Electroweak Baryogenesis after LHC8
|
|
- Barry Beasley
- 6 years ago
- Views:
Transcription
1 Electroweak Baryogenesis after LHC8 Gláuber Carvalho Dorsch with S. Huber and J. M. No University of Sussex arxiv: JHEP 131, 29(213) What NExT? Southampton November 27, 213 G. C. Dorsch EWBG after LHC8 What NExT? 1 / 19
2 The problem of baryogenesis I Observed BAU: n B s 1 1. G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
3 The problem of baryogenesis I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
4 The problem of baryogenesis I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
5 The problem of baryogenesis I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
6 The problem of baryogenesis I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; C/CP violation; X CKM matrix; G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
7 The problem of baryogenesis I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; C/CP violation; X CKM matrix; thermodynamical non-equilibrium. Xexpansion of Universe; XEW phase transition; G. C. Dorsch EWBG after LHC8 What NExT? 2 / 19
8 Baryogenesis in SM I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; C/CP violation; thermodynamical non-equilibrium; G. C. Dorsch EWBG after LHC8 What NExT? 3 / 19
9 Baryogenesis in SM I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; C/CP violation; thermodynamical non-equilibrium; G. C. Dorsch EWBG after LHC8 What NExT? 3 / 19
10 Baryogenesis in SM I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; C/CP violation; X CKM matrix; thermodynamical non-equilibrium; G. C. Dorsch EWBG after LHC8 What NExT? 3 / 19
11 Baryogenesis in SM I Observed BAU: n B s 1 1. I Assume BAU as initial condition of Universe? Inflation & sphaleron processes would wash out the initial asymmetry. I Baryogenesis ) Sakharov conditions: B number violation; X chiral anomaly and non-trivial SU(2) topology; C/CP violation; X CKM matrix; thermodynamical non-equilibrium; Xexpansion of Universe; XEW phase transition. G. C. Dorsch EWBG after LHC8 What NExT? 3 / 19
12 Electroweak baryogenesis in SM I B-number violating processes suppressed at T =... Probability e 16 2 /g G. C. Dorsch EWBG after LHC8 What NExT? 4 / 19
13 Electroweak baryogenesis in SM I B-number violating processes suppressed at T =... Probability e 16 2 /g I...but there is a threshold T. T c (EW scale) above which the rate of B violation Universe s expansion. G. C. Dorsch EWBG after LHC8 What NExT? 4 / 19
14 Electroweak baryogenesis in SM I B-number violating processes suppressed at T =... Probability e 16 2 /g I...but there is a threshold T. T c (EW scale) above which the rate of B violation Universe s expansion. I If T>T after EW phase transition, the generated asymmetry is washed out. G. C. Dorsch EWBG after LHC8 What NExT? 4 / 19
15 Electroweak baryogenesis in SM I B-number violating processes suppressed at T =... Probability e 16 2 /g I...but there is a threshold T. T c (EW scale) above which the rate of B violation Universe s expansion. I If T>T after EW phase transition, the generated asymmetry is washed out. I Successful baryogenesis requires a strong first order phase transition: v c T c & 1. Sphaleron CP χ L + χ L B χ R Sphaleron <φ> = <φ> = Bubble Wall Morrissey, Ramsey-Musolf [arxiv: ] G. C. Dorsch EWBG after LHC8 What NExT? 4 / 19
16 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
17 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
18 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
19 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
20 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. I Possibilities include... G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
21 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. I Possibilities include... I Extra scalar singlet G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
22 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. I Possibilities include... I Extra scalar singlet +extracpviolation; G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
23 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. I Possibilities include... I Extra scalar singlet +extracpviolation; I MSSM, NMSSM; G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
24 Electroweak baryogenesis in SM I EWPT in SM is strongly first order only if m h. m W. I CKM matrix alone does not supply sufficient CP violation. Even with a first order phase transition, BAU prediction would be 1 orders of magnitude below observed value. I EWBG requires BSM physics at EW scale with moderately large couplings to SM sector and new sources of CP! I Testable scenario in present and near-future colliders. I Possibilities include... I Extra scalar singlet +extracpviolation; I MSSM, NMSSM; I 2HDM. G. C. Dorsch EWBG after LHC8 What NExT? 5 / 19
25 EWBG in the MSSM MSSM Higgs sector ) two SU(2) L scalar doublets 1, 2: ' + i = i. h i + i i V MSSM tree = µ µ g2 + g 2 8 EW minimum: h 1 i = v cos 2 2 µ H.c g , h 2 i = 2 v sin Mass eigenstates: G,G ± {z } + h,h,a,h ±. {z } Goldstone bosons physical Higgs states. G. C. Dorsch EWBG after LHC8 What NExT? 6 / 19
26 EWBG in MSSM (?) I New scalars increase strength of phase transition ) light stop scenario (LSS): 8 GeV. m t R. 12 GeV. Many new sources of CP violation. However... G. C. Dorsch EWBG after LHC8 What NExT? 7 / 19
27 EWBG in MSSM (?) I New scalars increase strength of phase transition ) light stop scenario (LSS): 8 GeV. m t R. 12 GeV. Many new sources of CP violation. However... I m h = m Z cos(2 ) + R.C.. 13 GeV. m h 125 GeV + LSS ) heavy stop (naturalness?) 1 TeV G. C. Dorsch EWBG after LHC8 What NExT? 7 / 19
28 EWBG in MSSM (?) I New scalars increase strength of phase transition ) light stop scenario (LSS): 8 GeV. m t R. 12 GeV. Many new sources of CP violation. However... I m h = m Z cos(2 ) + R.C.. 13 GeV. m h 125 GeV + LSS ) heavy stop 1 TeV (naturalness?) I This scenario allows for rather definite predictions on SM Higgs production and branching ratios, with severe tension with experimental data! [Curtin, Jaiswal, Meade, arxiv: ] G. C. Dorsch EWBG after LHC8 What NExT? 7 / 19
29 EWBG in MSSM (?) I New scalars increase strength of phase transition ) light stop scenario (LSS): 8 GeV. m t R. 12 GeV. Many new sources of CP violation. However... I m h = m Z cos(2 ) + R.C.. 13 GeV. m h 125 GeV + LSS ) heavy stop 1 TeV (naturalness?) I This scenario allows for rather definite predictions on SM Higgs production and branching ratios, with severe tension with experimental data! [Curtin, Jaiswal, Meade, arxiv: ] I Could be alleviated if light neutralino has mass. 6 GeV. [Carena, Nardini, Quiros, Wagner, arxiv: ] G. C. Dorsch EWBG after LHC8 What NExT? 7 / 19
30 2HDM I Two-Higgs-doublet models are the minimal SM extension able to account for BAU. I Generalization of the MSSM Higgs sector. I Extra heavy bosons (h,h,a,h ± ) may strengthen the EW phase transition. I Additional sources of CP (explicit and/or spontaneous). G. C. Dorsch EWBG after LHC8 What NExT? 8 / 19
31 2HDM I Two-Higgs-doublet models are the minimal SM extension able to account for BAU. I Generalization of the MSSM Higgs sector. I Extra heavy bosons (h,h,a,h ± ) may strengthen the EW phase transition. I Additional sources of CP (explicit and/or spontaneous). I Correct BAU can be obtained for simplified cases and for particular combinations of parameters. [Fromme, Huber, Seniuch, hep-ph/65242] G. C. Dorsch EWBG after LHC8 What NExT? 8 / 19
32 2HDM I Two-Higgs-doublet models are the minimal SM extension able to account for BAU. I Generalization of the MSSM Higgs sector. I Extra heavy bosons (h,h,a,h ± ) may strengthen the EW phase transition. I Additional sources of CP (explicit and/or spontaneous). I Correct BAU can be obtained for simplified cases and for particular combinations of parameters. [Fromme, Huber, Seniuch, hep-ph/65242] I But what happens in the general case? G. C. Dorsch EWBG after LHC8 What NExT? 8 / 19
33 2HDM I General fermionic couplings: L Yukawa = Q L ( ) n R +... G. C. Dorsch EWBG after LHC8 What NExT? 9 / 19
34 2HDM I General fermionic couplings: L Yukawa = Q L ( ) n R +... I Diagonalizing mass matrix M n = 1 h' 1i + 2 h' 2i does not diagonalize 1,2 simultaneously, so induces tree-level FCNC. L FCNC = d L e 1 ' 1d R +... G. C. Dorsch EWBG after LHC8 What NExT? 9 / 19
35 2HDM I General fermionic couplings: L Yukawa = Q L ( ) n R +... I Diagonalizing mass matrix M n = 1 h' 1i + 2 h' 2i does not diagonalize 1,2 simultaneously, so induces tree-level FCNC. L FCNC = d L e 1 ' 1d R +... I Avoid this with Z 2 symmetry: 1! 1, 2! 2. u R d R e R Type I Type II + Type X + + Type Y + + Only top-quark is significant for phase transition. Then models differ only in phenomenological constraints on their parameter space. These come mainly from B-physics, so Type I Type X, Type II Type Y. G. C. Dorsch EWBG after LHC8 What NExT? 9 / 19
36 2HDM I For simplicity, consider CP conserving case only. V tree( 1, 2) = µ µ 2 2 µ H.c apple H.c.. 2 I EW minimum: h 1 i = I parameters: I v cos v 174 GeV and M, h 2 i = p µ. sin(2 ) I Masses: mh,m H,m A,m H ±. v sin I is the mixing angle between (G +,H + ) and (G,A ).. I Likewise, is the mixing angle between (h,h ). It is here defined such that = () h = h SM. G. C. Dorsch EWBG after LHC8 What NExT? 1 / 19
37 V = Vtree + VCW + VCT + VT. Fix mh = 125 GeV.4 tan 2 I Constraints: < 2 EW precision: 1 ; i < 4 ; metastability; B B (red/dashed) and B! Xs (black/full). I 1, I, I GeV µ 1 TeV, I 1 GeV ma, mh ± 1 TeV, 15 GeV mh 1 TeV. Type I/X Type II/Y tan tan I mh ± [GeV ] Type II/Y: mh ± G. C. Dorsch mh ± [GeV ] 36 GeV [Hermann et al., arxiv: ]. EWBG after LHC8 What NExT? 11 / 19
38 Results: tan Type I/X Type II/Y tan Preference for tan tan. 3 is excellent for baryogenesis, since n B (tan ) 2. G. C. Dorsch EWBG after LHC8 What NExT? 12 / 19
39 Results: Masses (a) (f) (b) mh ± [GeV] ma [GeV] mh [GeV] (e) (d) (c) ma mh± [GeV] m H ± ma mh [GeV] mh mh± [GeV] hardly influences the phase transition. G. C. Dorsch EWBG after LHC8 What NExT? 13 / 19
40 Results: Masses (a) (f) (b) mh ± [GeV] ma [GeV] mh [GeV] (e) (d) (c) ma mh± [GeV] ma mh [GeV] mh mh± [GeV] m H ± hardly influences the phase transition. Large pseudo-scalar masses, m A & 4 GeV, are favoured. G. C. Dorsch EWBG after LHC8 What NExT? 13 / 19
41 Results: Masses (a) (f) (b) mh ± [GeV] ma [GeV] mh [GeV] (e) (d) (c) ma mh± [GeV] ma mh [GeV] mh mh± [GeV] m H ± hardly influences the phase transition. Large pseudo-scalar masses, m A & 4 GeV, are favoured. s also prefer hierarchy m A >m H ' m H ±. G. C. Dorsch EWBG after LHC8 What NExT? 13 / 19
42 Results: Couplings 4 = 1 2v 2 M 2 + m 2 A 2m2 H ±, 5 = 1 2v 2 M 2 m 2 A Type I/X Type II/Y Type I/X Type II/Y G. C. Dorsch EWBG after LHC8 What NExT? 14 / 19
43 Results: 1 8 Type I/X Type II/Y /4 /4 /2 3 /4 - /4 /4 /2 3 /4 A strong PT favours a SM-like h. G. C. Dorsch EWBG after LHC8 What NExT? 15 / 19
44 Results: 1 8 Type I/X Type II/Y /4 /4 /2 3 /4 - /4 /4 /2 3 /4 A strong PT favours a SM-like h. Put another way, the observation of a SM-like h constrains the parameter space of 2HDMs in favour of strong PTs. G. C. Dorsch EWBG after LHC8 What NExT? 15 / 19
45 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
46 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
47 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
48 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: I tan 1; G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
49 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: I tan 1; I ma & 4 GeV; G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
50 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: I tan 1; I ma & 4 GeV; I mass hierarchy ma >m H ' m H ±. G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
51 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: I tan 1; I ma & 4 GeV; I mass hierarchy ma >m H ' m H ±. I What does this tell us about probing the 2HDM in LHC? Are there hidden scalars in current LHC data? [Arhrib, Ferreira, Santos, arxiv: ] How would a discovery impact the phase transition? G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
52 Conclusions I 2HDMs are robust candidates to explain BAU in light of LHC8 results. I h h SM favours a strong PT scenario. I also prefers: I tan 1; I ma & 4 GeV; I mass hierarchy ma >m H ' m H ±. I What does this tell us about probing the 2HDM in LHC? Are there hidden scalars in current LHC data? [Arhrib, Ferreira, Santos, arxiv: ] How would a discovery impact the phase transition? Thank you! G. C. Dorsch EWBG after LHC8 What NExT? 16 / 19
53 Appendix h! Type I Type II BR(h! ) BR(h! ) Coupling of h to b and : Type I: sin sin, Type II: cos cos. G. C. Dorsch EWBG after LHC8 What NExT? 17 / 19
54 Appendix µ parameter V tree µ H.c Type I/X Type II/Y µ [GeV] µ [GeV] Type II/Y: m H ± 36 GeV. G. C. Dorsch EWBG after LHC8 What NExT? 18 / 19
55 Appendix Surviving points after each step of tests: Total EW precision i < 4 Metastability Absolute Relative 1% 19.1% 2.3%.41%.69% fields: G + = cos ' + 1 +sin '+ 2 (charged Goldstone), H + = sin ' cos '+ 2 (charged scalar), G = cos 1 +sin 2 (neutral Goldstone), A = sin 1 + cos 2 (pseudo-scalar), h = cos h 1 +sin h 2 (lightest scalar), H = sin h 1 + cos h 2 (heaviest scalar). where i = ' + i h i + i i. G. C. Dorsch EWBG after LHC8 What NExT? 19 / 19
Electroweak 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 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 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 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 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
Electroweak Baryogenesis Eibun Senaha (KIAS) Feb. 13, 2013 HPNP2013 @U. of Toyama Outline Motivation Electroweak baryogenesis (EWBG) sphaleron decoupling condition strong 1 st order EW phase transition
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 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 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 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 informationTwo-Higgs-doublet models with Higgs symmetry
Two-Higgs-doublet models with Higgs symmetry Chaehyun Yu a a School of Physics, KIAS, Seoul 130-722, Korea Abstract We investigate two-higgs-doublet models (2HDMs) with local U(1) H Higgs flavor symmetry
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 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 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 informationElectroweak baryogenesis in the two Higgs doublet model
Michael Seniuch Bielefeld University 1 Electroweak baryogenesis in the two Higgs doublet model M. Seniuch, Bielefeld University COSMO 05 Bonn August 2005 Work is done in collaboration with Lars Fromme
More informationCP violation in charged Higgs production and decays in the Complex 2HDM
CP violation in charged Higgs production and decays in the Complex 2HDM Abdesslam Arhrib National Cheung Keung University (NCKU), Faculté des Sciences et Techniques Tangier, Morocco Based on: A.A, H. Eberl,
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 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 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 informationDouble Higgs production via gluon fusion (gg hh) in composite models
Double Higgs production via gluon fusion (gg hh) in composite models Ennio Salvioni CERN and University of Padova based on work in collaboration with C.Grojean (CERN), M.Gillioz (Zürich), R.Gröber and
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 informationSinglet Assisted Electroweak Phase Transitions and Precision Higgs Studies
Singlet Assisted Electroweak Phase Transitions and Precision Higgs Studies Peter Winslow Based on: PRD 91, 035018 (2015) (arxiv:1407.5342) S. Profumo, M. Ramsey-Musolf, C. Wainwright, P. Winslow arxiv:1510.xxxx
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 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 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 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 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 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 informationProbing the charged Higgs boson at the LHC in the CP-violating type-ii 2HDM
Probing the charged Higgs boson at the LHC in the CP-violating type-ii 2HDM Giovanni Marco Pruna IKTP TU Dresden charged 2012, Uppsala University, 10th of October Outline Motivation Standard Model: a solid
More informationBSM Higgs Searches at ATLAS
BSM Higgs Searches at ATLAS Martin zur Nedden Humboldt-Universität zu Berlin for the ATLAS Collaboration SUSY Conference 2014 Manchester July 20 th July 25 th, 2014 Introduction Discovery of a scalar Boson
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 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 informationTop Seesaw, Custodial Symmetry and the 126 GeV (Composite) Higgs
Top Seesaw, Custodial Symmetry and the 126 GeV (Composite) Higgs IAS Program on the Future of High Energy Physics Jan 21, 2015 based on arxiv:1311.5928, Hsin-Chia Cheng, Bogdan A. Dobrescu, JG JHEP 1408
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 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 informationAn Introduction to Cosmology Lecture 2. (University of Wisconsin Madison)
An Introduction to Cosmology Lecture 2 Daniel Chung (University of Wisconsin Madison) Outline of lecture 2 Quantitative elements of EW bgenesis number Explain transport eqs. for electroweak baryogenesis
More informationElectroweak Phase Transition at CEPC: A cosmologist s perspective
Electroweak Phase Transition at CEPC: A cosmologist s perspective (DR.) ANDREW LONG UNIVERSITY OF CHICAGO, KICP @ IHEP BEIJING WORKSHOP ON CEPC PHYSICS NOV 6, 2017 Based on 1608.06619 (PRD) with Peisi
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 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 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 informationElectroweak-scale Right-handed Neutrino Model And 126 GeV Higgs-like Particle
Electroweak-scale Right-handed Neutrino Model And 126 GeV Higgs-like Particle Ajinkya S. Kamat ask4db@virginia.edu http://people.virginia.edu/ ask4db With Prof. P. Q. Hung and Vinh Van Hoang (paper in
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 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 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 informationSearching for Beyond Standard Model Physics with Top Quarks at the ATLAS Detector
Searching for Beyond Standard Model Physics with Top Quarks at the ATLAS Detector (University of Hong Kong) Topical Mini-Workshop of the New Physics at the TeraScale @ Tsung-Dao Lee Institute, SJTU Introduction
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 informationHiggs Sector in New Physics and its Collider Phenomenology
Higgs Sector in New Physics and its Collider Phenomenology Shinya KANEMURA University of TOYAMA 7-8. Dec. 2008, ICRR Theory Meeting Plan of This Talk Electroweak Symmetry Breaking SM Higgs property Search
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 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 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 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 informationProbing Two Higgs Doublet Models with LHC and EDMs
Probing Two Higgs Doublet Models with LHC and EDMs Satoru Inoue, w/ M. Ramsey-Musolf and Y. Zhang (Caltech) ACFI LHC Lunch, March 13, 2014 Outline 1 Motivation for 2HDM w/ CPV 2 Introduction to 2HDM 3
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 informationLight Higgs Production in Two Higgs Doublets Models type III
Light Higgs Production in Two Higgs Doublets Models type III Camilo Andrés Jiménez-Cruz (M.Sc. Student), J.-Alexis Rodríguez López, Roberto Martinez Universidad Nacional de Colombia December 5, 2007 Abstract
More informationPhenomenology of a light singlet-like scalar in NMSSM
Phenomenology of a light singlet-like scalar in NMSSM Institute of Theoretical Physics, University of Warsaw Corfu Summer Institute, 12 September 2014 based on: MB, M. Olechowski and S. Pokorski, JHEP
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 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 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 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 informationA Cosmologist s Perspective on Higgs Factories
A Cosmologist s Perspective on Higgs Factories ANDREW LONG UNIVERSITY OF CHICAGO, KICP @ BLV 2017 CLEVELAND, OH MAY 16, 2017 based on [1608.06619, PRD] with Peisi Huang & Lian-Tao Wang Why are cosmologists
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 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 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 informationGolden SUSY, Boiling Plasma, and Big Colliders. M. Perelstein, Cornell University IPMU LHC Workshop talk, 12/18/07
Golden SUSY, Boiling Plasma, and Big Colliders M. Perelstein, Cornell University IPMU LHC Workshop talk, 12/18/07 Outline Part I: Supersymmetric Golden Region and its Collider Signature (with Christian
More informationComposite Higgs/ Extra Dimensions
Composite Higgs/ Extra Dimensions Eduardo Pontón Instituto de Física Teórica -UNESP & ICTP-SAIFR Snowmass on the Pacific, KITP May 30, 2013 Fundamental Question raised by the SM How and why is the Electroweak
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 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 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 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 informationLooking through the Higgs portal with exotic Higgs decays
Looking through the Higgs portal with exotic Higgs decays Jessie Shelton University of Illinois, Urbana-Champaign Unlocking the Higgs Portal (U. Mass. Amherst) May 1, 2014 A light SM-like Higgs is narrow
More informationHiggs Searches beyond SM
Higgs Searches beyond SM and MSSM at the LHC Daniela Rebuzzi Pavia University and INFN on behalf of the ATLAS and CMS Collaborations MCTP Spring Symposium on Higgs Boson Physics Ann Arbor, Michigan - May
More informationTwo-Higgs-Doublet Model
Two-Higgs-Doublet Model Logan A. Morrison University of California, Santa Cruz loanmorr@ucsc.edu March 18, 016 Logan A. Morrison (UCSC) HDM March 18, 016 1 / 7 Overview 1 Review of SM HDM Formalism HDM
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 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 informationStudies of Higgs Potential (Higgs Boson Self Coupling Measurements)
Studies of Higgs Potential (Higgs Boson Self Coupling Measurements) Theory of Higgs boson pair production Searches for Higgs boson pair production Constraint on the Higgs boson self coupling Jianming Qian
More informationCORFU2012 Corfu Maria Krawczyk (University of Warsaw)
CORFU2012 Corfu 16.09.2012 Maria Krawczyk (University of Warsaw) in collaboration with I. Ginzburg, K. Kanishev (Novosibirsk U.), D.Sokołowska, G. Gil, B. Gorczyca (Świeżewska) J. Bogdanowicz (U. of Warsaw)
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 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 informationElectroweak and Higgs Physics
Electroweak and Higgs Physics Lecture 2 : Higgs Mechanism in the Standard and Supersymmetric Models Alexei Raspereza DESY Summer Student Program Hamburg August 2017 Standard Model (Summary) Building blocks
More informationA SUPERSYMMETRIC VIEW OF THE HIGGS HUNTING
UC @ Santa Barbara Feb. 2nd, 2011 A SUPERSYMMETRIC VIEW OF THE HIGGS HUNTING Tao Liu UC @ Santa Barbara Higgs Boson And Particle Physics The Standard Model (SM) is a successful theory of describing the
More informationHidden Higgs boson in extended supersymmetric scenarios at the LHC
Hidden Higgs boson in extended supersymmetric scenarios at the LHC Priyotosh Bandyopadhyay INFN Lecce & University of Salento, Lecce arxiv:1512.09241, arxiv:1512.08651, JHEP 1512 (2015) 127, JHEP 1509
More informationarxiv: v1 [hep-ph] 16 Mar 2017
Flavon-induced lepton flavour violation arxiv:1703.05579v1 hep-ph] 16 Mar 017 Venus Keus Department of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu, FIN-00014 University of Helsinki,
More informationThe theory ends here. We need help. Experiments must clear up this mess. M. Veltman 2003
The theory ends here. We need help. Experiments must clear up this mess. M. Veltman 2003 Nobel 1999 "for elucidating the quantum structure of EW interactions Maria Krawczyk IFT, Wydział Fizyki UW I. Ginzburg,
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 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 informationChaehyun Yu. in collaboration with P. Ko (KIAS) and Yuji Omura (Nagoya University) The 16 th LHC Physics Monthly Meeting, KIAS, Korea, Jun 01,
Top FCNC Chaehyun Yu (Academia Sinica) in collaboration with P. Ko (KIAS) and Yuji Omura (Nagoya University) The 16 th LHC Physics Monthly Meeting, KIAS, Korea, Jun 01, 2015 1 Flavor changing neutral currents
More informationElectroweak baryogenesis and flavor
Electroweak baryogenesis and flavor Thomas Konstandin Utrecht, May 18, 2017 in collaboration with G. Servant, I. Baldes, S. Bruggisser The serendipity of electroweak baryogenesis Thomas Konstandin Geraldine
More informationHow high could SUSY go?
How high could SUSY go? Luc Darmé LPTHE (Paris), UPMC November 24, 2015 Based on works realised in collaboration with K. Benakli, M. Goodsell and P. Slavich (1312.5220, 1508.02534 and 1511.02044) Introduction
More informationarxiv: v1 [hep-ex] 5 Sep 2014
Proceedings of the Second Annual LHCP CMS CR-2014/199 September 8, 2014 Future prospects of Higgs Physics at CMS arxiv:1409.1711v1 [hep-ex] 5 Sep 2014 Miguel Vidal On behalf of the CMS Experiment, Centre
More informatione + e (ha) bbbb in Abelian Extended Supersymmetric Standard Model
arxiv:hep-ph/9809355v1 13 Sep 1998 e + e (ha) bbbb in Abelian Extended Supersymmetric Standard Model D. A. Demir, N. K. Pak Middle East Technical University, Department of Physics, 06531 Ankara, Turkey
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 informationThe Super-little Higgs
The Super-little Higgs Csaba Csaki (Cornell) with Guido Marandella (UC Davis) Yuri Shirman (Los Alamos) Alessandro Strumia (Pisa) hep-ph/0510294, Phys.Rev.D73:035006,2006 Padua University, July 4, 2006
More informationDmitri Sidorov Oklahoma State University On behalf of the ATLAS Collaboration DIS2014, 04/28/2014
Dmitri Sidorov Oklahoma State University On behalf of the ATLAS Collaboration DIS4, 4/8/4 Introduc)on We discovered a Standard Model (SM) like Higgs boson at mh=5 GeV. This is not the end of the story.
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 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 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 informationMass degenerate Higgs Hunters explore the 2HDM. Howard E. Haber West Coast LHC Theory UC Riverside December 7, 2012
Mass degenerate Higgs Hunters explore the 2HDM Howard E. Haber West Coast LHC Theory Meeting @ UC Riverside December 7, 2012 Outline A boson born on the 4 th of July 2012 Properties of the Higgs boson
More informationComplementarity of the CERN LEP collider, the Fermilab Tevatron, and the CERN LHC in the search for a light MSSM Higgs boson
Complementarity of the CERN LEP collider, the Fermilab Tevatron, and the CERN LHC in the search for a light MSSM Higgs boson M. Carena* Theory Division, CERN, 1211 Geneva 23, Switzerland S. Mrenna Physics
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 information