C T C
21 Triple Higgs boson coupling as a probe of EWBG EWBG signal can appear in the triple Higgs boson coupling.
22 2 Higgs doublet model (2HDM) Additional Higgs doublet is added to the SM Higgs sector. To suppress the FCNC processes, Z 2 symmetry is imposed Higgs potential Φ 1 Φ 1, Φ 2 Φ 2 (Type I, II etc) V 2HDM = m 2 1Φ 1 Φ 1 + m 2 2Φ 2 Φ 2 (m 2 3Φ 1 Φ 2 + h.c.) + λ 1 2 (Φ 1 Φ 1) 2 + λ 2 2 (Φ 2 Φ 2) 2 + λ 3 (Φ 1 Φ 1) 2 (Φ 2 Φ 2) 2 + λ 4 (Φ 1 Φ 2) 2 (Φ 2 Φ 1) 2 λ5 + 2 (Φ 1 Φ 2) 2 charged Higgs + h.c., φ + i Φ 1,2 (x) = (x) 1. 2 v i + h i (x)+ia i (x) m 2 3,λ 5 C Higgs VEV 6 free parameters (v and m h are known.) m h, m H, m A, m H ± α : mixing angle between h and H tan β = v 2 /v 1, (v = v v GeV) CP-even Higgs CP-odd Higgs M 2 = m 2 3/(sin β cos β)
23 Quantum corrections to hhh coupling Loop corrections of heavy Higgs bosons [S. Kanemura, S. Kiyoura, Y. Okada, E.S., C.-P. Yuan, PLB558 (2003) 157] h h h For sin(β α) = 1 λ 2HDM hhh 3m2 h v 1+ (SM-like limit) Φ=H,A,H ± c 12π 2 m 4 Φ m 2 h v2 1 M 2 m 2 Φ 3 c=1(2) for neutral (charged Higgs bosons) 2 kinds of large mass limits m 2 Φ M 2 + λ i v 2. For M 2 λ i v 2 (m 2 Φ λ iv 2 ), the quantum corrections would grow with m 4 Φ. nondecoupling limit (coupling constants get large) For M 2 λ i v 2 (m 2 Φ M 2 ), the quantum corrections would be suppressed. ordinary decoupling limit (1/mass) Loop corrections are sizable if the heavy Higgs bosons have nondecoupling property. (Successful EWBG enforces the former limit.)
24 Correlation between Δλhhh/λ SM hhh and vc/tc [S. Kanemura, Y. Okada, E.S.,PLB606 (2005) 361] Contour plot of hhh / hhh and c /T c in the m -M plane 100 % % EWPT is strongly m (GeV) % 20 % 30 % 1 st order hhh/ hhh = 5% sin( - ) = -1, tan = 1 50 mh = 120 GeV m = mh = ma = mh M (GeV) c/tc = 1 Heavy Higgs boson loops enhance the 1 st order EWPT E 2HDM For vc/tc>1, Δλhhh/λ SM hhh is greater than (10-20)%.
25 How about the MSSM?
26 Light stop scenario [Carena, Quiros, Wagner, PLB380 ( 96) 81] requirements: 1. large coupling λ, 2. small M top Yukawa small soft SUSY mass LEP bound on m H ρ parameter stop mass m 2 t 2 m 2 t 1 = m 2 q + y2 t sin 2 β 2 = m 2 t R + y2 t sin 2 β 2 m 2 q m 2 t R,X 2 t, X t = A t µ/ tan β. 1+ X t 2 v 2 + O(g 2 ) m 2 q, m 2 q 1 X t 2 v 2 + O(g 2 ). m 2 q At finite T, there is a thermal correction, T m 2 t R O(T 2 ) > 0. To have a large loop effect, m 2 t R + T m 2 t R m 2 t R (T ) m 2 t R + T m 2 t R =0 m 2 t R < 0 must be small. Charge-Color-Breaking vacuum m t 1 <m t light stop is needed!! X t = 0 (no-mixing) maximizes the loop effect
27 Δλhhh/λ SM hhh Coefficient of cubic term in Veff(T) V eff (E SM + E t 1 )Tv 3 E t 1 + y3 t sin 3 β 4 2π Deviation of hhh coupling λ MSSM hhh λ SM hhh m 4 t 2π 2 v 2 m 2 h 1 X t 2 1 X t 2 m 2 q For m h = 126 GeV, tan β = 10, X t =0 m 2 q 3 = 3/2. 2v4 m 2 t m 2 h (E t 1 ) 2 λ MSSM hhh λ SM hhh 0.05 Size of the loop effect is fixed by the top Yukawa coupling. SUSY models based on the strong dynamics can have a larger coupling constant, so the deviation can be larger. (Toshifumi Yamada s talk)
28 Current status of MSSM EWBG t 1 = mostly right-handed. EWPT can be strong 1 st order if m H < 127 GeV, m t 1 < 120 GeV [M. Carena, G. Nardini, M. Quiros, CEM. Wagner, NPB812, (2009) 243] This light stop scenario is now in tension with the current LHC data. In this scenario, σ(gg -> H), Γ(H->γγ), Γ(H->VV) has no drastic change. Enhanced σ(gg -> H -> VV) is not favored by the LHC data. [D. Curtin, P. Jaiswall, P. Meade., arxiv: ] For mh 125 GeV, MSSM EWBG is ruled out at greater than 98% CL (ma>1 TeV), at least 90% CL for light value of ma (~300 GeV) loophole [M. Carena, G. Nardini, M. Quiros, CEM. Wagner, arxiv: ] If m χ 0 1 < 60 GeV, Higgs invisible decay mode is open. reduce σ(gg -> H -> VV) tension may be loosen. MSSM EWBG is not fully excluded but is more and more unlikely.
29 Beyond the MSSM Next-to-MSSM (NMSSM) nearly-mssm (nmssm) W NMSSM λsh u H d + κ 3 S3 W nmssm λsh u H d + m2 12 λ S U(1) -extended-mssm (UMSSM) W UMSSM λsh u H d 1 st order EWPT is driven by singlet Higgs 4 Higgs doublets+singlets-extended MSSM (Toshifumi Yamada s talk) W = λ H d Φ u ζ + H u Φ d η H u Φ u Ω H d Φ d Ω + + n Φ Φ u Φ d + n Ω (Ω + Ω ζη) µ(h u H d n Φ n Ω ) µ Φ Φ u Φ d µ Ω (Ω + Ω ζη). 1 st order EWPT is driven by extra charged Higgs In the beyond the MSSM, the light stop is not necessarily required to have the strong 1 st order EWPT.
30 SM EWBG was ruled out. Summary Nondecoupling scalar is one of the possibilities to overcome the issue. Triple Higgs boson coupling is useful for probing the signal of EWBG. 2HDM: Δλhhh/λ SM hhh is greater than (10-20)% if the EWTP is strong 1st order. symmetric phase broken phase EW baryogenesis Large corrections to λ hhh MSSM EWBG is not fully excluded but is more and more unlikely due to the recent LHC data. (light stop scenario is not favored.) In the beyond the MSSM (e.g. NMSSM etc.), the light stop is not necessarily required to have the strong 1 st order EWPT.
31 Outlook To have the strong 1st order EWPT, the Higgs sector must be modified. Most of the EWBG scenarios would be tested by the LHC data., especially by σ Br (σ Br) SM Tree-level mixing driven 1 st order PT scenarios driven by (S inert) -> universal reduction of signal strengths. λ HS S 2 H 2 Thermal cubic term driven scenarios -colored scalar loop -> enhancement of σ(gg -> H) -charged scalar loop -> reduction of Γ(H->γγ)
Electroweak 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 informationHiggs physics as a probe of electroweak baryogenesis
Higgs physics as a probe of electroweak baryogenesis Eibun Senaha (NCU) @Kavli IPMU, May 27, 205. Outline Introduction! Review of electroweak baryogenesis (EWBG)! Real singlet-extended SM (rsm)! Electroweak
More informationElectroweak Baryogenesis and the triple Higgs boson coupling
Electroweak Baryogenesis and te triple Higgs boson coupling Eibun Senaa (Grad. Univ. Advanced Studies, KEK) Mar. 18-22, 2005, LCWS 05 @Stanford U. in collaboration wit Sinya Kanemura (Osaka U) Yasuiro
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 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 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 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 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 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 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 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 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 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 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 informationImplications of a Heavy Z Gauge Boson
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 References T. Han, B. McElrath, PL, hep-ph/0402064
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 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 informationThe Origin of Matter. Koichi Funakubo Dept. Physics Saga University. NASA Hubble Space Telescope NGC 4911
The Origin of Matter Koichi Funakubo Dept. Physics Saga University NASA Hubble Space Telescope NGC 4911 fundamental theory of elementary particles Local Quantum Field Theory causality relativistic quantum
More informationA biased review of Leptogenesis. Lotfi Boubekeur ICTP
A biased review of Leptogenesis Lotfi Boubekeur ICTP Baryogenesis: Basics Observation Our Universe is baryon asymmetric. n B s n b n b s 10 11 BAU is measured in CMB and BBN. Perfect agreement with each
More informationMatter vs Anti-matter
Baryogenesis Matter vs Anti-matter Earth, Solar system made of baryons B Our Galaxy Anti-matter in cosmic rays p/p O(10 4 ) secondary Our Galaxy is made of baryons p galaxy p + p p + p + p + p galaxy γ
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 informationProbing the Majorana nature in radiative seesaw models at collider experiments
Probing the Majorana nature in radiative seesaw models at collider experiments Shinya KANEMURA (U. of Toyama) M. Aoki, SK and O. Seto, PRL 102, 051805 (2009). M. Aoki, SK and O. Seto, PRD80, 033007 (2009).
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 informationElectroweak Baryogenesis A Status Report
Electroweak Baryogenesis A Status Report Thomas Konstandin Odense, August 19, 2013 review: arxiv:1302.6713 Outline Introduction SUSY Composite Higgs Standard Cosmology time temperature Standard Cosmology
More informationWhat Shall We Learn from h^3 Measurement. Maxim Perelstein, Cornell Higgs Couplings Workshop, SLAC November 12, 2016
What Shall We Learn from h^3 Measurement Maxim Perelstein, Cornell Higgs Couplings Workshop, SLAC November 12, 2016 The Shape of Things to Come LHC: spin-0, elementary-looking Higgs field This field is
More informationMaking baryons at the electroweak phase transition. Stephan Huber, University of Sussex
Making baryons at the electroweak phase transition Stephan Huber, University of Sussex UK BSM '07 Liverpool, March 2007 Why is it interesting? There are testable consequences: New particles (scalars?!)
More informationHiggs phenomenology & new physics. Shinya KANEMURA (Univ. of Toyama)
Higgs phenomenology & new physics Shinya KANEMURA (Univ. of Toyama) KEKTH07, Dec. 13. 2007 Content of talk Introduction Electroweak Symmetry Breaking Physics of Higgs self-coupling Self-coupling measurement
More informationImplications 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 informationNon-Abelian SU(2) H and Two-Higgs Doublets
Non-Abelian SU(2) H and Two-Higgs Doublets Technische Universität Dortmund Wei- Chih Huang 25 Sept 2015 Kavli IPMU arxiv:1510.xxxx(?) with Yue-Lin Sming Tsai, Tzu-Chiang Yuan Plea Please do not take any
More informationPhase transitions in cosmology
Phase transitions in cosmology Thomas Konstandin FujiYoshida, August 31, 2017 Electroweak phase transition gravitational waves baryogenesis Outline Introduction MSSM Composite Higgs Baryogenesis [Sakharov
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 informationCan the Hbb coupling be equal in magnitude to its Standard Model value but opposite in sign? Howard E. Haber July 22, 2014
Can the Hbb coupling be equal in magnitude to its Standard Model value but opposite in sign? Howard E. Haber July 22, 2014 Outline I. Higgs physics afer discovery Ø What is the current data telling us?
More informationElectroweak baryogenesis from a dark sector
Electroweak baryogenesis from a dark sector with K. Kainulainen and D. Tucker-Smith Jim Cline, McGill U. Moriond Electroweak, 24 Mar., 2017 J. Cline, McGill U. p. 1 Outline Has electroweak baryogenesis
More informationDecoupling and Alignment in Light of the Higgs Data. Howard E. Haber Pi Day, 2014 Bay Area ParCcle Physics Seminar San Francisco State Univ.
Decoupling and Alignment in Light of the Higgs Data Howard E. Haber Pi Day, 2014 Bay Area ParCcle Physics Seminar San Francisco State Univ. Outline I. IntroducCon Ø Snapshot of the LHC Higgs data Ø SuggesCons
More informationElectroweak phase transition with two Higgs doublets near the alignment limit
Electroweak phase transition with two Higgs doublets near the alignment limit Jérémy Bernon The Hong Kong University of Science and Technology Based on 1712.08430 In collaboration with Ligong Bian (Chongqing
More informationQuantum transport and electroweak baryogenesis
Quantum transport and electroweak baryogenesis Thomas Konstandin Mainz, August 7, 2014 review: arxiv:1302.6713 Outline Introduction MSSM Composite Higgs Baryogenesis [Sakharov '69] Baryogenesis aims at
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 informationHiggs Boson Couplings as a Probe of New Physics
Higgs Boson Couplings as a Probe of New Physics Kei Yagyu Based on S. Kanemura, K. Tsumura, KY, H. Yokoya, PRD90, 075001 (2014) S. Kanemura, M. Kikuchi, and KY, PLB731, 27 (2014) S. Kanemura, M. Kikuchi,
More informationElectroweak baryogenesis in light of the Higgs discovery
Electroweak baryogenesis in light of the Higgs discovery Thomas Konstandin Grenoble, March 25, 2013 review: arxiv:1302.6713 Outline Introduction SUSY Composite Higgs Baryogenesis [Sakharov '69] Baryogenesis
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 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 informationElectroweak baryogenesis after LHC8
Electroweak baryogenesis after LHC8 Stephan Huber, University of Sussex Mainz, Germany August 2014 Moduli-induced baryogenesis [arxiv:1407.1827] WIMPy baryogenesis [arxiv:1406.6105] Baryogenesis by black
More informationKoji TSUMURA (NTU à Nagoya U.)
Koji TSUMURA (NTU à Nagoya U.) Toyama mini WS 20-21/2/2012 S. Kanemura, K. Tsumura and H. Yokoya, arxiv:1111.6089 M. Aoki, S. Kanemura, K. Tsumura and K. Yagyu, Phys. Rev. D80 015017 (2009) Outline The
More informationElectroweak Baryogenesis and Higgs Signatures
Timothy Cohen (SLAC) 1/27 Electroweak Baryogenesis and Higgs Signatures Timothy Cohen (SLAC) with Aaron Pierce arxiv:1110.0482 with David Morrissey and Aaron Pierce arxiv:1203.2924 Second MCTP Spring Symposium
More informationLeptogenesis. Neutrino 08 Christchurch, New Zealand 30/5/2008
Leptogenesis Neutrino 08 Christchurch, New Zealand 30/5/2008 Yossi Nir (Weizmann Institute of Science) Sacha Davidson, Enrico Nardi, YN Physics Reports, in press [arxiv:0802.2962] E. Roulet, G. Engelhard,
More informationEntropy, Baryon Asymmetry and Dark Matter from Heavy Neutrino Decays.
Entropy, Baryon Asymmetry and Dark Matter from Heavy Neutrino Decays. Kai Schmitz Deutsches Elektronen-Synchrotron DESY, Hamburg, Germany Based on arxiv:1008.2355 [hep-ph] and arxiv:1104.2750 [hep-ph].
More informationKoji TSUMURA (NTU Nagoya U.) KEK 16-18/2/2012
Koji TSUMURA (NTU Nagoya U.) @ KEK 16-18/2/2012 Outline: -Two-Higgs-doublet model -Leptophilic Higgs boson S. Kanemura, K. Tsumura and H. Yokoya, arxiv:1111.6089 M. Aoki, S. Kanemura, K. Tsumura and K.
More informationA New Look at the Electroweak Baryogenesis in the post-lhc Era. Jing Shu ITP-CAS
A New Look at the Electroweak Baryogenesis in the post-lhc Era. W. Huang, J. S,Y. Zhang, JHEP 1303 (2013) 164 J. S,Y. Zhang, Phys. Rev. Lett. 111 (2013) 091801 W. Huang, ZF. Kang, J. S, PW. Wu, JM. Yang,
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 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 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 informationtan(beta) Enhanced Yukawa Couplings for Supersymmetric Higgs
tan(beta) Enhanced Yukawa Couplings for Supersymmetric Higgs Singlets at One-Loop Theoretical Particle Physics University of Manchester 5th October 2006 Based on RNH, A. Pilaftsis hep-ph/0612188 Outline
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 informationPOST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY
POST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY LOUIS YANG ( 楊智軒 ) UNIVERSITY OF CALIFORNIA, LOS ANGELES (UCLA) DEC 30, 2016 4TH INTERNATIONAL WORKSHOP ON DARK MATTER,
More informationSO(10) SUSY GUTs with family symmetries: the test of FCNCs
SO(10) SUSY GUTs with family symmetries: the test of FCNCs Outline Diego Guadagnoli Technical University Munich The DR Model: an SO(10) SUSY GUT with D 3 family symmetry Top down approach to the MSSM+
More informationEW Baryogenesis and Dimensional Reduction in SM extensions
EW Baryogenesis and Dimensional Reduction in SM extensions Tuomas V.I. Tenkanen In collaboration with: T. Brauner, A. Tranberg, A. Vuorinen and D. J. Weir (SM+real singlet) J. O. Anderssen, T. Gorda, L.
More informationNatural SUSY and the LHC
Natural SUSY and the LHC Clifford Cheung University of California, Berkeley Lawrence Berkeley National Lab N = 4 SYM @ 35 yrs I will address two questions in this talk. What is the LHC telling us about
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 informationTesting the Electroweak Baryogenesis at the LHC and CEPC
Testing the Electroweak Baryogenesis at the LHC and CEPC Fa Peng Huang based on the works of arxiv : 1511.xxxxx with Xinmin Zhang, Xiaojun Bi, PeiHong Gu and PengFei Yin and Phy.Rev.D92, 075014(2015)(arXiv
More informationNatural Nightmares for the LHC
Dirac Neutrinos and a vanishing Higgs at the LHC Athanasios Dedes with T. Underwood and D. Cerdeño, JHEP 09(2006)067, hep-ph/0607157 and in progress with F. Krauss, T. Figy and T. Underwood. Clarification
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 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 informationNeutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers
Neutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers DPG Frühjahrstagung 014 in Mainz Based on Phys. Rev. Lett. 110, 31801 (013), Phys. Rev. D 88, 051701(R) (013), arxiv:1309.3970
More informationCharged Higgs Beyond the MSSM at the LHC. Katri Huitu University of Helsinki
Charged Higgs Beyond the MSSM at the LHC Katri Huitu University of Helsinki Outline: Mo;va;on Charged Higgs in MSSM Charged Higgs in singlet extensions H ± à aw ± Charged Higgs in triplet extensions H
More informationRecent progress in leptogenesis
XLIII rd Rencontres de Moriond Electroweak Interactions and Unified Theories La Thuile, Italy, March 1-8, 2008 Recent progress in leptogenesis Steve Blanchet Max-Planck-Institut for Physics, Munich March
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 informationNews on electroweak baryogenesis
News on electroweak baryogenesis Stephan Huber, University of Sussex SEWM 2012 Swansea, July 2012 Outline Electroweak phase transition Electroweak baryogenesis Models: Two Higgs doublet model SM with higher-dimensional
More informationHiggs Couplings and Electroweak Phase Transition
Higgs Couplings and Electroweak Phase Transition Maxim Perelstein, Cornell! ACFI Workshop, Amherst MA, September 17, 2015 Based on:! Andrew Noble, MP, 071018, PRD! Andrey Katz, MP, 1401.1827, JHEP ElectroWeak
More informationMaria Krawczyk U. of Warsaw
Higgs as a probe of a new physics Toyama, 11.2. 2015 Maria Krawczyk U. of Warsaw In coll. with I. Ginzburg, K. Kanishev, D.Sokolowska, B. Świeżewska, G. Gil, P.Chankowski, M. Matej, N. Darvishi, A. Ilnicka,
More informationDynamics of a two-step Electroweak Phase Transition
Dynamics of a two-step Electroweak Phase Transition May 2, 2014 ACFI Higgs Portal Workshop in Collaboration with Pavel Fileviez Pérez Michael J. Ramsey-Musolf Kai Wang hiren.patel@mpi-hd.mpg.de Electroweak
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 informationLight Stop Bound State Production at the LHC. Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim at Yonsei U.
Light Stop Bound State Production at the LHC Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim 0. 6. 8 at Yonsei U. Outline About stop Motivation for light stop Phenomenology Formalism Summary
More informationLeptogenesis with Composite Neutrinos
Leptogenesis with Composite Neutrinos Based on arxiv:0811.0871 In collaboration with Yuval Grossman Cornell University Friday Lunch Talk Yuhsin Tsai, Cornell University/CIHEP Leptogenesis with Composite
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 informationPOST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY
POST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY LOUIS YANG ( 楊智軒 ) UNIVERSITY OF CALIFORNIA, LOS ANGELES (UCLA) DEC 27, 2016 NATIONAL TSING HUA UNIVERSITY OUTLINE Big
More informationThe Inert Doublet Matter
55 Zakopane, June. 2015 The Inert Doublet Matter Maria Krawczyk University of Warsaw In coll. with I. Ginzburg, K. Kanishev, D.Sokolowska, B. Świeżewska, G. Gil, P.Chankowski, M. Matej, N. Darvishi, A.
More informationHiggs Boson: from Collider Test to SUSY GUT Inflation
Higgs Boson: from Collider Test to SUSY GUT Inflation Hong-Jian He Tsinghua University String-2016, Tsinghua, Beijing, August 5, 2016 String Theory Supergravity,GUT Effective Theory: SM, + eff operators
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 informationElectroweak baryogenesis in the MSSM and nmssm
Electroweak baryogenesis in the MSSM and nmssm Thomas Konstandin, IFAE Barcelona in collaboration with S. Huber, T. Prokopec, M.G. Schmidt and M. Seco Outline 1 Introduction The Basic Picture 2 Semiclassical
More informationBaryogenesis and Leptogenesis
Baryogenesis and Leptogenesis Mark Trodden Department of Physics, Syracuse University, Syracuse, NY 13244-1130, USA. The energy budget of the universe contains two components, dark matter and dark energy,
More informationSearch for physics beyond the Standard Model at LEP 2
Search for physics beyond the Standard Model at LEP 2 Theodora D. Papadopoulou NTU Athens DESY Seminar 28/10/03 1 Outline Introduction about LEP Alternatives to the Higgs mechanism Technicolor Contact
More informationBaryogenesis in Higher Dimension Operators. Koji Ishiwata
Baryogenesis in Higher Dimension Operators Koji Ishiwata Caltech In collaboration with Clifford Cheung (Caltech) Based on arxiv:1304.0468 BLV2013 Heidelberg, April 9, 2013 1. Introduction The origin of
More informationTeV-scale type-i+ii seesaw mechanism and its collider signatures at the LHC
TeV-scale type-i+ii seesaw mechanism and its collider signatures at the LHC Wei Chao (IHEP) Outline Brief overview of neutrino mass models. Introduction to a TeV-scale type-i+ii seesaw model. EW precision
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 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 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 informationSearches for Beyond SM Physics with ATLAS and CMS
Searches for Beyond SM Physics with ATLAS and CMS (University of Liverpool) on behalf of the ATLAS and CMS collaborations 1 Why beyond SM? In 2012 the Standard Model of Particle Physics (SM) particle content
More informationEW phase transition in a hierarchical 2HDM
EW phase transition in a hierarchical 2HDM G. Dorsch, S. Huber, K. Mimasu, J. M. No ACFI workshop, UMass Amherst Phys. Rev. Lett. 113 (2014) 211802 [arxiv:1405.5537] September 18th, 2015 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 informationCreating Matter-Antimatter Asymmetry from Dark Matter Annihilations in Scotogenic Scenarios
Creating Matter-Antimatter Asymmetry from Dark Matter Annihilations in Scotogenic Scenarios Based on arxiv:1806.04689 with A Dasgupta, S K Kang (SeoulTech) Debasish Borah Indian Institute of Technology
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 informationEW Naturalness in Light of the LHC Data. Maxim Perelstein, Cornell U. ACP Winter Conference, March
EW Naturalness in Light of the LHC Data Maxim Perelstein, Cornell U. ACP Winter Conference, March 3 SM Higgs: Lagrangian and Physical Parameters The SM Higgs potential has two terms two parameters: Higgs
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 informationHiggs Portal & Cosmology: Theory Overview
Higgs Portal & Cosmology: Theory Overview M.J. Ramsey-Musolf U Mass Amherst http://www.physics.umass.edu/acfi/ Higgs Portal WS May 2014! 1 The Origin of Matter Baryons Cosmic Energy Budget Dark Matter
More informationNeutrino Oscillation, Leptogenesis and Spontaneous CP Violation
Neutrino Oscillation, Leptogenesis and Spontaneous CP Violation Mu-Chun Chen Fermilab (Jan 1, 27: UC Irvine) M.-C. C & K.T. Mahanthappa, hep-ph/69288, to appear in Phys. Rev. D; Phys. Rev. D71, 351 (25)
More informationTwin Higgs Theories. Z. Chacko, University of Arizona. H.S Goh & R. Harnik; Y. Nomura, M. Papucci & G. Perez
Twin Higgs Theories Z. Chacko, University of Arizona H.S Goh & R. Harnik; Y. Nomura, M. Papucci & G. Perez Precision electroweak data are in excellent agreement with the Standard Model with a Higgs mass
More informationSearching for neutral Higgs bosons in non-standard channels
Searching for neutral Higgs bosons in non-standard channels Arjun Menon University of Oregon April 9, 2013 Motivation A SM-Higgs like resonance has been observed at the LHC The Higgs sector may also have
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 informationImpact of a CP-violating Higgs Boson
Impact of a CP-violating Higgs Boson Yue Zhang (Caltech) Talk at Pheno 2013, University of Pittsburgh In collaboration with, Jing Shu, arxiv:1304.0773, Higgs Couplings Higgs: always L (v + h) n Beyond
More informationProbing Supersymmetric Baryogenesis: from Electric Dipole Moments to Neutrino Telescopes
Stefano Profumo California Institute of Technology TAPIR Theoretical AstroPhysics Including Relativity Kellogg Rad Lab Probing Supersymmetric Baryogenesis: from Electric Dipole Moments to Neutrino Telescopes
More information