Light Stop Bound State Production at the LHC. Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim at Yonsei U.
|
|
- Delilah Robertson
- 6 years ago
- Views:
Transcription
1 Light Stop Bound State Production at the LHC Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim at Yonsei U.
2 Outline About stop Motivation for light stop Phenomenology Formalism Summary
3 About Stop Stop is Special SUSY e s μ c τ b b W Z W ± W 0 t t Large Yukawa coupling to Higgs 3
4 light Higgs mass in MSSM : Thanks to large Yukawa coupling, stop loop correction plays crucial role for Higgs mass to avoid LEP bound. 4
5 We are interested in light stop. m < m < m + m χ χ 0 t t 0 χ 0 LSP t NLSP t 5
6 Motivation RG evolution of stop Large Yukawa coupling 6 CMSSM m0>>m/
7 Motivation Stop mixing m ma ma LL t t * t t mrr Mixing term is large due to large Yukawa coupling ( LL RR ( LL RR ) 4 t f ) m = m + m m m + ma, t Mass difference becomes bigger than before. 7
8 Motivation 3 DM relic density Neutralino LSP is one of the favorite DM candidate DM relic density : Ω = ± nbmh DM is decoupled out of equilibrium at T < T f, the abundance remains. 8 DM relic density can be obtained by solving Boltzmann eq.: dn dt ( ) = Hn n n n 3 σ eq DM in Abell 689, Image credit:hst
9 Coannihilation processes Griest, Seckel (9 ) If LSP-NLSP mass splitting is small The NLSP density is as abundant as LSP density Thus, coannihlation with NLSP play significant role for DM relic density. The Boltzmann equation is 9
10 When light stop is NLSP with small mass difference from LSP Coannihilation processes: 0. <Ω h < DM 0. GeV < δ m < 33GeV 0 Boehm, Djouadi, Drees (00 )
11 Motivation 4 EW Baryogenesis Baryon Asymmetry of Universe : Sakharov s 3 condition (967) n b n s b = (8.9 ± 0.4) 0 Senaha s talk, at KIAS Baryon Number Violation C and CP violation Out of Equilibrium Sphaleron process CPV in SM st order EW phase transition 3 λt 4 Veff D( T T0 ) v ETv + v 4 SM EWBG fails mh 48GeV 3 3 m In MSSM Veff y Tv + yv for large y and small m 3/ Light stop
12 LEP search m < m < m + m χ t 0 0 t χ M t > 9GeV ALEPH, PLB 537 (00) 5
13 CDF search m < m < m + m χ t 0 0 t χ LHC will cover this region CDF
14 Phenomenology Stop pair production 4
15 Near threshold region N N p p t soft soft t z M = = ε sˆ ε 0 threshold region soft soft p β = = sˆˆ sˆ ( m t ) ε Large logarithm ln β Nonrelativistic regime Form stop bound state Stoponium s 5
16 Stop decays We consider following kinematics: t is NLSP 0 χ Is LSP mt 0 < mt + m χ m < m + m + m t 0 W χ Possible decays are - body 4 - body b t t b 0 χ W 0 t χ 6
17 Hikasa, Kobayashi, (87 ) Γ( t c ) = e m m ~ () ev 0 0 χ χ α c t mt loop function ~ 0^(-4) tt bound state can be described by Shroedinger eq. from pnrqcd p = ψ + m C (0) Fαs V () r = r (0) () r i 0 V () r corrections ψ() r Binding Energy : ~ () GeV B.E. = mc t Fαs( mv t ) Γ( t ) Γ m bl νχ t = (0.0 ~ 0.) 0 4 ( t c χ) m χ ml : negligible L Γ( t ) B.E. It will form stop bound state before decay. 7
18 Formalism SCET (Soft Collinear Effective Theory) Example: Consider Heavy to light decay n p set order parameter λ = m p = n p n + n pn + p µ µ µ µ for decaying quark: λ w.r.t. mb n-collinear field n p~, n p~, p ~ λ b b p µ = ( λ,, λ) p µ = (, λ, λ) p µ ( n p, n p, p ) = ( λλλ,, ) sγ p µ = ( λ, λ, λ ) n n µ = (,0,0,) n µ = (,0,0, ) n-collinear n-collinear Soft Ultra Soft n 8
19 Integrate out Hard interaction region +perm = S +perm = W n ( ) n ( x ) s x W ( x) = P exp ig ds n A ( sn) n S( x) = P exp ig ds n A ( sn) J µ = ψ µ sγ ψ b J = CP (, µξ ) WΓ S h µ µ eff n n v 9 SU(3) gauge transformation J µ eff Collinear gauge transformation Soft gauge transformation Usoft gauge transformation is Collinear, soft gauge invariant SCET operator usoft term is decoupled from the operator. It reproduces all the Infra-Red nature of full theory.
20 We do for given process Construct gauge invariant SCET operators. Typical coll. gauge invariant n collinear field: χ = W ξ, n n n σ = H J S B = nw G W µ µν n ν n n n Derive Factorization formula H : J : S : Hard scattering function process dependant Jet function universal Soft function universal Calculate each perturbative functions. Use RGE Large Log resummation can be automatically performed 0
21 Effective Operator: µ,a c ν,b d incoming color state: 8 8 = 8S 8A outgoing color state: 3 3= 8 Effective Opeartor: R f = C ( µ ) m= ( Ri, Rf ) { (,), (8 S,8), (8 A,8) } eff 3 m m mt m µ + ( ) ( µ ) ( ) ( ) ( m) a b * c * d m = Eabcd n n n n v v v v ( ρν ) ( x) = in g G ( x) : n-collinear gauge invariant gluon field a, µ ρ µν ba b n, n n, v ( x ) s ( x ) n ( x) = P exp ig ds v A ( sv) : soft Wilson lines ( v = nnv,, ) ab c cab ( x) = P exp ig ds n A ( sn) : collinear Wilson line in adjoint Rep. n R i
22 Factorization formula: N N dσ ( NN ttx ) = dπ ttx NN ttx eff s X = dπ NN O O NN s tt eff k k eff dσ ( NN ttx ) = H PDF J H S PDF Hard (H) PDF Coulomb Interaction (J) Soft (S)
23 Hard function : HM (, µ )= CM (, µ ) matching + many more We are working on NLO hard function 3
24 Soft function : Beneke, Falgari, Schwinn (00 ) s S(, ), ( z, µ ) = δ ( z) + α ( C C ) A( z, µ ) CB( z, µ ) π + + I I F I I F Idilbi, Chul Kim, Mehen (0 ) By running S( z, µ ) from µ S to we can resum the large logarithmic term ( α ln β) n NLO+NLL s µ F 4
25 Coulomb Interaction function : ψ R n ( x) is NR wave function 3 ( R, α ) R* d k R + a b On = Cα ab M ψ (k) (k) ( k) 3 n Sv Sv ( π ) Then + r s ( Rf, α) ( Rf, α) + * v * w v v k k v v 0 S S O O S S 0 = R * R R αrs Cαvw ψ k f f f MC (0) 5 k where R f k ψk = R δ( q M ) (0) Im G (0,0, E) f Mπ ψ ψ GR ( xx,, E) = x x = H E E E R k R R* k ( x) k ( x) α ( µ ) iµ G E C m f s R (0,0,, µ ) = R t + ln + ( κ) Beneke, f 4π κ mv t k
26 Summary Our GOAL is to predict resonance signal with high precision (NLO+NLL) for pp t t γγ, WW, ZZ ( ) dσ pp tt + ( γγ ) dσ pp S S 6 Kiyo, Kuhn, Moch, Steinhauser, Uwer (09 ) Idilbi, Chul Kim, Mehen (0 )
27 Summary Light stop is favored in both theory and phenomenology. Waiting for light stop search at the LHC. To be or not to be... SCET is powerful tool for describing the light stop bound state production near threshold region. NLO+NLL precision will be helpful for stop bound state search at the LHC. 7
Higgs 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 informationYu Gao Mitchell Institute for Fundamental physics and Astronomy Texas A&M University
Probing Light Nonthermal Dark Matter @ LHC Yu Gao Mitchell Institute for Fundamental physics and Astronomy Texas A&M University Outline Minimal extension to SM for baryogenesis & dark matter Current constraints
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 informationSingle Color-Octet Scalar Production at the LHC
ingle Color-Octet calar Production at the LHC : Factorization and Resummation A. Idilbi, C. Kim and T. Mehen, ArXiv:0903.3668 [hep-ph] Chul Kim Duke University Motivation calar ector in tandard Model (M)
More informationPerspectives on Future Supersymmetry at Colliders
Perspectives on Future Supersymmetry at Colliders Sunghoon Jung Korea Institute for Advanced Study (KIAS) The Future of High Energy Physics @ HKUST IAS Based on collaborations with B.Batell, E.J.Chun,
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 informationNonthermal Dark Matter & Top polarization at Collider
Nonthermal Dark Matter & Top polarization at Collider Yu Gao Texas A&M University R.Allahverdi, M. Dalchenko, B.Dutta, YG, T. Kamon, in progress B. Dutta, YG, T. Kamon, arxiv: PRD 89 (2014) 9, 096009 R.
More informationFour-fermion production near the W-pair production threshold. Giulia Zanderighi, Theory Division, CERN ILC Physics in Florence September
Four-fermion production near the W-pair production threshold Giulia Zanderighi, Theory Division, CERN ILC Physics in Florence September 12-14 2007 International Linear Collider we all believe that no matter
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 informationA pnrqcd approach to t t near threshold
LoopFest V, SLAC, 20. June 2006 A pnrqcd approach to t t near threshold Adrian Signer IPPP, Durham University BASED ON WORK DONE IN COLLABORATION WITH A. PINEDA AND M. BENEKE, V. SMIRNOV LoopFest V p.
More informationCMS Searches for SUSY in Final States with Taus. Alfredo Gurrola (Vanderbilt) on behalf of the CMS Collaboration
CMS Searches for SUSY in Final States with Taus Alfredo Gurrola (Vanderbilt) on behalf of the CMS Collaboration Why SUSY with Taus? 2 Theoretical motivation ( Naturalness ) SUSY can cancel top loop corrections
More informationSoft Collinear Effective Theory: An Overview
Soft Collinear Effective Theory: An Overview Sean Fleming, University of Arizona EFT09, February 1-6, 2009, Valencia Spain Background Before SCET there was QCD Factorization Factorization: separation of
More informationDanny van Dyk. B Workshop Neckarzimmern February 19th, Danny van Dyk (TU Dortmund) News on B K µ + µ 1 / 35
News on B K µ + µ Danny van Dyk B Workshop Neckarzimmern February 19th, 2010 Danny van Dyk (TU Dortmund) News on B K µ + µ 1 / 35 The Goal 15 1 10 0.8 5 0.6 C10 0-5 0.4-10 0.2-15 -15-10 -5 0 5 10 15 C
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 informationEffective-theory methods for top-quark and squark pair production at LHC and Tevatron
Effective-theory methods for top-quark and squark pair production at LHC and Tevatron Christian Schwinn Univ. Freiburg 21.10.2010 (Based on M.Beneke, P.Falgari, CS, arxiv:0907.1443 [hep-ph], arxiv:1007.5414
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 informationPrecision Jet Physics At the LHC
Precision Jet Physics At the LHC Matthew Schwartz Harvard University JETS AT THE LHC An (almost) universal feature of SUSY is and Source: Atlas TDR SIGNAL VS. BACKGROUND Source: Atlas TDR Can we trust
More informationSearches at LEP. Ivo van Vulpen CERN. On behalf of the LEP collaborations. Moriond Electroweak 2004
Searches at LEP Moriond Electroweak 2004 Ivo van Vulpen CERN On behalf of the LEP collaborations LEP and the LEP data LEP: e + e - collider at s m Z (LEP1) and s = 130-209 GeV (LEP2) Most results (95%
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 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 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 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 informationQCD threshold corrections for gluino pair production at NNLL
Introduction: Gluino pair production at fixed order QCD threshold corrections for gluino pair production at NNLL in collaboration with Ulrich Langenfeld and Sven-Olaf Moch, based on arxiv:1208.4281 Munich,
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 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 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 informationAndrey Katz C. Brust, AK, S. Lawrence, and R. Sundrum; arxiv:
SUSY, the Third Generation and the LHC Andrey Katz C. Brust, AK, S. Lawrence, and R. Sundrum; arxiv:1011.6670 Harvard University January 9, 2012 Andrey Katz (Harvard) SUSY petite January 9, 2012 1 / 27
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 informationTop Quarks, Unstable Particles... and NRQCD
Top Quarks, Unstable Particles... and NRQCD André H. Hoang Max-Planck-Institute for Physics Munich (Thanks to A. Manohar, I. Stewart, T. Teubner, C. Farrell, C. Reisser, M. Stahlhofen ) INT Workshop, May
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 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 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 informationEffects of Reheating on Leptogenesis
Effects of Reheating on Leptogenesis Florian Hahn-Woernle Max-Planck-Institut für Physik München 2. Kosmologietag Florian Hahn-Woernle (MPI-München) Effects of Reheating on Leptogenesis Kosmologietag 2007
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 informationAsymmetric WIMP DM. Luca Vecchi. Aspen (CO) 2/2011. in collaboration with Michael Graesser and Ian Shoemaker (LANL)
Asymmetric WIMP DM Luca Vecchi in collaboration with Michael Graesser and Ian Shoemaker (LANL) Aspen (CO) 2/2011 Outline 1 Motivations 2 The relic abundance of asymmetric species 3 Asymmetric WIMP Dark
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 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 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 informationBSM physics and Dark Matter
BSM physics and Dark Matter Andrea Mammarella University of Debrecen 26-11-2013 1 Introduction and motivation 2 Dark Matter 3 MiAUMSSM 4 Dark Matter in the MiAUMSSM 5 Conclusion Introduction and motivation
More information12 Best Reasons to Like CP Violation
12 Best Reasons to Like CP Violation SSI 2012 The Electroweak Scale: Unraveling the Mysteries at the LHC SLAC, California 27 July 2012 Yossi Nir (Weizmann Institute of Science) SSI40 1/35 CP Violation
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 informationHadronic B decays from SCET. Christian Bauer LBNL FPCP 2006, Vancouver
Hadronic B decays from SCET Christian Bauer LBNL FPCP 2006, Vancouver Outline of the Talk Introduction Hadronic B deays in SCET Phenomenology of Hadronic B decays Conclusions Introduction Flavor Physics
More informationRight-handed SneutrinoCosmology and Hadron Collider Signature
Right-handed Sneutrino and Hadron Northwestern University with Andre de Gouvea ( Northwestern) & Werner Porod ( Valencia)... June 15, 2006 Susy 06, UC Irvine Right-handed Sneutrino and Hadron Collider
More information*** LIGHT GLUINOS? Cracow-Warsaw Workshop on LHC Institut of Theoretical Physics, University of Warsaw
LIGHT GLUINOS? Cracow-Warsaw Workshop on LHC 15.01.2010 Marek Olechowski Institut of Theoretical Physics, University of Warsaw LIGHT GLUINOS? Early supersymmetry discovery potential of the LHC Phenomenology
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 informationSearches for SUSY in Final States with Photons
SUSY4: The nd International Conference on Supersymmetry and Unification of Fundamental Interactions" -6 July 4, Manchester, England" Searches for SUSY in Final States with Photons On Behalf of the CMS
More informationTop pair production near threshold at LHC (NLO/NLL analysis in NRQCD)
Top@LHC LHC TTbar-Threshold Threshold@ILC/LHC Green Functions Top pair production near threshold at LHC (NLO/NLL analysis in NRQCD) Yuichiro Kiyo TTP, Universität Karlsruhe Collaboration with: J. H. Kühn(KA),
More informationThe role of ElectroWeak corrections in indirect Dark Matter searches Firenze, 18/12/ / 26
The role of ElectroWeak corrections in indirect Dark Matter searches Paolo Ciafaloni INFN, sezione di Lecce Firenze, 18/12/2013 The role of ElectroWeak corrections in indirect Dark Matter searches Firenze,
More informationStatus of Supersymmetric Models
Status of Supersymmetric Models Sudhir K Vempati CHEP, IISc Bangalore Institute of Physics, Bhubhaneswar Feb, 203 Outline Why Supersymmetry? Structure of MSSM Experimental Status New models of SUSY S/(S+B)
More informationLectures on Standard Model Effective Field Theory
Lectures on Standard Model Effective Field Theory Yi Liao Nankai Univ SYS Univ, July 24-28, 2017 Page 1 Outline 1 Lecture 4: Standard Model EFT: Dimension-six Operators SYS Univ, July 24-28, 2017 Page
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 informationFull Mass Determination from M T 2 with Combinatorial Background
Full Mass Determination from M T 2 with Combinatorial Background David Curtin bla arxiv:1004.5350, arxiv:xxxx.xxxx In Collaboration with Maxim Perelstein, Monika Blanke bla Cornell Institute for High Energy
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 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 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 informationAsymmetric Sneutrino Dark Matter
Asymmetric Sneutrino Dark Matter Stephen West Oxford University Asymmetric Sneutrino Dark Matter and the Ω b /Ω dm Puzzle; hep-ph/0410114, PLB, Dan Hooper, John March- Russell, and SW from earlier work,
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 informationExperimental Summary 40 th Rencontres de Moriond QCD and High Energy Hadronic Interactions. Heidi Schellman Northwestern University
Experimental Summary 40 th Rencontres de Moriond QCD and High Energy Hadronic Interactions Heidi Schellman Northwestern University Thank you To the conference organizers The secretariat The Hotel Planibel
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 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 informationEarly SUSY Searches in Events with Leptons with the ATLAS-Detector
Early SUSY Searches in Events with Leptons with the ATLAS-Detector Timo Müller Johannes Gutenberg-Universität Mainz 2010-29-09 EMG Annual Retreat 2010 Timo Müller (Universität Mainz) Early SUSY Searches
More informationNon-local 1/m b corrections to B X s γ
Non-local 1/m b corrections to B X s γ Michael Benzke TU München September 16, 2010 In collaboration with S. J. Lee, M. Neubert, G. Paz Michael Benzke (JGU) Non-local 1/m b corrections to B X s γ TU München
More information2 2 ω 0 = m B m D. B D + ρ B D 0 π, B D 0 π,
.3 Massive Gauge Boson Form Factor & Rapidity Divergences MORE SCET I APPLICATIONS then we may move all usoft wilson lines into the usoft part of the operator yielding,5 (c),5 (d) Q [h Γ Y T a Y h (b)
More informationWZ di-boson production at CMS
WZ di-boson production at CMS 1 Outline Physics motivations Existing results (Tevatron s = 1.96TeV) Existing prospects for CMS at s = 14TeV Preliminary prospects for CMS at s = 7TeV 2 WZ Physics motivation
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 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 informationSUSY at Accelerators (other than the LHC)
SUSY at Accelerators (other than the LHC) Beate Heinemann, University of Liverpool Introduction Final LEP Results First Tevatron Run 2 Results Summary and Outlook IDM 2004, Edinburgh, September 2004 Why
More informationHiggs-charm Couplings
Higgs-charm Couplings Wai Kin Lai TUM December 21, 2017 MLL Colloquium, TUM OUTLINE Higgs physics at the LHC OUTLINE Higgs physics at the LHC H J/ψ + γ as a key channel to measure Hc c coupling CHRISTMAS
More informationHIGGS + 2 JET PRODUCTION AT THE LHC
IGGS + 2 JET PRODUCTION AT TE LC Dieter Zeppenfeld Universität Karlsruhe, Germany Seminar at KITP, Santa Barbara, March 13, 2008 LC goals Vector boson fusion Measurement of iggs couplings jj production
More informationQCD and High Energy Hadronic Interactions. Northwestern University. Heidi Schellman. Experimental Summary. 40 th Rencontres de Moriond
Experimental Summary 40 th Rencontres de Moriond QCD and High Energy Hadronic Interactions Heidi Schellman Northwestern University Thank you To the conference organizers The secretariat The Hotel Planibel
More informationThe Story of Wino Dark matter
The Story of Wino Dark matter Varun Vaidya Dept. of Physics, CMU DIS 2015 Based on the work with M. Baumgart and I. Rothstein, 1409.4415 (PRL) & 1412.8698 (JHEP) Evidence for dark matter Rotation curves
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 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 informationBound-state effects in ttbar production at the LHC
1 Bound-state effects in ttbar production at the LHC Hiroshi YOKOYA (National Taiwan University) based on works in collaboration with K.Hagiwara(KEK) and Y.Sumino(Tohoku U) GGI workshop, Firenze, 2011.09.28
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 informationSUSY Phenomenology & Experimental searches
SUSY Phenomenology & Experimental searches Alex Tapper Slides available at: http://www.hep.ph.ic.ac.uk/tapper/lecture.html Reminder Supersymmetry is a theory which postulates a new symmetry between fermions
More informationInterconnection between Particle Physics and Cosmology at the LHC
Interconnection between Particle Physics and Cosmology at the LHC Selections from the Cosmo Secret Cube Catalogue Transformer Cube Standard Model Cube PPC Cube Premiere Props Teruki Kamon Mitchell Institute
More informationEffective Theory for Electroweak Doublet Dark Matter
Effective Theory for Electroweak Doublet Dark Matter University of Ioannina, Greece 3/9/2016 In collaboration with Athanasios Dedes and Vassilis Spanos ArXiv:1607.05040 [submitted to PhysRevD] Why dark
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 information(Non-minimal) SUSY Phenomenology of the minimal R-symmetric SUSY model
(Non-minimal) SUSY Phenomenology of the minimal R-symmetric SUSY model Dominik Stöckinger TU Dresden KIAS Workshop, October 2016 based on work with: [Philip Diessner, Jan Kalinowski, Wojciech Kotlarski,
More informationRevisiting gravitino dark matter in thermal leptogenesis
Revisiting gravitino dark matter in thermal leptogenesis Motoo Suzuki Institute for Cosmic Ray Research (ICRR) The University of Tokyo arxiv:1609.06834 JHEP1702(2017)063 In collaboration with Masahiro
More informationGravitino LSP as Dark Matter in the Constrained MSSM
Gravitino LSP as Dark Matter in the Constrained MSSM Ki Young Choi The Dark Side of the Universe, Madrid, 20-24 June 2006 Astro-Particle Theory and Cosmology Group The University of Sheffield, UK In collaboration
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 informationCalculation of Momentum Distribution Function of a Non-Thermal Fermionic Dark Matter
Calculation of Momentum Distribution Function of a Non-Thermal Fermionic Dark Matter, March 8, 2017. arxiv:1612.02793, with Anirban Biswas. Aritra Gupta Why Non-Thermal? 1 / 31 The most widely studied
More informationNon-Standard Higgs Decays
Non-Standard Higgs Decays David Kaplan Johns Hopkins University in collaboration with M McEvoy, K Rehermann, and M Schwartz Standard Higgs Decays Standard Higgs Decays 1 _ bb 140 GeV WW BR for SM Higgs
More informationSquark and top quark pair production at the LHC and Tevatron
Squark and top quark pair production at the LHC and Tevatron M. Beneke (RWTH Aachen) 10th Hellenic School and Workshop on Elementary Particle Physics and Gravity Corfu, Greece, August 31, 2010 Outline
More informationSho IWAMOTO. 7 Nov HEP phenomenology joint Cavendish DAMTP U. Cambridge
MSSM scenario Sho IWAMOTO 7 Nov. 2016 HEP phenomenology joint Cavendish DAMTP seminar @ U. Cambridge Based on [1608.00283] in collaboration with M. Abdullah, J. L. Feng, and B. Lillard (UC Irvine) The
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 and Gauged Baryon Number
Dark Matter and Gauged Baryon Number Sebastian Ohmer Collaborators: Pavel Fileviez Pérez and Hiren H. Patel P. Fileviez Pérez, SO, H. H. Patel, Phys.Lett.B735(2014)[arXiv:1403.8029] P.Fileviez Pérez, SO,
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 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 informationsin(2θ ) t 1 χ o o o
Production of Supersymmetric Particles at High-Energy Colliders Tilman Plehn { Search for the MSSM { Production of Neutralinos/Charginos { Stop Mixing { Production of Stops { R Parity violating Squarks
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 informationThe Shadow of a Scale-Invariant Hidden U(1)
The Shadow of a Scale-Invariant Hidden U1) We-Fu Chang Feb. 26, 2008 at APCTP 2008 with John Ng and Jackson Wu) PRD74:095005,75:115016 Motivation Model Coleman-Weinberg Phenomenology and U1) We-Fu Chang,
More informationSupersymmetry at the ILC
Supersymmetry at the ILC Abdelhak DJOUADI (LPT Paris Sud). Introduction 2. High precision measurements 3. Determination of the SUSY lagrangian 4. Connection to cosmology 5. Conclusion For more details,
More information8.882 LHC Physics. Higgs Physics and Other Essentials. [Lecture 22, April 29, 2009] Experimental Methods and Measurements
8.882 LHC Physics Experimental Methods and Measurements Higgs Physics and Other Essentials [Lecture 22, April 29, 2009] Organization Next week lectures: Monday 2pm and Tuesday 9:30am (which room?) Project
More informationNeutralino Dark Matter and SUSY Spectroscopy. M. E. Peskin June 2004 YITP
Neutralino Dark Matter and SUSY Spectroscopy M. E. Peskin June 2004 YITP - 2004 The prediction of cosmic dark matter is an important argument for the presence of SUSY in Nature. This is a robust prediction
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 informationLeptogenesis in Higgs triplet model
Leptogenesis in Higgs triplet model S. Scopel Korea Institute of Advanced Study (KIAS) Seoul (Korea) Dark Side of the Universe, Madrid,, 20-24 24 June 2006 Introduction Non-zero neutrino masses and mixing
More informationThe Higgs boson and the scale of new physics
The Higgs boson and the scale of new physics Giuseppe Degrassi Dipartimento di Matematica e Fisica, Università di Roma Tre, I.N.F.N. Sezione di Roma Tre Corfu Summer School and Workshop on The Standard
More information