Two-Component Fermion Notation and Supersymmetry
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Path Integrals in Quantum Mechanics
Path Integrals in Quantum Mechanics Dennis V. Perepelitsa MIT Department of Physics 70 Amherst Ave. Cambridge, MA 02142 Abstract We present the path integral formulation of quantum mechanics and demon- strate its equivalence to the Schr¨odinger picture. We apply the method to the free particle and quantum harmonic oscillator, investigate the Euclidean path integral, and discuss other applications. 1 Introduction A fundamental question in quantum mechanics is how does the state of a particle evolve with time? That is, the determination the time-evolution ψ(t) of some initial | i state ψ(t ) . Quantum mechanics is fully predictive [3] in the sense that initial | 0 i conditions and knowledge of the potential occupied by the particle is enough to fully specify the state of the particle for all future times.1 In the early twentieth century, Erwin Schr¨odinger derived an equation specifies how the instantaneous change in the wavefunction d ψ(t) depends on the system dt | i inhabited by the state in the form of the Hamiltonian. In this formulation, the eigenstates of the Hamiltonian play an important role, since their time-evolution is easy to calculate (i.e. they are stationary). A well-established method of solution, after the entire eigenspectrum of Hˆ is known, is to decompose the initial state into this eigenbasis, apply time evolution to each and then reassemble the eigenstates. That is, 1In the analysis below, we consider only the position of a particle, and not any other quantum property such as spin. 2 D.V. Perepelitsa n=∞ ψ(t) = exp [ iE t/~] n ψ(t ) n (1) | i − n h | 0 i| i n=0 X This (Hamiltonian) formulation works in many cases. -
Constraints from Electric Dipole Moments on Chargino Baryogenesis in the Minimal Supersymmetric Standard Model
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by National Tsing Hua University Institutional Repository PHYSICAL REVIEW D 66, 116008 ͑2002͒ Constraints from electric dipole moments on chargino baryogenesis in the minimal supersymmetric standard model Darwin Chang NCTS and Physics Department, National Tsing-Hua University, Hsinchu 30043, Taiwan, Republic of China and Theory Group, Lawrence Berkeley Lab, Berkeley, California 94720 We-Fu Chang NCTS and Physics Department, National Tsing-Hua University, Hsinchu 30043, Taiwan, Republic of China and TRIUMF Theory Group, Vancouver, British Columbia, Canada V6T 2A3 Wai-Yee Keung NCTS and Physics Department, National Tsing-Hua University, Hsinchu 30043, Taiwan, Republic of China and Physics Department, University of Illinois at Chicago, Chicago, Illinois 60607-7059 ͑Received 9 May 2002; revised 13 September 2002; published 27 December 2002͒ A commonly accepted mechanism of generating baryon asymmetry in the minimal supersymmetric standard model ͑MSSM͒ depends on the CP violating relative phase between the gaugino mass and the Higgsino term. The direct constraint on this phase comes from the limit of electric dipole moments ͑EDM’s͒ of various light fermions. To avoid such a constraint, a scheme which assumes that the first two generation sfermions are very heavy is usually evoked to suppress the one-loop EDM contributions. We point out that under such a scheme the most severe constraint may come from a new contribution to the electric dipole moment of the electron, the neutron, or atoms via the chargino sector at the two-loop level. As a result, the allowed parameter space for baryogenesis in the MSSM is severely constrained, independent of the masses of the first two generation sfermions. -
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. -
Supersymmetric Dark Matter
Supersymmetric dark matter G. Bélanger LAPTH- Annecy Plan | Dark matter : motivation | Introduction to supersymmetry | MSSM | Properties of neutralino | Status of LSP in various SUSY models | Other DM candidates z SUSY z Non-SUSY | DM : signals, direct detection, LHC Dark matter: a WIMP? | Strong evidence that DM dominates over visible matter. Data from rotation curves, clusters, supernovae, CMB all point to large DM component | DM a new particle? | SM is incomplete : arbitrary parameters, hierarchy problem z DM likely to be related to physics at weak scale, new physics at the weak scale can also solve EWSB z Stable particle protect by symmetry z Many solutions – supersymmetry is one best motivated alternative to SM | NP at electroweak scale could also explain baryonic asymetry in the universe Relic density of wimps | In early universe WIMPs are present in large number and they are in thermal equilibrium | As the universe expanded and cooled their density is reduced Freeze-out through pair annihilation | Eventually density is too low for annihilation process to keep up with expansion rate z Freeze-out temperature | LSP decouples from standard model particles, density depends only on expansion rate of the universe | Relic density | A relic density in agreement with present measurements (Ωh2 ~0.1) requires typical weak interactions cross-section Coannihilation | If M(NLSP)~M(LSP) then maintains thermal equilibrium between NLSP-LSP even after SUSY particles decouple from standard ones | Relic density then depends on rate for all processes -
Effective Dirac Equations in Honeycomb Structures
Effective Dirac equations in honeycomb structures Effective Dirac equations in honeycomb structures Young Researchers Seminar, CERMICS, Ecole des Ponts ParisTech William Borrelli CEREMADE, Universit´eParis Dauphine 11 April 2018 It is self-adjoint on L2(R2; C2) and the spectrum is given by σ(D0) = R; σ(D) = (−∞; −m] [ [m; +1) The domain of the operator and form domain are H1(R2; C2) and 1 2 2 H 2 (R ; C ), respectively. Remark The negative spectrum is associated with antiparticles, in relativistic theories. Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle. It acts on C2-valued spinors. The domain of the operator and form domain are H1(R2; C2) and 1 2 2 H 2 (R ; C ), respectively. Remark The negative spectrum is associated with antiparticles, in relativistic theories. Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle. It acts on C2-valued spinors. It is self-adjoint on L2(R2; C2) and the spectrum is given by σ(D0) = R; σ(D) = (−∞; −m] [ [m; +1) Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle. -
Majorana Fermions in Condensed Matter Physics: the 1D Nanowire Case
Majorana Fermions in Condensed Matter Physics: The 1D Nanowire Case Philip Haupt, Hirsh Kamakari, Edward Thoeng, Aswin Vishnuradhan Department of Physics and Astronomy, University of British Columbia, Vancouver, B.C., V6T 1Z1, Canada (Dated: November 24, 2018) Majorana fermions are fermions that are their own antiparticles. Although they remain elusive as elementary particles (how they were originally proposed), they have rapidly gained interest in condensed matter physics as emergent quasiparticles in certain systems like topological supercon- ductors. In this article, we briefly review the necessary theory and discuss the \recipe" to create Majorana particles. We then consider existing experimental realisations and their methodologies. I. MOTIVATION A). Kitaev used a simplified quantum wire model to show Ettore Majorana, in 1937, postulated the existence of how Majorana modes might manifest as an emergent an elementary particle which is its own antiparticle, so phenomena, which we will now discuss. Consider 1- called Majorana fermions [1]. It is predicted that the neu- dimensional tight binding chain with spinless fermions trinos are one such elementary particle, which is yet to and p-orbital hopping. The use of unphysical spinless be detected via extremely rare neutrino-less double beta- fermions calls into question the validity of the model, decay. The research on Majorana fermions in the past but, as has been subsequently realised, in the presence few years, however, have gained momentum in the com- of strong spin orbit coupling it is possible for electrons pletely different field of condensed matter physics. Arti- to be approximated as spinless in the presence of spin- ficially engineered low-dimensional nanostructures which orbit coupling as well as a Zeeman field [9]. -
$ Z $ Boson Mediated Dark Matter Beyond the Effective Theory
MCTP-16-27 FERMILAB-PUB-16-534-T Z boson mediated dark matter beyond the effective theory John Kearney Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, IL 60510 USA Nicholas Orlofsky and Aaron Pierce Michigan Center for Theoretical Physics (MCTP) Department of Physics, University of Michigan, Ann Arbor, MI 48109 (Dated: April 11, 2017) Direct detection bounds are beginning to constrain a very simple model of weakly interacting dark matter|a Majorana fermion with a coupling to the Z boson. In a particularly straightforward gauge-invariant realization, this coupling is introduced via a higher-dimensional operator. While attractive in its simplicity, this model generically induces a large ρ parameter. An ultraviolet completion that avoids an overly large contribution to ρ is the singlet-doublet model. We revisit this model, focusing on the Higgs blind spot region of parameter space where spin-independent interactions are absent. This model successfully reproduces dark matter with direct detection mediated by the Z boson, but whose cosmology may depend on additional couplings and states. Future direct detection experiments should effectively probe a significant portion of this parameter space, aside from a small coannihilating region. As such, Z-mediated thermal dark matter as realized in the singlet-doublet model represents an interesting target for future searches. I. INTRODUCTION Z, and their spin-dependent (SD) couplings, which at tree level arise from exchange of the Z. The latest bounds on SI scattering arise from PandaX Weakly interacting massive particles (WIMPs) re- [1] and LUX [2]. DM that interacts with the Z main an attractive thermal dark matter (DM) can- boson via vectorial couplings, g (¯χγ χ)Zµ, is very didate. -
Quantum Statistics: Is There an Effective Fermion Repulsion Or Boson Attraction? W
Quantum statistics: Is there an effective fermion repulsion or boson attraction? W. J. Mullin and G. Blaylock Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003 ͑Received 13 February 2003; accepted 16 May 2003͒ Physicists often claim that there is an effective repulsion between fermions, implied by the Pauli principle, and a corresponding effective attraction between bosons. We examine the origins and validity of such exchange force ideas and the areas where they are highly misleading. We propose that explanations of quantum statistics should avoid the idea of an effective force completely, and replace it with more appropriate physical insights, some of which are suggested here. © 2003 American Association of Physics Teachers. ͓DOI: 10.1119/1.1590658͔ ͒ϭ ͒ Ϫ␣ Ϫ ϩ ͒2 I. INTRODUCTION ͑x1 ,x2 ,t C͕f ͑x1 ,x2 exp͓ ͑x1 vt a Ϫ͑x ϩvtϪa͒2͔Ϫ f ͑x ,x ͒ The Pauli principle states that no two fermions can have 2 2 1 ϫ Ϫ␣ Ϫ ϩ ͒2Ϫ ϩ Ϫ ͒2 the same quantum numbers. The origin of this law is the exp͓ ͑x2 vt a ͑x1 vt a ͔͖, required antisymmetry of the multi-fermion wavefunction. ͑1͒ Most physicists have heard or read a shorthand way of ex- pressing the Pauli principle, which says something analogous where x1 and x2 are the particle coordinates, f (x1 ,x2) ϭ ͓ Ϫ ប͔ to fermions being ‘‘antisocial’’ and bosons ‘‘gregarious.’’ Of- exp imv(x1 x2)/ , C is a time-dependent factor, and the ten this intuitive approach involves the statement that there is packet width parameters ␣ and  are unequal. -
Table of Contents (Print)
PERIODICALS PHYSICAL REVIEW D Postmaster send address changes to: For editorial and subscription correspondence, PHYSICAL REVIEW D please see inside front cover APS Subscription Services „ISSN: 0556-2821… Suite 1NO1 2 Huntington Quadrangle Melville, NY 11747-4502 THIRD SERIES, VOLUME 69, NUMBER 7 CONTENTS D1 APRIL 2004 RAPID COMMUNICATIONS ϩ 0 ⌼ ϩ→ ϩ 0→ 0 Measurement of the B /B production ratio from the (4S) meson using B J/ K and B J/ KS decays (7 pages) ............................................................................ 071101͑R͒ B. Aubert et al. ͑BABAR Collaboration͒ Cabibbo-suppressed decays of Dϩ→ϩ0,KϩK¯ 0,Kϩ0 (5 pages) .................................. 071102͑R͒ K. Arms et al. ͑CLEO Collaboration͒ Ϯ→ Ϯ ͑ ͒ Measurement of the branching fraction for B c0K (7 pages) ................................... 071103R B. Aubert et al. ͑BABAR Collaboration͒ Generalized Ward identity and gauge invariance of the color-superconducting gap (5 pages) .............. 071501͑R͒ De-fu Hou, Qun Wang, and Dirk H. Rischke ARTICLES Measurements of (2S) decays into vector-tensor final states (6 pages) ............................... 072001 J. Z. Bai et al. ͑BES Collaboration͒ Measurement of inclusive momentum spectra and multiplicity distributions of charged particles at ͱsϳ2 –5 GeV (7 pages) ................................................................... 072002 J. Z. Bai et al. ͑BES Collaboration͒ Production of ϩ, Ϫ, Kϩ, KϪ, p, and ¯p in light ͑uds͒, c, and b jets from Z0 decays (26 pages) ........ 072003 Koya Abe et al. ͑SLD Collaboration͒ Heavy flavor properties of jets produced in pp¯ interactions at ͱsϭ1.8 TeV (21 pages) .................. 072004 D. Acosta et al. ͑CDF Collaboration͒ Electric charge and magnetic moment of a massive neutrino (21 pages) ............................... 073001 Maxim Dvornikov and Alexander Studenikin → decays in the resonance effective theory (13 pages) .................................... -
A Generalization of the One-Dimensional Boson-Fermion Duality Through the Path-Integral Formalsim
A Generalization of the One-Dimensional Boson-Fermion Duality Through the Path-Integral Formalism Satoshi Ohya Institute of Quantum Science, Nihon University, Kanda-Surugadai 1-8-14, Chiyoda, Tokyo 101-8308, Japan [email protected] (Dated: May 11, 2021) Abstract We study boson-fermion dualities in one-dimensional many-body problems of identical parti- cles interacting only through two-body contacts. By using the path-integral formalism as well as the configuration-space approach to indistinguishable particles, we find a generalization of the boson-fermion duality between the Lieb-Liniger model and the Cheon-Shigehara model. We present an explicit construction of n-boson and n-fermion models which are dual to each other and characterized by n−1 distinct (coordinate-dependent) coupling constants. These models enjoy the spectral equivalence, the boson-fermion mapping, and the strong-weak duality. We also discuss a scale-invariant generalization of the boson-fermion duality. arXiv:2105.04288v1 [quant-ph] 10 May 2021 1 1 Introduction Inhisseminalpaper[1] in 1960, Girardeau proved the one-to-one correspondence—the duality—between one-dimensional spinless bosons and fermions with hard-core interparticle interactions. By using this duality, he presented a celebrated example of the spectral equivalence between impenetrable bosons and free fermions. Since then, the one-dimensional boson-fermion duality has been a testing ground for studying strongly-interacting many-body problems, especially in the field of integrable models. So far there have been proposed several generalizations of the Girardeau’s finding, the most promi- nent of which was given by Cheon and Shigehara in 1998 [2]: they discovered the fermionic dual of the Lieb-Liniger model [3] by using the generalized pointlike interactions. -
1 Standard Model: Successes and Problems
Searching for new particles at the Large Hadron Collider James Hirschauer (Fermi National Accelerator Laboratory) Sambamurti Memorial Lecture : August 7, 2017 Our current theory of the most fundamental laws of physics, known as the standard model (SM), works very well to explain many aspects of nature. Most recently, the Higgs boson, predicted to exist in the late 1960s, was discovered by the CMS and ATLAS collaborations at the Large Hadron Collider at CERN in 2012 [1] marking the first observation of the full spectrum of predicted SM particles. Despite the great success of this theory, there are several aspects of nature for which the SM description is completely lacking or unsatisfactory, including the identity of the astronomically observed dark matter and the mass of newly discovered Higgs boson. These and other apparent limitations of the SM motivate the search for new phenomena beyond the SM either directly at the LHC or indirectly with lower energy, high precision experiments. In these proceedings, the successes and some of the shortcomings of the SM are described, followed by a description of the methods and status of the search for new phenomena at the LHC, with some focus on supersymmetry (SUSY) [2], a specific theory of physics beyond the standard model (BSM). 1 Standard model: successes and problems The standard model of particle physics describes the interactions of fundamental matter particles (quarks and leptons) via the fundamental forces (mediated by the force carrying particles: the photon, gluon, and weak bosons). The Higgs boson, also a fundamental SM particle, plays a central role in the mechanism that determines the masses of the photon and weak bosons, as well as the rest of the standard model particles. -
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.