110. Supersymmetry, Part II (Experiment) 1 110
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The Pev-Scale Split Supersymmetry from Higgs Mass and Electroweak Vacuum Stability
The PeV-Scale Split Supersymmetry from Higgs Mass and Electroweak Vacuum Stability Waqas Ahmed ? 1, Adeel Mansha ? 2, Tianjun Li ? ~ 3, Shabbar Raza ∗ 4, Joydeep Roy ? 5, Fang-Zhou Xu ? 6, ? CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, P. R. China ~School of Physical Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, P. R. China ∗ Department of Physics, Federal Urdu University of Arts, Science and Technology, Karachi 75300, Pakistan Institute of Modern Physics, Tsinghua University, Beijing 100084, China Abstract The null results of the LHC searches have put strong bounds on new physics scenario such as supersymmetry (SUSY). With the latest values of top quark mass and strong coupling, we study the upper bounds on the sfermion masses in Split-SUSY from the observed Higgs boson mass and electroweak (EW) vacuum stability. To be consistent with the observed Higgs mass, we find that the largest value of supersymmetry breaking 3 1:5 scales MS for tan β = 2 and tan β = 4 are O(10 TeV) and O(10 TeV) respectively, thus putting an upper bound on the sfermion masses around 103 TeV. In addition, the Higgs quartic coupling becomes negative at much lower scale than the Standard Model (SM), and we extract the upper bound of O(104 TeV) on the sfermion masses from EW vacuum stability. Therefore, we obtain the PeV-Scale Split-SUSY. The key point is the extra contributions to the Renormalization Group Equation (RGE) running from arXiv:1901.05278v1 [hep-ph] 16 Jan 2019 the couplings among Higgs boson, Higgsinos, and gauginos. -
Color Breaking in the Quantum Leaped Stop Decay
Color breaking in the quantum leaped stop decay Imre Czövek [email protected] Abstract. The superfield propagator contains a measurable quantum leap, which comes from the definition of SUSY. In the sfermion -> Goldstino + fermion vertex change: 1. the spin of sparticle with discrete 1/2, 2. the Grassman superspace with the Goldstino shift operator. 3. the spacetime as the result of extra dimensional leap. The leap nature of SUSY transformations appears in the squark decay, it is the analog definition of SUSY. The quantum leaped outgoing propagators are determined and break locally the energy and the charge. Like to the teleportation the entangled pairs are here the b quark and the Goldstino. The dominant stop production is from gluons. The stop-antistop pair decay to quantum leaped b (c or t) quark, and the decay break the color. I get for the (color breaking) quantum leap: 10^-18 m. 10^-11 m color breaking would be needed for a color breaking chain reaction. The open question is: Are the colliders producing supersymmetry charge? Because some charges in QGP can make long color breaking and a chain reaction. A long color broken QGP state in the re-Big Bang theory could explain the near infinite energy and the near infinite mass of the universe: - at first was random color QGP in the flat space-time, - at twice the color restoration in the curved space-time, which eats the Goldstinos, - and finally the baryon genesis. The re Big Bang make a supernova like collapse and a flat explosion of Universe. This explanation of SUSY hides the Goldstone fermion in the extra dimensions, the Goldstino propagate only in superspace and it is a not observable dark matter. -
Measuring the Spin of SUSY Particles SUSY: • Every SM Fermion (Spin 1/2
Measuring the spin of SUSY particles SUSY: • every SM fermion (spin 1/2) ↔ SUSY scalar (spin 0) • every SM boson (spin 1 or 0) ↔ SUSY fermion (spin 1/2) Want to check experimentally that (e.g.) eL,R are really spin 0 and Ce1,2 are really spin 1/2. 2 preserve the 5th dimensional momentum (KK number). The corresponding coupling constants among KK modes Model with a 500 GeV-size extra are simply equal to the SM couplings (up to normaliza- tion factors such as √2). The Feynman rules for the KK dimension could give a rather SUSY- modes can easily be derived (e.g., see Ref. [8, 9]). like spectrum! In contrast, the coefficients of the boundary terms are not fixed by Standard Model couplings and correspond to new free parameters. In fact, they are renormalized by the bulk interactions and hence are scale dependent [10, 11]. One might worry that this implies that all pre- dictive power is lost. However, since the wave functions of Standard Model fields and KK modes are spread out over the extra dimension and the new couplings only exist on the boundaries, their effects are volume sup- pressed. We can get an estimate for the size of these volume suppressed corrections with naive dimensional analysis by assuming strong coupling at the cut-off. The FIG. 1: One-loop corrected mass spectrum of the first KK −1 result is that the mass shifts to KK modes from bound- level in MUEDs for R = 500 GeV, ΛR = 20 and mh = 120 ary terms are numerically equal to corrections from loops GeV. -
Electroweak Radiative B-Decays As a Test of the Standard Model and Beyond Andrey Tayduganov
Electroweak radiative B-decays as a test of the Standard Model and beyond Andrey Tayduganov To cite this version: Andrey Tayduganov. Electroweak radiative B-decays as a test of the Standard Model and beyond. Other [cond-mat.other]. Université Paris Sud - Paris XI, 2011. English. NNT : 2011PA112195. tel-00648217 HAL Id: tel-00648217 https://tel.archives-ouvertes.fr/tel-00648217 Submitted on 5 Dec 2011 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. LAL 11-181 LPT 11-69 THESE` DE DOCTORAT Pr´esent´eepour obtenir le grade de Docteur `esSciences de l’Universit´eParis-Sud 11 Sp´ecialit´e:PHYSIQUE THEORIQUE´ par Andrey Tayduganov D´esint´egrationsradiatives faibles de m´esons B comme un test du Mod`eleStandard et au-del`a Electroweak radiative B-decays as a test of the Standard Model and beyond Soutenue le 5 octobre 2011 devant le jury compos´ede: Dr. J. Charles Examinateur Prof. A. Deandrea Rapporteur Prof. U. Ellwanger Pr´esident du jury Prof. S. Fajfer Examinateur Prof. T. Gershon Rapporteur Dr. E. Kou Directeur de th`ese Dr. A. Le Yaouanc Directeur de th`ese Dr. -
The Minimal Supersymmetric Standard Model: Group Summary Report
PM/98–45 December 1998 The Minimal Supersymmetric Standard Model: Group Summary Report Conveners: A. Djouadi1, S. Rosier-Lees2 Working Group: M. Bezouh1, M.-A. Bizouard3,C.Boehm1, F. Borzumati1;4,C.Briot2, J. Carr5,M.B.Causse6, F. Charles7,X.Chereau2,P.Colas8, L. Duflot3, A. Dupperin9, A. Ealet5, H. El-Mamouni9, N. Ghodbane9, F. Gieres9, B. Gonzalez-Pineiro10, S. Gourmelen9, G. Grenier9, Ph. Gris8, J.-F. Grivaz3,C.Hebrard6,B.Ille9, J.-L. Kneur1, N. Kostantinidis5, J. Layssac1,P.Lebrun9,R.Ledu11, M.-C. Lemaire8, Ch. LeMouel1, L. Lugnier9 Y. Mambrini1, J.P. Martin9,G.Montarou6,G.Moultaka1, S. Muanza9,E.Nuss1, E. Perez8,F.M.Renard1, D. Reynaud1,L.Serin3, C. Thevenet9, A. Trabelsi8,F.Zach9,and D. Zerwas3. 1 LPMT, Universit´e Montpellier II, F{34095 Montpellier Cedex 5. 2 LAPP, BP 110, F{74941 Annecy le Vieux Cedex. 3 LAL, Universit´e de Paris{Sud, Bat{200, F{91405 Orsay Cedex 4 CERN, Theory Division, CH{1211, Geneva, Switzerland. 5 CPPM, Universit´e de Marseille-Luminy, Case 907, F-13288 Marseille Cedex 9. 6 LPC Clermont, Universit´e Blaise Pascal, F{63177 Aubiere Cedex. 7 GRPHE, Universit´e de Haute Alsace, Mulhouse 8 SPP, CEA{Saclay, F{91191 Cedex 9 IPNL, Universit´e Claude Bernard de Lyon, F{69622 Villeurbanne Cedex. 10 LPNHE, Universit´es Paris VI et VII, Paris Cedex. 11 CPT, Universit´e de Marseille-Luminy, Case 907, F-13288 Marseille Cedex 9. Report of the MSSM working group for the Workshop \GDR{Supersym´etrie". 1 CONTENTS 1. Synopsis 4 2. The MSSM Spectrum 9 2.1 The MSSM: Definitions and Properties 2.1.1 The uMSSM: unconstrained MSSM 2.1.2 The pMSSM: “phenomenological” MSSM 2.1.3 mSUGRA: the constrained MSSM 2.1.4 The MSSMi: the intermediate MSSMs 2.2 Electroweak Symmetry Breaking 2.2.1 General features 2.2.2 EWSB and model–independent tanβ bounds 2.3 Renormalization Group Evolution 2.3.1 The one–loop RGEs 2.3.2 Exact solutions for the Yukawa coupling RGEs 3. -
Color Screening in Quantum Chromodynamics Arxiv
Color Screening in Quantum Chromodynamics Alexei Bazavov, Johannes H. Weber Department of Computational Mathematics, Science and Engineering and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA October 6, 2020 Abstract We review lattice studies of the color screening in the quark-gluon plasma. We put the phenomena related to the color screening into the context of similar aspects of other physical systems (electromag- netic plasma or cold nuclear matter). We discuss the onset of the color screening and its signature and significance in the QCD transi- tion region, and elucidate at which temperature and to which extent the weak-coupling picture based on hard thermal loop expansion, po- tential nonrelativistic QCD, or dimensionally-reduced QCD quantita- tively captures the key properties of the color screening. We discuss the different regimes pertaining to the color screening and thermal arXiv:2010.01873v1 [hep-lat] 5 Oct 2020 dissociation of the static quarks in depth for various spatial correla- tion functions that are studied on the lattice, and clarify the status of their asymptotic screening masses. We finally discuss the screening correlation functions of dynamical mesons with a wide range of flavor and spin content, and how they conform with expectations for low- and high-temperature behavior. 1 Contents 1 Introduction3 2 Field theoretical foundations7 2.1 Partition function and Lagrangian . .7 2.2 Finite temperature field theory . 11 2.3 Lattice regularization . 14 2.4 Renormalization and weak coupling . 17 2.5 Light quarks . 19 2.6 Heavy quarks . 21 2.7 Implementation of QCD on the lattice . -
The Magnetic Dipole Moment of the Muon in Different SUSY Models
The magnetic dipole moment of the muon in different SUSY models Bachelor-Arbeit zur Erlangung des Hochschulgrades Bachelor of Science im Bachelor-Studiengang Physik vorgelegt von Jobst Ziebell geboren am 05.11.1992 in Herrljunga Institut für Kern- und Teilchenphysik Fachrichtung Physik Fakultät Mathematik und Naturwissenschaften Technische Universität Dresden 2015 Eingereicht am 1. Juli 2015 1. Gutachter: Prof. Dr. Dominik Stöckinger 2. Gutachter: Prof. Dr. Kai Zuber Abstract The magnetic dipole moment of the muon is one of the most precisely measured quantities in modern physics. Theory however predicts values that disagree with measurement by several standard deviations [1, Abstract]. Because this may hint at physics beyond the standard model, it is a great opportunity to ex- amine the magnetic dipole moment in different supersymmetric models. It is then possible to calculate dependences of the dipole moment on various model parameters as well as to find constraints for their particular values. The purpose of this paper is to describe how the magnetic dipole moment is obtained in su- persymmetric extensions of the standard model and to document the implementation of its calculation in FlexibleSUSY, a spectrum generator for supersymmetric models [2, Abstract]. Contents 1 Introduction 1 2 The gyromagnetic ratio 2 2.1 In classical mechanics . .2 2.2 In quantum mechanics . .3 2.3 In quantum field theory . .4 3 The implementation in FlexibleSUSY 7 3.1 The C++ part . .7 3.2 The Mathematica part . 11 3.3 The FlexibleSUSY part . 12 4 Results 13 Appendices 17 A The Loop functions . 17 B The VertexFunction template . 17 C The DiagramEvaluator<...>::value() functions . -
Supersymmetric Particle Searches
Citation: K.A. Olive et al. (Particle Data Group), Chin. Phys. C38, 090001 (2014) (URL: http://pdg.lbl.gov) Supersymmetric Particle Searches A REVIEW GOES HERE – Check our WWW List of Reviews A REVIEW GOES HERE – Check our WWW List of Reviews SUPERSYMMETRIC MODEL ASSUMPTIONS The exclusion of particle masses within a mass range (m1, m2) will be denoted with the notation “none m m ” in the VALUE column of the 1− 2 following Listings. The latest unpublished results are described in the “Supersymmetry: Experiment” review. A REVIEW GOES HERE – Check our WWW List of Reviews CONTENTS: χ0 (Lightest Neutralino) Mass Limit 1 e Accelerator limits for stable χ0 − 1 Bounds on χ0 from dark mattere searches − 1 χ0-p elastice cross section − 1 eSpin-dependent interactions Spin-independent interactions Other bounds on χ0 from astrophysics and cosmology − 1 Unstable χ0 (Lighteste Neutralino) Mass Limit − 1 χ0, χ0, χ0 (Neutralinos)e Mass Limits 2 3 4 χe ,eχ e(Charginos) Mass Limits 1± 2± Long-livede e χ± (Chargino) Mass Limits ν (Sneutrino)e Mass Limit Chargede Sleptons e (Selectron) Mass Limit − µ (Smuon) Mass Limit − e τ (Stau) Mass Limit − e Degenerate Charged Sleptons − e ℓ (Slepton) Mass Limit − q (Squark)e Mass Limit Long-livede q (Squark) Mass Limit b (Sbottom)e Mass Limit te (Stop) Mass Limit eHeavy g (Gluino) Mass Limit Long-lived/lighte g (Gluino) Mass Limit Light G (Gravitino)e Mass Limits from Collider Experiments Supersymmetrye Miscellaneous Results HTTP://PDG.LBL.GOV Page1 Created: 8/21/2014 12:57 Citation: K.A. Olive et al. -
R-Parity Violation and Light Neutralinos at Ship and the LHC
BONN-TH-2015-12 R-Parity Violation and Light Neutralinos at SHiP and the LHC Jordy de Vries,1, ∗ Herbi K. Dreiner,2, y and Daniel Schmeier2, z 1Institute for Advanced Simulation, Institut f¨urKernphysik, J¨ulichCenter for Hadron Physics, Forschungszentrum J¨ulich, D-52425 J¨ulich, Germany 2Physikalisches Institut der Universit¨atBonn, Bethe Center for Theoretical Physics, Nußallee 12, 53115 Bonn, Germany We study the sensitivity of the proposed SHiP experiment to the LQD operator in R-Parity vi- olating supersymmetric theories. We focus on single neutralino production via rare meson decays and the observation of downstream neutralino decays into charged mesons inside the SHiP decay chamber. We provide a generic list of effective operators and decay width formulae for any λ0 cou- pling and show the resulting expected SHiP sensitivity for a widespread list of benchmark scenarios via numerical simulations. We compare this sensitivity to expected limits from testing the same decay topology at the LHC with ATLAS. I. INTRODUCTION method to search for a light neutralino, is via the pro- duction of mesons. The rate for the latter is so high, Supersymmetry [1{3] is the unique extension of the ex- that the subsequent rare decay of the meson to the light ternal symmetries of the Standard Model of elementary neutralino via (an) R-parity violating operator(s) can be particle physics (SM) with fermionic generators [4]. Su- searched for [26{28]. This is analogous to the production persymmetry is necessarily broken, in order to comply of neutrinos via π or K-mesons. with the bounds from experimental searches. -
String Phenomenology 1 Minimal Supersymmetric Standard Model
Swedish String/Supergravity Course 2008 String Phenomenology Marcus Berg 1 Minimal Supersymmetric Standard Model A good reference is Martin [2], a review that was first posted on hep-ph in 1997 but which has been updated three times, most recently in 2006. The MSSM consists of a number of chiral and vector supermultiplets, one for each existing quark or 1 lepton or gauge boson Aµ in the Standard Model (SM): spin: 0 1/2 1 N = 1 chiral supermultiplet φ N = 1 vector supermultiplet λ Aµ The new fields, the superpartners of and Aµ, are denoted by tildes and called "s-" for the new scalars, ~, and "-ino" for the new fermions, A~: 0 1/2 1 squarks, sleptons −! ~ − quarks, leptons gauginos−! A~ Aµ − gauge bosons This is just the generic notation; usually one is more specific. So for example, one N = 1 chiral mul- tiplet has the t quark as the fermionic field, and the scalar superpartner is the "stop", t~. We impose that the superpartner masses are around the TeV scale, or even a little lower. The scale of superpartner masses is not \derived" in any real sense2 in the MSSM, but from the point of view of particle phenomenology, an MSSM-like theory with only very heavy superpartners would be indistinguishable from the nonsuper- symmetric standard model at any experiments done in the foreseeable future, so why bother? In fact, even string theorists should have some favored scenario what will happen at near-future experiments and observations, so let's try to understand where people who do experiments for a living have put their money. -
Arxiv:1711.04534V4 [Hep-Ph]
UCI-HEP-TR-2017-15 Millicharged Scalar Fields, Massive Photons and the Breaking of SU(3)C U(1)EM × Jennifer Rittenhouse West∗ Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA and SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94309, USA (Dated: April 10, 2019) Under the assumption that the current epoch of the Universe is not special, i.e. is not the final state of a long history of processes in particle physics, the cosmological fate of SU(3)C × U(1)EM is investigated. Spontaneous symmetry breaking of U(1)EM at the temperature of the Universe today is carried out. The charged scalar field φEM which breaks the symmetry is found to be ruled out for the charge of the electron, q = e. − Scalar fields with millicharges are viable and limits on their masses and charges are found to be q . 10 3e and −5 mφEM . 10 eV. Furthermore, it is possible that U(1)EM has already been broken at temperatures higher −18 than T = 2.7K given the nonzero limits on the mass of the photon. A photon mass of mγ = 10 eV, the ∼ −13 current upper limit, is found to require a spontaneous symmetry breaking scalar mass of mφEM 10 eV with charge q = 10−6e, well within the allowed parameter space of the model. Finally, the cosmological fate of the strong interaction is studied. SU(3)C is tested for complementarity in which the confinement phase of QCD + colored scalars is equivalent to a spontaneously broken SU(3) gauge theory. -
A Study of Mesons and Glueballs
A Study of Mesons and Glueballs Tapashi Das Department of Physics Gauhati University This thesis is submitted to Gauhati University as requirement for the degree of Doctor of Philosophy Faculty of Science July 2017 Scanned by CamScanner Scanned by CamScanner Scanned by CamScanner Scanned by CamScanner Abstract The main work of the thesis is devoted to the study of heavy flavored mesons using a QCD potential model. Chapter 1 deals with the brief introduction of the theory of Quantum Chro- modynamics (QCD), potential models and the use of perturbation theory. In Chapter 2, the improved potential model is introduced and the solution of the non-relativistic Schro¨dinger’s equation for a Coulomb-plus-linear potential, V(r) = 4αs + br + c, Cornell potential has − 3r been conducted. The first-order wave functions are obtained using Dalgarno’s method. We explicitly consider two quantum mechanical aspects in our improved model: (a) the scale factor ‘c’ in the potential should not affect the wave function of the system even while applying the perturbation theory and (b) the choice of perturbative piece of the Hamiltonian (confinement or linear) should determine the effective radial separation between the quarks and antiquarks. Therefore for the validation of the quantum mechanical idea, the constant factor ‘c’ is considered to be zero and a cut-off rP is obtained from the theory. The model is then tested to calculate the masses, form factors, charge radii, RMS radii of mesons. In Chapter 3, the Isgur-Wise function and its derivatives of semileptonic decays of heavy-light mesons in both HQET limit (m ∞) and finite mass limit are calculated.