Exotic Goldstone Particles: Pseudo-Goldstone Boson and Goldstone Fermion
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Goldstini Can Give the Higgs a Boost
Goldstini Can Give the Higgs a Boost The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Thaler, Jesse, and Zachary Thomas. “Goldstini can give the Higgs a boost.” Journal of High Energy Physics 2011.7 (2011). As Published http://dx.doi.org/10.1007/jhep07(2011)060 Publisher Springer Berlin/Heidelberg Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/72016 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike 3.0 Detailed Terms http://creativecommons.org/licenses/by-nc-sa/3.0/ Preprint typeset in JHEP style - HYPER VERSION MIT-CTP 4226 Goldstini Can Give the Higgs a Boost Jesse Thaler and Zachary Thomas Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA E-mail: [email protected], [email protected] Abstract: Supersymmetric collider phenomenology depends crucially on whether the lightest observable-sector supersymmetric particle (LOSP) decays, and if so, what the LOSP decay products are. For instance, in SUSY models where the gravitino is lighter than the LOSP, the LOSP decays to its superpartner and a longitudinal gravitino via super- current couplings. In this paper, we show that LOSP decays can be substantially modified when there are multiple sectors that break supersymmetry, where in addition to the grav- itino there are light uneaten goldstini. As a particularly striking example, a bino-like LOSP can have a near 100% branching fraction to a higgs boson and an uneaten goldstino, even if the LOSP has negligible higgsino fraction. This occurs because the uneaten goldstino is unconstrained by the supercurrent, allowing additional operators to mediate LOSP decay. -
3. Models of EWSB
The Higgs Boson and Electroweak Symmetry Breaking 3. Models of EWSB M. E. Peskin Chiemsee School September 2014 In this last lecture, I will take up a different topic in the physics of the Higgs field. In the first lecture, I emphasized that most of the parameters of the Standard Model are associated with the couplings of the Higgs field. These parameters determine the Higgs potential, the spectrum of quark and lepton masses, and the structure of flavor and CP violation in the weak interactions. These parameters are not computable within the SM. They are inputs. If we want to compute these parameters, we need to build a deeper and more predictive theory. In particular, a basic question about the SM is: Why is the SU(2)xU(1) gauge symmetry spontaneously broken ? The SM cannot answer this question. I will discuss: In what kind of models can we answer this question ? For orientation, I will present the explanation for spontaneous symmetry breaking in the SM. We have a single Higgs doublet field ' . It has some potential V ( ' ) . The potential is unknown, except that it is invariant under SU(2)xU(1). However, if the theory is renormalizable, the potential must be of the form V (')=µ2 ' 2 + λ ' 4 | | | | Now everything depends on the sign of µ 2 . If µ2 > 0 the minimum of the potential is at ' =0 and there is no symmetry breaking. If µ 2 < 0 , the potential has the form: and there is a minimum away from 0. That’s it. Don’t ask any more questions. -
Symmetries of the Strong Interaction
Symmetries of the strong interaction H. Leutwyler University of Bern DFG-Graduiertenkolleg ”Quanten- und Gravitationsfelder” Jena, 19. Mai 2009 H. Leutwyler – Bern Symmetries of the strong interaction – p. 1/33 QCD with 3 massless quarks As far as the strong interaction goes, the only difference between the quark flavours u,d,...,t is the mass mu, md, ms happen to be small For massless fermions, the right- and left-handed components lead a life of their own Fictitious world with mu =md =ms =0: QCD acquires an exact chiral symmetry No distinction between uL,dL,sL, nor between uR,dR,sR Hamiltonian is invariant under SU(3) SU(3) ⇒ L× R H. Leutwyler – Bern Symmetries of the strong interaction – p. 2/33 Chiral symmetry of QCD is hidden Chiral symmetry is spontaneously broken: Ground state is not symmetric under SU(3) SU(3) L× R symmetric only under the subgroup SU(3)V = SU(3)L+R Mesons and baryons form degenerate SU(3)V multiplets ⇒ and the lowest multiplet is massless: Mπ± =Mπ0 =MK± =MK0 =MK¯ 0 =Mη =0 Goldstone bosons of the hidden symmetry H. Leutwyler – Bern Symmetries of the strong interaction – p. 3/33 Spontane Magnetisierung Heisenbergmodell eines Ferromagneten Gitter von Teilchen, Wechselwirkung zwischen Spins Hamiltonoperator ist drehinvariant Im Zustand mit der tiefsten Energie zeigen alle Spins in dieselbe Richtung: Spontane Magnetisierung Grundzustand nicht drehinvariant ⇒ Symmetrie gegenüber Drehungen gar nicht sichtbar Symmetrie ist versteckt, spontan gebrochen Goldstonebosonen in diesem Fall: "Magnonen", "Spinwellen" Haben keine Energielücke: ω 0 für λ → → ∞ Nambu realisierte, dass auch in der Teilchenphysik Symmetrien spontan zusammenbrechen können H. -
Super-Higgs in Superspace
Article Super-Higgs in Superspace Gianni Tallarita 1,* and Moritz McGarrie 2 1 Departamento de Ciencias, Facultad de Artes Liberales, Universidad Adolfo Ibáñez, Santiago 7941169, Chile 2 Deutsches Elektronen-Synchrotron, DESY, Notkestrasse 85, 22607 Hamburg, Germany; [email protected] * Correspondence: [email protected] or [email protected] Received: 1 April 2019; Accepted: 10 June 2019; Published: 14 June 2019 Abstract: We determine the effective gravitational couplings in superspace whose components reproduce the supergravity Higgs effect for the constrained Goldstino multiplet. It reproduces the known Gravitino sector while constraining the off-shell completion. We show that these couplings arise by computing them as quantum corrections. This may be useful for phenomenological studies and model-building. We give an example of its application to multiple Goldstini. Keywords: supersymmetry; Goldstino; superspace 1. Introduction The spontaneous breakdown of global supersymmetry generates a massless Goldstino [1,2], which is well described by the Akulov-Volkov (A-V) effective action [3]. When supersymmetry is made local, the Gravitino “eats” the Goldstino of the A-V action to become massive: The super-Higgs mechanism [4,5]. In terms of superfields, the constrained Goldstino multiplet FNL [6–12] is equivalent to the A-V formulation (see also [13–17]). It is, therefore, natural to extend the description of supergravity with this multiplet, in superspace, to one that can reproduce the super-Higgs mechanism. In this paper we address two issues—first we demonstrate how the Gravitino, Goldstino, and multiple Goldstini obtain a mass. Secondly, by using the Spurion analysis, we write down the most minimal set of new terms in superspace that incorporate both supergravity and the Goldstino multiplet in order to reproduce the super-Higgs mechanism of [5,18] at lowest order in M¯ Pl. -
Goldstone Theorem, Higgs Mechanism
Introduction to the Standard Model Lecture 12 Classical Goldstone Theorem and Higgs Mechanism The Classical Goldstone Theorem: To each broken generator corresponds a massless field (Goldstone boson). Proof: 2 ∂ V Mij = ∂φi∂φj φ~= φ~ h i V (φ~)=V (φ~ + iεaT aφ~) ∂V =V (φ~)+ iεaT aφ~ + ( ε 2) ∂φj O | | ∂ ∂V a Tjlφl =0 ⇒∂φk ∂φj 2 ∂ ∂V a ∂ V a ∂V a Til φl = Tjlφl + Tik ∂φk ∂φi ∂φi∂φj ∂φi φ~= φ~ h i 0= M T a φ +0 ki il h li =~0i | 6 {z } If T a is a broken generator one has T a φ~ = ~0 h i 6 ⇒ Mik has a null eigenvector null eigenvalues massless particle since the eigenvalues of the mass matrix are the particle⇒ masses. ⇒ We now combine the concept of a spontaneously broken symmetry to a gauge theory. The Higgs Mechanism for U(1) gauge theory Consider µ 2 2 1 µν = D φ∗ D φ µ φ∗φ λ φ∗φ F F L µ − − − 4 µν µν µ ν ν µ with Dµ = ∂µ + iQAµ and F = ∂ A ∂ A . Gauge symmetry here means invariance under Aµ Aµ ∂µΛ. − → − 2 2 2 case a) unbroken case, µ > 0 : V (φ)= µ φ∗φ + λ φ∗φ with a minimum at φ = 0. The ground state or vaccuum is U(1) symmetric. The corresponding theory is known as Scalar Electrodynamics of a massive spin-0 boson with mass µ and charge Q. 1 case b) nontrivial vaccuum case 2 µ 2 v iα V (φ) has a minimum for 2 φ∗φ = − = v which gives φ = e . -
TASI 2008 Lectures: Introduction to Supersymmetry And
TASI 2008 Lectures: Introduction to Supersymmetry and Supersymmetry Breaking Yuri Shirman Department of Physics and Astronomy University of California, Irvine, CA 92697. [email protected] Abstract These lectures, presented at TASI 08 school, provide an introduction to supersymmetry and supersymmetry breaking. We present basic formalism of supersymmetry, super- symmetric non-renormalization theorems, and summarize non-perturbative dynamics of supersymmetric QCD. We then turn to discussion of tree level, non-perturbative, and metastable supersymmetry breaking. We introduce Minimal Supersymmetric Standard Model and discuss soft parameters in the Lagrangian. Finally we discuss several mech- anisms for communicating the supersymmetry breaking between the hidden and visible sectors. arXiv:0907.0039v1 [hep-ph] 1 Jul 2009 Contents 1 Introduction 2 1.1 Motivation..................................... 2 1.2 Weylfermions................................... 4 1.3 Afirstlookatsupersymmetry . .. 5 2 Constructing supersymmetric Lagrangians 6 2.1 Wess-ZuminoModel ............................... 6 2.2 Superfieldformalism .............................. 8 2.3 VectorSuperfield ................................. 12 2.4 Supersymmetric U(1)gaugetheory ....................... 13 2.5 Non-abeliangaugetheory . .. 15 3 Non-renormalization theorems 16 3.1 R-symmetry.................................... 17 3.2 Superpotentialterms . .. .. .. 17 3.3 Gaugecouplingrenormalization . ..... 19 3.4 D-termrenormalization. ... 20 4 Non-perturbative dynamics in SUSY QCD 20 4.1 Affleck-Dine-Seiberg -
2.4 Spontaneous Chiral Symmetry Breaking
70 Hadrons 2.4 Spontaneous chiral symmetry breaking We have earlier seen that renormalization introduces a scale. Without a scale in the theory all hadrons would be massless (at least for vanishing quark masses), so the anomalous breaking of scale invariance is a necessary ingredient to understand their nature. The second ingredient is spontaneous chiral symmetry breaking. We will see that this mechanism plays a quite important role in the light hadron spectrum: it is not only responsible for the Goldstone nature of the pions, but also the origin of the 'constituent quarks' which produce the typical hadronic mass scales of 1 GeV. ∼ Spontaneous symmetry breaking. Let's start with some general considerations. Suppose 'i are a set of (potentially composite) fields which transform nontrivially under some continuous global symmetry group G. For an infinitesimal transformation we have δ'i = i"a(ta)ij 'j, where "a are the group parameters and ta the generators of the Lie algebra of G in the representation to which the 'i belong. Let's call the representation matrices Dij(") = exp(i"ata)ij. The quantum-field theoretical version of this relation is ei"aQa ' e−i"aQa = D−1(") ' [Q ;' ] = (t ) ' ; (2.128) i ij j , a i − a ij j where the charge operators Qa form a representation of the algebra on the Hilbert space. (An example of this is Eq. (2.47).) If the symmetry group leaves the vacuum invariant, ei"aQa 0 = 0 , then all generators Q must annihilate the vacuum: Q 0 = 0. Hence, j i j i a aj i when we take the vacuum expectation value (VEV) of this equation we get 0 ' 0 = D−1(") 0 ' 0 : (2.129) h j ij i ij h j jj i If the 'i had been invariant under G to begin with, this relation would be trivially −1 satisfied. -
The Equivalence Theorem and the Production of Gravitinos After Inflation
CERN-TH/99-373 The equivalence theorem and the production of gravitinos after inflation 1; 2; Antonio L. Maroto ∗ and Jos´eR.Pel´aez † 1CERN Theory Division, CH-1211 Geneva 23, Switzerland 2Departamento de F´ısica Te´orica, Universidad Complutense de Madrid, 28040 Madrid, Spain ABSTRACT We study the application of the high-energy equivalence between helicity 1/2 gravitinos and goldstinos in order to calculate the production of helicity 1/2 gravitinos± in time-dependent scalar and gravitational backgrounds. We derive this equivalence± for equations of motion, paying attention to several subtleties that appear in this context and are not present in the standard derivations of the theorem, mainly because of the presence of external sources. We also propose the Landau gauge as an alternative to the usual gauge choices given in the standard proofs at the Lagrangian level. CERN-TH/99-373 November 1999 ∗E-mail: [email protected] †E-mail: [email protected] 1 Introduction In supergravity theories [1, 2] the superpartner of the graviton field is a spin 3/2 particle called the gravitino. This particle couples only with gravitational strength to the rest of matter fields, and accordingly its lifetime can be very long, with a decay rate of Γ m3 /M 2 .In 3=2 ' 3=2 P particular, gravitinos lighter than m3=2 < 100 MeV will live longer than the age of the Universe. This fact can have important consequences in cosmology and imposes stringent constraints on supergravity models. Owing to their weak couplings, gravitinos freeze out very early when they 3 are still relativistic; therefore their primordial abundance can be estimated as n3=2/s 10− [3]. -
Doi:10.5281/Zenodo.2566644
Higgs, dark sector and the vacuum: From Nambu-Goldstone bosons to massive particles via the hydrodynamics of a doped vacuum. Marco Fedi * v2, February 16, 2019 Abstract is the energy density of the vacuum, whose units corre- spond to pressure (J=m3 = Pa), hence justifying the re- Here the physical vacuum is treated as a superfluid, fun- pulsive action of dark energy. One can describe the damental quantum scalar field, coinciding with dark en- virtual pairs forming and annihilating in quantum vac- ergy and doped with particle dark matter, able to pro- uum – considered as a fundamental, scalar, quantum duce massive particles and interactions via a hydrody- field – as vortex-antivortex pairs of vacuum’s quanta, namic reinterpretation of the Higgs mechanism. Here via a mechanism analogous to the Higgs mechanism, the Nambu-Goldstone bosons are circularly polarized where phonons in the superfluid vacuum are the Nambu- phonons around the edge of the Brillouin zone of vac- Goldstone bosons, which here trigger quantized vortices uum’s quasi-lattice and they give mass to particles by trig- and the mass-acquisition process, due to the interaction gering quantized vortices, whose dynamics reproduces with diffused particle dark matter [2], which acts as a any possible spin. Doped vortices also exert hydrody- dopant of the superfluid vacuum and that could be the rea- namic forces which may correspond to fundamental in- son for vacuum dilatancy, described and proven in [22]. teractions. Hence, is the Higgs field really something different or along with the dark sector and quantum vacuum we are Keywords— quantum vacuum; dilatant vacuum; dark en- using different names to refer to the same thing? Dilatant ergy; dark matter; Higgs mechanism; spin; fundamental vacuum [22] could refer to the possible apparent viscosity interactions. -
The Symmetries of QCD (And Consequences)
Introduction QCD Lattice Physics Challenges The symmetries of QCD (and consequences) Sinéad M. Ryan Trinity College Dublin antum Universe Symposium, Groningen, March 2018 Understand nature in terms of fundamental building blocks Introduction QCD Lattice Physics Challenges The Rumsfeld Classification “As we know, there are known knowns. There are things we know we know. We also know, there are known unknowns. That is to say we know there are some things we do not know. But there are also unknown unknowns, the ones we don’t know we don’t know.” – Donald Rumsfeld, U.S. Secretary of Defense, Feb. 12, 2002 Introduction QCD Lattice Physics Challenges Some known knowns antum ChromoDynamics - the theory of quarks and gluons Embarassingly successful Precision tests of SM can reveal new physics - more important than ever! Why focus on the 4.6%? QCD is the only experimentally studied strongly-interacting quantum field theory - highlights many subtleties. A paradigm for other strongly-interacting theories in BSM physics. There are still puzzles and surprises in this well-studied arena. Introduction QCD Lattice Physics Challenges What is QCD? A gauge theory for SU(3) colour interactions of quarks and gluons: Color motivated by experimental measurements; not a “measureable” quantum number. Lagrangian invariant under colour transformations. Elementary fields: arks Gluons 8 colour a = 1,..., 3 < colour a = 1,..., 8 (q )a spin 1/2 Dirac fermions Aa α f μ spin 1bosons : avour f = u, d, s, c, b, t 1 L = ¯q i muD m q Ga Ga f γ μ f f μν μν − − 4 with Ga = Aa Aa + gf abcAb Ac μν ∂μ ν ∂ν μ μ ν and − i μD q = μ i + gAa ta q γ μ γ ∂μ μ Generates gluon self-interactions - might expect consequences! Introduction QCD Lattice Physics Challenges Elucidating the effect of the self-interactions: QED vs QCD In QED: coupling runs and bare e is − screened at large distances - reducing Same but dierent for QCD with anti-screening from gluon interactions dominates! Asymptotic freedom Coupling small at high energies - energetic quarks are (almost) free. -
Aspects of Supersymmetry and Its Breaking
1 Aspects of Supersymmetry and its Breaking a b Thomas T. Dumitrescu ∗ and Zohar Komargodski † aDepartment of Physics, Princeton University, Princeton, New Jersey, 08544, USA bSchool of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey, 08540, USA We describe some basic aspects of supersymmetric field theories, emphasizing the structure of various supersym- metry multiplets. In particular, we discuss supercurrents – multiplets which contain the supersymmetry current and the energy-momentum tensor – and explain how they can be used to constrain the dynamics of supersym- metric field theories, supersymmetry breaking, and supergravity. These notes are based on lectures delivered at the Carg´ese Summer School 2010 on “String Theory: Formal Developments and Applications,” and the CERN Winter School 2011 on “Supergravity, Strings, and Gauge Theory.” 1. Supersymmetric Theories In this review we will describe some basic aspects of SUSY field theories, emphasizing the structure 1.1. Supermultiplets and Superfields of various supermultiplets – especially those con- A four-dimensional theory possesses = 1 taining the supersymmetry current. In particu- supersymmetry (SUSY) if it contains Na con- 1 lar, we will show how these supercurrents can be served spin- 2 charge Qα which satisfies the anti- used to study the dynamics of supersymmetric commutation relation field theories, SUSY-breaking, and supergravity. ¯ µ Qα, Qα˙ = 2σαα˙ Pµ . (1) We begin by recalling basic facts about super- { } multiplets and superfields. A set of bosonic and Here Q¯ is the Hermitian conjugate of Q . (We α˙ α fermionic operators B(x) and F (x) fur- will use bars throughout to denote Hermitian con- i i nishes a supermultiplet{O if these} operators{O satisfy} jugation.) Unless otherwise stated, we follow the commutation relations of the schematic form conventions of [1]. -
Goldstone Bosons in a Crystalline Chiral Phase
Goldstone Bosons in a Crystalline Chiral Phase Goldstone Bosonen in einer Kristallinen Chiralen Phase Zur Erlangung des Grades eines Doktors der Naturwissenschaften (Dr. rer. nat.) genehmigte Dissertation von M.Sc. Marco Schramm, Tag der Einreichung: 29.06.2017, Tag der Prüfung: 24.07.2017 Darmstadt 2017 — D 17 1. Gutachten: PD Dr. Michael Buballa 2. Gutachten: Prof. Dr. Jens Braun Fachbereich Physik Institut für Kernphysik NHQ Goldstone Bosons in a Crystalline Chiral Phase Goldstone Bosonen in einer Kristallinen Chiralen Phase Genehmigte Dissertation von M.Sc. Marco Schramm, 1. Gutachten: PD Dr. Michael Buballa 2. Gutachten: Prof. Dr. Jens Braun Tag der Einreichung: 29.06.2017 Tag der Prüfung: 24.07.2017 Darmstadt 2017 — D 17 Bitte zitieren Sie dieses Dokument als: URN: urn:nbn:de:tuda-tuprints-66977 URL: http://tuprints.ulb.tu-darmstadt.de/6697 Dieses Dokument wird bereitgestellt von tuprints, E-Publishing-Service der TU Darmstadt http://tuprints.ulb.tu-darmstadt.de [email protected] Die Veröffentlichung steht unter folgender Creative Commons Lizenz: Namensnennung – Keine kommerzielle Nutzung – Keine Bearbeitung 4.0 International https://creativecommons.org/licenses/by-nc-nd/4.0/ Abstract The phase diagram of strong interaction matter is expected to exhibit a rich structure. Different models have shown, that crystalline phases with a spatially varying chiral condensate can occur in the regime of low temperatures and moderate densities, where they replace the first-order phase transition found for spatially constant order parameters. We investigate this inhomogeneous phase, where in addition to the chiral symmetry, transla- tional and rotational symmetry are broken as well, in a two flavor Nambu–Jona-Lasinio model.