Models as existence proofs, speculations or... peaces of physical reality
|
|
- Isabella Sara Scott
- 6 years ago
- Views:
Transcription
1 Models as existence proofs, speculations or... peaces of physical reality Riccardo Barbieri Zuoz II, July 16/21, 2006 An example of what could happen, based on: An ultra-bottom-up hypothesis 2 concrete realizations (why not a single one?)
2 The idea RB, Hall Seek simple Higgs sector that: 1. Agrees with all data (EWPT) 2. Is fully natural up to 1.5 TeV ( + maybe something else) A modest ultra-bottom-up approach, with crucial consequences for LHC
3 A Heavy SM Higgs and the EWPT T IDM = T SM +!T S IDM = S SM +!S A heavy Higgs m h = GeV + a positive ΔT Origin of ΔT?? (Peskin, Wells and many others) prefer models that populate the 1-2σ ellipse in most of parameter space. Are there any?
4 2 HDM in an alternative phase RB, Hall, Rychkov IDM controlled by approximate SU(2) V
5 The IDM is natural and perturbative up to ~1.5 TeV (instead of the SM only up to ~ 400 GeV) H NL L with and m h = GeV ] m H m NL ]!m mh mnl and an average mass m av (m L,m NL,m H ) 100 GeV 1 TeV m
6 A Dark Matter candidate Unbroken H 2 H 2 Inert scalars always in pair (for natural flavour conservation) Stable lightest inert scalar To get the observed! m need co-annihilation of S, A into light fermions as dominant process m GeV m L GeV Shouldn t one have seen S and A at LEP2 via e + e A + S (Z + S) + S What about direct DM detection! h (Lp Lp) pb ( "L 0.5? ) 2 ( ) 2 ( 70GeV 500GeV m L? m h ) 4
7 Can one do better than! nat 1.5 TeV? 2H doublets Supersymmetry ( UV completion )... but without a light Higgs boson! How?? In the most straightforward way: Add a coupling λ through! f = "SH 1 H 2 with λ only constrained by perturbativity up to TeV λsusy NMSSM with! low energy 2 dominating over all other couplings RB, Hall, Nomura, Rychkov Not consistent with gauge unification? An open question, depending on the physics above TeV See, e.g., Harnik et al, Gripaios and West
8 ElectroWeak Precision Tests in λsusy S and T from Higgs s M( S)! = 2 S and T from Higgsinos tan! 2.5 m( H ± ) For and s-particles in their natural range, most of parameter space inside the 1-2σ ellipse tan! = 1 an exact custodial symmetry point
9 Particle spectrum (naturalness bounds) in λsusy! = 2 with up to 20% tuning (m max! "/5) and no significant bound on other s-fermions and SU(2)xU(1) gauginos! mess = 100 TeV
10 Dark Matter in λsusy blue:!h 2 = white:!h 2 < 0.09 red:!h 2 > 0.13 grey: m LSP < 45 GeV black lines: m LSP = m W,m Z LSP =! S + " H 1 + # H 2 with no special relation among parameters (MSSM)
11 Provisional conclusions Doubling the Higgs multiplet the simplest solution (?) of the l.h.p., realized in several possible ways 1 TeV H ±,A,H 500 GeV h + possibly something else Relevant to supersymmetry itself? LHC will explore for the first time the relevant energy range, well above the Fermi scale
12 An example: The Inert Doublet Model Consider the most general 2H doublet model invariant under H 2 H 2 to get natural flavour conservation (i.e., only couples to matter) +! 4 H 1 H 2 2 +! 5 2 [(H 1 H 2) 2 + h.c.] H 1 RB, Hall, Rychkov V = µ 2 1 H µ 2 2 H 2 2 +! 1 H 1 4 +! 2 H 2 4 +! 3 H 1 2 H 2 2! 4,! 5 custodial symmetry! 5 PQ symmetry Take µ 2 1 < 0, µ 2 2 > 0 so that H 1 = ( φ + v + (h + iχ)/ 2 ), H 2 = ( H + (S + ia)/ 2 )
13 The Inert Doublet Model (continued) Parameter space: µ 2 1,! 1 v(m Z ), m h! 2 (in the usual way) (not relevant to the spectrum) µ 2 2,! 3,4,5 m L,m NL,m H ;! L m 2 H = µ 2 2 +! 3 v 2 m 2 S = µ (! 3 +! 4 +! 5 )v 2 m 2 A = µ (! 3 +! 4! 5 )v 2! L! 3 +! 4! 5 custodial symm. limit: PQ symmetry limit: m H = m S = m A m S = m A absolute minimum:! 1,2 > 0! 3,! L! 3 +! 4! 5 > 2(! 1! 2 ) 1/2
14 Naturalness, perturbativity, EWPT in the IDM!m 2 h = " t # t 2 + " g # 2 g + " 11 # 2 H 1 + " 12 # 2 H 2!µ 2 2 = 1 ( "g # 2 g + " 22 # 2 H " 21 # 2 ) H 1 16! 2 d" i d log# = $ i(")! nat = min(! i ) 1.5 TeV
15 T IDM = T SM +!T SIDM = S SM +!S!S!T negligible 1 24" 2 #v 2(m H m A )(m H m S ) In the Standard Model: m h = GeV In the IDM: m h = GeV (m H m S )(m H m A ) = M 2, M = GeV
16 Collider Signals 1. m h = GeV A standard Higgs boson? h SS,AA,H + H at! h = 68 GeV m h = 500 GeV 2. pp W HA or HS H AW or SW A SZ ( ) for the DM parameters, looking for 3 charged leptons! signal 3.5 fb! bg 20 fb
Hidden 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 informationThe inert doublet model in light of LHC and XENON
The inert doublet model in light of LHC and XENON Sara Rydbeck 24 July 212 Identification of Dark Matter, IDM 212, Chicago 1 The CERN Large Hadron Collider Only discovery so far. If no new strongly interacting
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 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 informationBeyond the SM: SUSY. Marina Cobal University of Udine
Beyond the SM: SUSY Marina Cobal University of Udine Why the SM is not enough The gauge hierarchy problem Characteristic energy of the SM: M W ~100 GeV Characteristic energy scale of gravity: M P ~ 10
More 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 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 informationInert Doublet Model:
Inert Doublet Model: Dark Matter Implication and Collider Phenomenology Shufang Su U. of Arizona S. Su In collaboration with E. Dolle, X. Miao and B. Thomas Inert Doublet Model Introduce another Higgs
More informationarxiv: v1 [hep-ph] 16 Jun 2011
IL NUOVO CIMENTO Vol.?, N.?? On the MSSM with hierarchical squark masses and a heavier Higgs boson arxiv:16.3253v1 [hep-ph] 16 Jun 2011 E. Bertuzzo( ) Scuola Normale Superiore and INFN, Piazza dei Cavalieri
More informationLecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model
Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,
More 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 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 informationLecture 4 - Beyond the Standard Model (SUSY)
Lecture 4 - Beyond the Standard Model (SUSY) Christopher S. Hill University of Bristol Warwick Flavour ++ Week April 11-15, 2008 Recall the Hierarchy Problem In order to avoid the significant finetuning
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 informationImplications of the 125 GeV Higgs for the inert dark matter
Implications of the 125 GeV Higgs for the inert dark matter Bogumiła Świeżewska Faculty of Physics, University of Warsaw 26.03.2014 Recontres de Moriond QCD and High Energy Interactions, La Thuile, Italy
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 informationPhysics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002
Physics at e + e - Linear Colliders 4. Supersymmetric particles M. E. Peskin March, 2002 In this final lecture, I would like to discuss supersymmetry at the LC. Supersymmetry is not a part of the Standard
More 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 informationPhysics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1
Physics 662 Particle Physics Phenomenology February 21, 2002 Physics 662, lecture 13 1 Physics Beyond the Standard Model Supersymmetry Grand Unified Theories: the SU(5) GUT Unification energy and weak
More informationThe first year of the LHC and Theory. G.G.Ross, Krakow, December 09
The first year of the LHC and Theory G.G.Ross, Krakow, December 09 The LHC a discovery machine The gauge sector : new gauge bosons? The maber sector : new quarks and leptons? The scalar sector : the hierarchy
More informationProspettive future della fenomenologia delle particelle. Riccardo Barbieri IFAE Pavia 19/21 Aprile
Prospettive future della fenomenologia delle particelle Riccardo Barbieri IFAE 2006 - Pavia 19/21 Aprile Particle Physics in one page L SM = 1 4 Fa µ!f aµ! + i "D" +! i " i j! j h + h.c. + D µ h 2 V (h)
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 informationDark Matter Implications for SUSY
Dark Matter Implications for SUSY Sven Heinemeyer, IFCA (CSIC, Santander) Madrid, /. Introduction and motivation. The main idea 3. Some results 4. Future plans Sven Heinemeyer, First MultiDark workshop,
More informationComposite Higgs Overview
Composite Higgs Overview Tony Gherghetta Fundamental Composite Dynamics, IBS CTPU, Daejeon, Korea, December 6, 2017 1 IBS Daejeon - 6 December 2017 Composite Higgs New strong force with coupling, g s g
More informationLittle Higgs Models Theory & Phenomenology
Little Higgs Models Theory Phenomenology Wolfgang Kilian (Karlsruhe) Karlsruhe January 2003 How to make a light Higgs (without SUSY) Minimal models The Littlest Higgs and the Minimal Moose Phenomenology
More informationTheory of the ElectroWeak Interactions
Theory of the ElectroWeak Interactions Riccardo Barbieri 1st Summer School of ITN Corfu, September 4-15, 2011 1. The Standard Model: the indirect informations 2. Higgsless Grojean 3. The Higgs boson as
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 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 informationWhither SUSY? G. Ross, Birmingham, January 2013
Whither SUSY? G. Ross, Birmingham, January 2013 whither Archaic or poetic adv 1. to what place? 2. to what end or purpose? conj to whatever place, purpose, etc. [Old English hwider, hwæder; related to
More informationA Motivated Non-Standard Supersymmetric Spectrum
A Motivated Non-Standard Supersymmetric Spectrum Paolo Lodone, EPFL, CH PhD Thesis discussed on December 09, 2011 Scuola Normale Superiore and INFN, Pisa Supervisor: Riccardo Barbieri Outline 1) Introduction:
More informationDiscovery potential of toppartners in a realistic composite Higgs model with early LHC data
Discovery potential of toppartners in a realistic composite Higgs model with early LHC data Günther Dissertori, Elisabetta Furlan, Filip Moortgat, JHEP09(20)019 Kick-off Meeting Of The LHCPhenoNet Initial
More informationOblique corrections from Light Composite Higgs
Oblique corrections from Light Composite Higgs Slava Rychkov (ENS Paris & CERN) with Axel Orgogozo 1111.3534 & work in progress EWPT in Standard Model M H 0.0 M W -1.2 % W 0.2 M Z 0.2 % Z 0.1 0! had 0
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 informationImplications et perspectives theoriques
Implications et perspectives theoriques Riccardo Barbieri SNS and INFN, Pisa 1/26 Particle Physics in one page L ST L SM = 1 4 Fa µnf aµn + iȳ 6Dy + D µ h 2 V (h) +y i l ij y j h + h.c. The gauge sector
More informationKaluza-Klein Theories - basic idea. Fig. from B. Greene, 00
Kaluza-Klein Theories - basic idea Fig. from B. Greene, 00 Kaluza-Klein Theories - basic idea mued mass spectrum Figure 3.2: (Taken from [46]). The full spectrum of the UED model at the first KK level,
More informationThe Hierarchy Problem on Neutral
The Hierarchy Problem on Neutral Natural Theories with Colorless Top Partners Gustavo Burdman University of São Paulo - IAS Princeton Is the discovery of the Higgs the End of Naturalness? Naturalness and
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 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 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 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 informationSUPERSYMETRY FOR ASTROPHYSICISTS
Dark Matter: From the Cosmos to the Laboratory SUPERSYMETRY FOR ASTROPHYSICISTS Jonathan Feng University of California, Irvine 29 Jul 1 Aug 2007 SLAC Summer Institute 30 Jul 1 Aug 07 Feng 1 Graphic: N.
More informationNovember 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model
Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one
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 informationKaluza-Klein Dark Matter
Kaluza-Klein Dark Matter Hsin-Chia Cheng UC Davis Pre-SUSY06 Workshop Complementary between Dark Matter Searches and Collider Experiments Introduction Dark matter is the best evidence for physics beyond
More informationWhither SUSY? G. Ross, RAL, January 2013
Whither SUSY? G. Ross, RAL, January 2013 whither Archaic or poetic adv 1. to what place? 2. to what end or purpose? conj to whatever place, purpose, etc. [Old English hwider, hwæder; related to Gothic
More informationComposite gluino at the LHC
Composite gluino at the LHC Thomas Grégoire University of Edinburgh work in progress with Ami Katz What will we see at the LHC? Natural theory of EWSB? Supersymmetry? Higgs as PGSB (LH, RS-like)? Extra-
More informationCORFU HDMs. symmetry The Inert Model Various vacua Today= Inert phase Thermal evolutions Z 2
CORFU2010 5.09. 2010 2HDMs Z 2 symmetry The Inert Model Various vacua Today= Inert phase Thermal evolutions Maria Krawczyk University of Warsaw I. Ginzburg, K. Kanishev (Novosibirsk University), D.Sokołowska,
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: Interpretation and Implications. Marco Farina April 19, 2013
Higgs: Interpretation and Implications Marco Farina April 19, 2013 Discovery! ATLAS coll. ATLAS-CONF-2013-034. CMS coll. CMS-PAS-HIG-13-002 Data Giardino et al. 1303.3570 Giardino et al. 1303.3570 Higgs
More informationSearch for SUperSYmmetry SUSY
PART 3 Search for SUperSYmmetry SUSY SUPERSYMMETRY Symmetry between fermions (matter) and bosons (forces) for each particle p with spin s, there exists a SUSY partner p~ with spin s-1/2. q ~ g (s=1)
More informationGauge-Higgs Unification on Flat Space Revised
Outline Gauge-Higgs Unification on Flat Space Revised Giuliano Panico ISAS-SISSA Trieste, Italy The 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions Irvine,
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 informationExotic W + W Z Signals at the LHC
Exotic W + W Z Signals at the LHC Jared Evans jaevans@ucdavis.edu w/ M.Luty and S.Chang Department of Physics University of California - Davis WCLHC Evans (UCD) WWZ at LHC April 14, 011 1 / 11 Premise
More informationInvisible Sterile Neutrinos
Invisible Sterile Neutrinos March 25, 2010 Outline Overview of Sterile Neutrino Dark Matter The Inert Doublet Model with 3 Singlet Fermions Non-thermal Dark Matter Conclusion Work done in collaboration
More information+ µ 2 ) H (m 2 H 2
I. THE HIGGS POTENTIAL AND THE LIGHT HIGGS BOSON In the previous chapter, it was demonstrated that a negative mass squared in the Higgs potential is generated radiatively for a large range of boundary
More 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 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 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 informationCold Dark Matter beyond the MSSM
Cold Dark Matter beyond the MM Beyond the MM inglet Extended MM inglet Extended tandard Model References V. Barger, P. Langacker, M. McCaskey, M. J. Ramsey-Musolf and G. haughnessy, LHC Phenomenology of
More 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 informationPseudo-Dirac Bino as Dark Matter and Signatures of D-Type G
and Signatures of D-Type Gauge Mediation Ken Hsieh Michigan State Univeristy KH, Ph. D. Thesis (2007) ArXiv:0708.3970 [hep-ph] Other works with M. Luty and Y. Cai (to appear) MSU HEP Seminar November 6,
More information*** 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 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 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 informationPAMELA from Dark Matter Annihilations to Vector Leptons
PAMELA from Dark Matter Annihilations to Vector Leptons phalendj@umich.edu With Aaron Pierce and Neal Weiner University of Michigan LHC and Dark Matter Workshop 2009 University of Michigan Outline PAMELA
More informationDark Matter Searches and Fine-Tuning in Supersymmetry. Maxim Perelstein, Cornell University PACIFIC 2011 Symposium September 9, 2011
Dark Matter Searches and Fine-Tuning in Supersymmetry Maxim Perelstein, Cornell University PACIFIC 2011 Symposium September 9, 2011 Bibliography Primary reference: MP, Shakya, arxiv:1107.5048 [hep-ph]
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 informationSUSY with light electroweakino
SUSY with light electroweakino Sho IWAMOTO A self introduction 17 Dec. 2014 Joint HEP Seminar @ Tel Aviv University References: * M. Endo, K. Hamaguchi, S. I., and T. Yoshinaga [1303.4256] * S. I., T.
More informationMSSM4G: MOTIVATIONS AND ALLOWED REGIONS
MSSM4G: MOTIVATIONS AND ALLOWED REGIONS ATLAS SUSY WG Meeting CERN Jonathan Feng, University of California, Irvine 31 January 2018 Based on 1510.06089, 1608.00283 with Mohammad Abdullah (Texas A&M), Sho
More informationLecture 39, 40 Supplement: Particle physics in the LHC era
Lecture 39, 40 Supplement: Particle physics in the LHC era The Matter Particles (Fermions) plus their antiparticles... What is measured? quarks confined into hadrons A zoo of strongly interacting particles...
More informationString Theory in the LHC Era
String Theory in the LHC Era J Marsano (marsano@uchicago.edu) 1 String Theory in the LHC Era 1. Electromagnetism and Special Relativity 2. The Quantum World 3. Why do we need the Higgs? 4. The Standard
More informationThe Yang and Yin of Neutrinos
The Yang and Yin of Neutrinos Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA The Yang and Yin of Neutrinos (2018) back to start 1 Contents Introduction The
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 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 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 informationSupersymmetry Basics. J. Hewett SSI J. Hewett
Supersymmetry Basics J. Hewett SSI 2012 J. Hewett Basic SUSY References A Supersymmetry Primer, Steve Martin hep-ph/9709356 Theory and Phenomenology of Sparticles, Manual Drees, Rohini Godbole, Probir
More 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 informationarxiv: v2 [hep-ph] 2 Apr 2016
Blind spots for neutralino dark matter in the NMSSM Marcin Badziak 1, Marek Olechowski 2, Pawe l Szczerbiak 3 arxiv:1512.02472v2 [hep-ph] 2 Apr 2016 Institute of Theoretical Physics, Faculty of Physics,
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 informationBeyond the SM Higgs a crucial aspect of the cross roads
Beyond the SM Higgs a crucial aspect of the cross roads Dark Matter String Landscape Naturalness Anthropics Elementary BSM Higgs SM Higgs Composite Higgs SUSY T-parity Extra Dim. Dark Energy Jack Gunion
More informationarxiv: v1 [hep-ph] 26 May 2011
Higgs boson signals in λsusy with a Scale Invariant Superpotential Enrico Bertuzzo, Marco Farina Scuola Normale Superiore and INFN, Piazza dei Cavalieri 7, 5616 Pisa, Italy May 30, 011 arxiv:1105.5389v1
More informationYasunori Nomura. UC Berkeley; LBNL. hep-ph/ [PLB] hep-ph/ [PLB] hep-ph/ [PRD] Based on work with Ryuichiro Kitano (SLAC)
Yasunori Nomura UC Berkeley; LBNL Based on work with Ryuichiro Kitano (SLAC) hep-ph/0509039 [PLB] hep-ph/0509221 [PLB] hep-ph/0602096 [PRD] We will be living in the Era of Hadron Collider Exploring highest
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 informationarxiv: v1 [hep-ph] 31 Jan 2014
The price of being SM-like in SUSY Tony Gherghetta a,b,1, Benedict von Harling c,, Anibal D. Medina b,3, Michael A. Schmidt b,4 a School of Physics & Astronomy, University of Minnesota, Minneapolis, MN
More informationSplit SUSY at LHC and a 100 TeV collider
Split SUSY at LHC and a 100 TeV collider Thomas Grégoire With Hugues Beauchesne and Kevin Earl 1503.03099 GGI - 2015 Status of Supersymmetry stop searches gluino searches m t & 700GeV m g & 1.4TeV What
More informationKiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.)
Exploring New Physics beyond the Standard Model of Particle Physics Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb. 2011 (Tohoku Univ.) We are confronting a critical moment of particle physics with the CERN
More informationNaturalizing Supersymmetry with the Relaxion
Naturalizing Supersymmetry with the Relaxion Tony Gherghetta University of Minnesota Beyond the Standard Model OIST Workshop, Okinawa, Japan, March 4, 2016 Jason Evans, TG, Natsumi Nagata, Zach Thomas
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 informationIntroducing SModelS - with an application to light neutralino DM
Hi! Introducing SModelS - with an application to light neutralino DM Suchita Kulkarni (LPSC, Grenoble) based on: 1) work in progress with W. Waltenberger, U. Laa, A. Lessa, D. Proschofsky, S. Kraml 2)
More informationmh = 125 GeV and SUSY naturalness
mh = 125 GeV and SUSY naturalness Josh Ruderman (UC Berkeley) March 13, 212 Lawrence Hall, David Pinner, JTR 1112.273 h! ATLAS CMS p Observed p 1-2 1 2 SM H expected p Data 211, s = 7 TeV Ldt = 4.9 fb
More informationThe Standard Model of particle physics and beyond
The Standard Model of particle physics and beyond - Lecture 3: Beyond the Standard Model Avelino Vicente IFIC CSIC / U. Valencia Physics and astrophysics of cosmic rays in space Milano September 2016 1
More informationLECTURE 2: Super theories
LECTURE 2: Super theories Carlos Muñoz Universidad Autónoma de Madrid & Instituto de Física Teórica UAM/CSIC ISAPP09-Como, July 8-16 Carlos Muñoz Super theories 2 ~0.00000001 Carlos Muñoz Super theories
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 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 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 informationPerspectives for Particle Physics beyond the Standard Model
Perspectives for Particle Physics beyond the Standard Model What is the Higgs boson trying to tell us? Is supersymmetry waiting? Can LHC Run 2 find it? What if X(750) exists? John Ellis Higgs Champagne
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 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 information