Theories of Baryon and Lepton Number Violation
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Baryogen, a Monte Carlo Generator for Sphaleron-Like Transitions in Proton-Proton Collisions
Prepared for submission to JHEP BaryoGEN, a Monte Carlo Generator for Sphaleron-Like Transitions in Proton-Proton Collisions Cameron Bravo1 and Jay Hauser Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA E-mail: [email protected] Abstract: Sphaleron and instanton solutions of the Standard Model provide violation of baryon and lepton numbers and could lead to spectacular events at the LHC or future colliders. Certain models of new physics can also lead to sphaleron-like vacuum transitions. This nonperturbative physics could be relevant to the generation of the matter-antimatter asymmetry of the universe. We have developed BaryoGEN, an event generator that facili- tates the exploration of sphaleron-like transitions in proton-proton collisions with minimal assumptions. BaryoGEN outputs standard Les Houches Event files that can be processed by PYTHIA, and the code is publicly available. We also discuss various approaches to experimental searches for such transitions in proton-proton collisions. arXiv:1805.02786v3 [hep-ph] 21 Jul 2018 1Corresponding author. Contents 1 Introduction1 2 Physics Content2 2.1 Fermionic Content of Transitions2 2.2 Incoming Partons and Cancellations3 2.3 Color Flow5 2.4 Simulation Results6 3 Using the Generator6 4 Conclusions8 1 Introduction The class of solutions of gauge field theories to which the sphaleron belongs were first proposed in 1976 by ’t Hooft [1]. These solutions are nonperturbative, so the cross-sections for processes mediated by the sphaleron cannot be calculated perturbatively, e.g. by using Feynman diagrams. The solutions are high-energy but are unstable and decay immediately. The electroweak (EW) sphaleron was first described in 1984 [2]. -
Neutrino CPV Phase and Leptogenesis
Neutrino CPV phase and Leptogenesis Andrew, Brandon, Erika, Larry, Varuna, Wing The Question How can the CP-violating phase in the neutrino mixing matrix, delta, possibly be related to leptogenesis? Can you make a model where this is transparent and has testable predictions? 2 What is it? ● Experiments have observed an asymmetry in the number of baryons versus anti-baryons in the universe ● Leptogenesis – The process of generating baryogenesis through lepton asymmetry ● This lepton asymmetry is converted into a baryon asymmetry by the sphaleron process ● Leptogenesis is a mechanism that attempts to explain the observed asymmetry – Many different models of Leptogenesis exist – We only consider Leptogenesis with Type I Seesaw 3 Sakharov Conditions Three conditions for dynamically generated baryon asymmetry: I. Baryon (and lepton) Number Violation II. C and CP Symmetry Violation III. Interactions out of Thermal Equilibrium 4 Seesaw Mechanism ● Introduce three right-handed heavy neutrinos, NRi with the following Lagrangian: ● The Majorana mass matrix M is diagonal, the Yukawa matrix may be complex, and the Higgs will give a Majorana mass term to the neutrinos after symmetry breaking ● This gives a mass to the light neutrinos: ● For 0.1 eV light neutrinos and taking λ at the GeV scale, that gives a heavy mass scale of 1010 GeV 5 Seesaw Mechanism ● Self energy diagram N showing flavor change at high energy νf νf’ ● The interaction can be described by: H ● Self energy diagram at low energy νf νf’ with the heavy fields integrated out ● Creates an effective point interaction that can be described by: 6 Seesaw Mechanism ● Relating the high and low energy interactions, we can write the following: ● Where R is orthogonal but may be complex (Casas-Ibarra parametrization); it reshuffles and re-phases the flavors. -
Grand Unification and Proton Decay
Grand Unification and Proton Decay Borut Bajc J. Stefan Institute, 1000 Ljubljana, Slovenia 0 Reminder This is written for a series of 4 lectures at ICTP Summer School 2011. The choice of topics and the references are biased. This is not a review on the sub- ject or a correct historical overview. The quotations I mention are incomplete and chosen merely for further reading. There are some good books and reviews on the market. Among others I would mention [1, 2, 3, 4]. 1 Introduction to grand unification Let us first remember some of the shortcomings of the SM: • too many gauge couplings The (MS)SM has 3 gauge interactions described by the corresponding carriers a i Gµ (a = 1 ::: 8) ;Wµ (i = 1 ::: 3) ;Bµ (1) • too many representations It has 5 different matter representations (with a total of 15 Weyl fermions) for each generation Q ; L ; uc ; dc ; ec (2) • too many different Yukawa couplings It has also three types of Ng × Ng (Ng is the number of generations, at the moment believed to be 3) Yukawa matrices 1 c c ∗ c ∗ LY = u YU QH + d YDQH + e YELH + h:c: (3) This notation is highly symbolic. It means actually cT αa b cT αa ∗ cT a ∗ uαkiσ2 (YU )kl Ql abH +dαkiσ2 (YD)kl Ql Ha +ek iσ2 (YE)kl Ll Ha (4) where we denoted by a; b = 1; 2 the SU(2)L indices, by α; β = 1 ::: 3 the SU(3)C indices, by k; l = 1;:::Ng the generation indices, and where iσ2 provides Lorentz invariants between two spinors. -
$\Delta L= 3$ Processes: Proton Decay And
IFIC/18-03 ∆L = 3 processes: Proton decay and LHC Renato M. Fonseca,1, ∗ Martin Hirsch,1, y and Rahul Srivastava1, z 1AHEP Group, Institut de F´ısica Corpuscular { C.S.I.C./Universitat de Val`encia,Parc Cient´ıficde Paterna. C/ Catedr´atico Jos´eBeltr´an,2 E-46980 Paterna (Valencia) - SPAIN We discuss lepton number violation in three units. From an effective field theory point of view, ∆L = 3 processes can only arise from dimension 9 or higher operators. These operators also violate baryon number, hence many of them will induce proton decay. Given the high dimensionality of these operators, in order to have a proton half-life in the observable range, the new physics associated to ∆L = 3 processes should be at a scale as low as 1 TeV. This opens up the possibility of searching for such processes not only in proton decay experiments but also at the LHC. In this work we analyze the relevant d = 9; 11; 13 operators which violate lepton number in three units. We then construct one simple concrete model with interesting low- and high-energy phenomenology. I. INTRODUCTION could be related to some particular combinations of lep- ton/quark flavours, as argued for example in [8], or to The standard model conserves baryon (B) and lepton total lepton and baryon numbers. The possibility we dis- (L) number perturbatively. However, this is no longer cuss in this paper is that lepton number might actually true for non-renormalizable operators [1] which might be be violated only in units of three: ∆L = 3. -
Balancing Asymmetric Dark Matter with Baryon Asymmetry by Sphaleron Transitions †
Proceeding Paper Balancing Asymmetric Dark Matter with Baryon Asymmetry by Sphaleron Transitions † Arnab Chaudhuri 1,* and Maxim Khlopov 2,3,4 1 Department of Physics and Astronomy, Novosibirsk State University, Novosibirsk, 630090 Novosibirsk Oblast, Russia 2 Institute of Physics, Southern Federal University, 344006 Rostov on Don, Russia; [email protected] 3 Astroparticule et Cosmologie, Université de Paris, CNRS, F-75013 Paris, France 4 National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 115409 Moscow, Russia * Correspondence: [email protected] † Presented at the 1st Electronic Conference on Universe, 22–28 February 2021; Available online: https://ecu2021.sciforum.net/. Abstract: The effect of the electroweak sphaleron transition in balance between baryon excess and and the excess of stable quarks of 4th generation is studied in this paper. Considering the non-violation of SU(2) symmetry and the conservation of electroweak and new charges and quantum numbers of the new family, it makes possible sphaleron transitions between baryons, leptons and 4th family of leptons and quarks. In this paper, we have tried to established a possible definite relationship between the value and sign of the 4th family excess relative to baryon asymmetry. If U-type quarks are the lightest quarks of the 4th family and sphaleron transitions provide excessive U¯ antiquarks, asymmetric dark matter in the form of dark atom bound state of (U¯ U¯ U¯ ) with primordial He nuclei is balanced with baryon asymmetry. Keywords: electroweak phase transition; 4th generation; early universe Citation: Chaudhuri, A.; Khlopov, M. Balancing Asymmetric Dark Matter with Baryon Asymmetry by 1. Introduction Sphaleron Transitions. -
Arxiv:1806.08204V2 [Hep-Ph] 7 Nov 2018
DO-TH 18/12 CP3-Origins-2018-022 DNRF90 Scalar Dark Matter, GUT baryogenesis and Radiative neutrino mass Wei-Chih Huang∗ CP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark , Fakult¨atf¨urPhysik, Technische Universit¨atDortmund, 44221 Dortmund, Germany Heinrich P¨asy and Sinan Zeißnerz Fakult¨atf¨urPhysik, Technische Universit¨atDortmund, 44221 Dortmund, Germany Abstract We investigate an interesting correlation among dark matter phenomenology, neutrino mass generation and GUT baryogenesis, based on the scotogenic model. The model contains additional right-handed neutrinos N and a second Higgs doublet Φ, both of which are odd under an imposed Z2 symmetry. The neutral component of Φ, i.e. the lightest of the Z2-odd particles, is the dark matter candidate. Due to a Yukawa coupling involving Φ, N and the Standard Model leptons, the lepton asymmetry is converted into the dark matter asymmetry so that a non-vanishing B L − asymmetry can arise from (B L)-conserving GUT baryogenesis, leading to a nonzero baryon − asymmetry after the sphalerons decouple. On the other hand, Φ can also generate neutrino masses radiatively. In other words, the existence of Φ as the dark matter candidate resuscitates GUT baryogenesis and realizes neutrino masses. arXiv:1806.08204v2 [hep-ph] 7 Nov 2018 ∗Electronic address: [email protected] yElectronic address: [email protected] zElectronic address: [email protected] 1 I. INTRODUCTION The origin of the observed baryon asymmetry can not be accounted for within the Standard Model (SM) and is one of the unresolved issues in particle physics and cosmology. -
Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √S = 13 Tev
Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √s = 13 TeV The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Sirunyan, A. M. et al. “Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √s = 13 TeV.” Journal of High Energy Physics 2018, 11 (November 2018): 42 © 2018 The Author(s) As Published https://doi.org/10.1007/JHEP11(2018)042 Publisher Springer Nature Version Final published version Citable link http://hdl.handle.net/1721.1/119253 Terms of Use Creative Commons Attribution 4.0 International License Detailed Terms http://creativecommons.org/licenses/by/4.0/ Published for SISSA by Springer Received: May 15, 2018 Revised: August 28, 2018 Accepted: October 27, 2018 Published: November 7, 2018 Search for black holes and sphalerons in high-multiplicity final states in proton-proton collisions JHEP11(2018)042 p at s = 13 TeV The CMS collaboration E-mail: [email protected] Abstract: A search in energetic, high-multiplicity final states for evidence of physics beyond the standard model, such as black holes, string balls, and electroweak sphalerons, is presented. The data sample corresponds to an integrated luminosity of 35.9 fb−1 collected with the CMS experiment at the LHC in proton-proton collisions at a center-of-mass energy of 13 TeV in 2016. Standard model backgrounds, dominated by multijet production, are determined from control regions in data without any reliance on simulation. -
Proton Decay at the Drip-Line Magic Number Z = 82, Corresponding to the Closure of a Major Nuclear Shell
NEWS AND VIEWS NUCLEAR PHYSICS-------------------------------- case since it has one proton more than the Proton decay at the drip-line magic number Z = 82, corresponding to the closure of a major nuclear shell. In Philip Woods fact the observed proton decay comes from an excited intruder state configura WHAT determines whether a nuclear ton decay half-life measurements can be tion formed by the promotion of a proton species exists? For nuclear scientists the used to explore nuclear shell structures in from below the Z=82 shell closure. This answer to this poser is that the species this twilight zone of nuclear existence. decay transition was used to provide should live long enough to be identified The proton drip-line sounds an inter unique information on the quantum mix and its properties studied. This still begs esting place to visit. So how do we get ing between normal and intruder state the fundamental scientific question of there? The answer is an old one: fusion. configurations in the daughter nucleus. what the ultimate boundaries to nuclear In this case, the fusion of heavy nuclei Following the serendipitous discovery existence are. Work by Davids et al. 1 at produces highly neutron-deficient com of nuclear proton decay4 from an excited Argonne National Laboratory in the pound nuclei, which rapidly de-excite by state in 1970, and the first example of United States has pinpointed the remotest boiling off particles and gamma-rays, leav ground-state proton decay5 in 1981, there border post to date, with the discovery of ing behind a plethora of highly unstable followed relative lulls in activity. -
Arxiv:Hep-Ph/9603208V2 10 Apr 1996 Ac ,1996 1, March INR-913/96 CERN-TH/96-13 5, No Anni 166, 75Th Volume Sakharov’S Nauk, of Fiz
CERN-TH/96-13 INR-913/96 hep-ph/9603208 March 1, 1996 ELECTROWEAK BARYON NUMBER NON-CONSERVATION IN THE EARLY UNIVERSE AND IN HIGH ENERGY COLLISIONS V. A. Rubakova,1 and M. E. Shaposhnikovb,a,2 a Institute for Nuclear Research of the Russian Academy of Sciences, 60-th October Anniversary Prospect 7a, Moscow 117312, Russia bTheory Division, CERN, CH-1211 Geneva 23, Switzerland Abstract We review recent progress in the study of the anomalous baryon number non-conservation at high temperatures and in high energy collisions. Recent results on high temperature phase transitions are described, and applications to electroweak baryogenesis are considered. The current status of the problem of electroweak instanton-like processes at high energies is outlined. This paper is written on the occasion of Sakharov’s 75th anniversary and will appear in the memorial volume of Uspekhi (Usp. Fiz. Nauk, volume 166, No 5, May 1996). arXiv:hep-ph/9603208v2 10 Apr 1996 CERN-TH/96-13 INR-913/96 March 1, 1996 [email protected] [email protected] Contents 1 Introduction 2 2 Basics of anomalous non-conservation of fermion quantum numbers 4 3 Baryon asymmetry: preliminaries 8 4 Sphaleron rate at finite temperatures 11 4.1 Qualitativediscussion. ...... 11 4.2 TheGreen’sfunctionapproach . ..... 14 4.3 The relation to the “probability flux” formulae . ........... 17 4.4 Quantumversusclassicalrate . ...... 18 4.5 Thesphaleronrateinthebrokenphase . ....... 20 4.6 Real time numerical simulations . ....... 21 4.7 Strongsphalerons................................ ... 23 4.8 Concludingremarks............................... ... 23 5 Phase transitions in gauge theories 24 5.1 Equilibrium approximation . ...... 25 5.2 Simpleestimates ................................ -
The Equation of State and the Sphaleron Rate in the Standard Model
The equation of state and the sphaleron rate in the Standard Model Kari Rummukainen University of Helsinki and Helsinki Institute of Physics D'Onofrio, Rummukainen, Tranberg arXiv:1404.3565 D'Onofrio, Rummukainen, arXiv:1508.07161 Big Bang and the little bangs, CERN 8/2016 K. Rummukainen (Helsinki) SM equation of state 1 / 25 The \Bump" The \bump" has ceased to be (. or is it just resting?) the Standard Model rules (still) K. Rummukainen (Helsinki) SM equation of state 2 / 25 Phase transitions in the Standard Model No phase transitions in the Standard Model (at µ = 0) I QCD and EW \phase transitions" are cross-overs Many BSM models have a first order EW phase transition 7! I EW baryogenesis (Kainulainen) I Gravitational waves (Weir) K. Rummukainen (Helsinki) SM equation of state 3 / 25 In this talk: Precision results of EW: I Pseudocritical temperature I Equation of state - \softness", width of the cross-over I Sphaleron rate Why study these? I it's the Standard. I Background to cosmological applications, e.g. leptogenesis I Precision properties of physics K. Rummukainen (Helsinki) SM equation of state 4 / 25 Phase diagram of the electroweak SM After lots of activity on and off the lattice: > ! No phase transition at all, smooth \cross-over" for mHiggs∼72 GeV 130 symmetric phase 120 [Kajantie,Laine,K.R.,Shaposhnikov,Tsypin 95{98] 110 2nd order endpoint /GeV c T 100 see also 1st order transition [Csikor,Fodor, Heitger] 90 [G¨urtler,Ilgenfritz,Schiller,Strecha] broken Higgs phase 80 50 60 70 80 90 mH/GeV K. Rummukainen (Helsinki) SM equation of state 5 / 25 Overall EOS [Laine, Schr¨oder2006] 0.4 12 10 0.3 8 4 6 p / T w m = 150 GeV 0.2 2 4 H c m = 200 GeV s H 1/3 2 0.1 0 1 2 3 4 5 6 1 2 3 4 5 6 10 10 10 10 10 10 10 10 10 10 10 10 T / MeV T / MeV Perturbation theory + Lattice QCD + Hadron RG Here EW transition featureless K. -
Inclusive Nucleon Decay Searches As a Frontier of Baryon Number Violation
UCI-TR-2019-24 Inclusive Nucleon Decay Searches as a Frontier of Baryon Number Violation Julian Heeck1, ∗ and Volodymyr Takhistov2, y 1Department of Physics and Astronomy, University of California, Irvine Irvine, California, 92697-4575, USA 2Department of Physics and Astronomy, University of California, Los Angeles Los Angeles, California, 90095-1547, USA Proton decay, and the decay of nucleons in general, constitutes one of the most sensitive probes of high-scale physics beyond the Standard Model. Most of the existing nucleon decay searches have focused primarily on two-body decay channels, motivated by Grand Unified Theories and supersymmetry. However, many higher-dimensional operators violating baryon number by one unit, ∆B = 1, induce multi-body nucleon decay channels, which have been only weakly constrained thus far. While direct searches for all such possible channels are desirable, they are highly impractical. In light of this, we argue that inclusive nucleon decay searches, N ! X+anything (where X is a light Standard Model particle with an unknown energy distribution), are particularly valuable, as are model-independent and invisible nucleon decay searches such as n ! invisible. We comment on complementarity and opportunities for such searches in the current as well as upcoming large- scale experiments Super-Kamiokande, Hyper-Kamiokande, JUNO, and DUNE. Similar arguments apply to ∆B > 1 processes, which kinematically allow for even more involved final states and are essentially unexplored experimentally. CONTENTS I. INTRODUCTION I. Introduction 1 Baryon number B and lepton number L are seem- ingly accidentally conserved in the Standard Model (SM), II. Nucleon decay operators 2 which makes searches for their violation extremely impor- A. -
ELEMENTARY PARTICLES in PHYSICS 1 Elementary Particles in Physics S
ELEMENTARY PARTICLES IN PHYSICS 1 Elementary Particles in Physics S. Gasiorowicz and P. Langacker Elementary-particle physics deals with the fundamental constituents of mat- ter and their interactions. In the past several decades an enormous amount of experimental information has been accumulated, and many patterns and sys- tematic features have been observed. Highly successful mathematical theories of the electromagnetic, weak, and strong interactions have been devised and tested. These theories, which are collectively known as the standard model, are almost certainly the correct description of Nature, to first approximation, down to a distance scale 1/1000th the size of the atomic nucleus. There are also spec- ulative but encouraging developments in the attempt to unify these interactions into a simple underlying framework, and even to incorporate quantum gravity in a parameter-free “theory of everything.” In this article we shall attempt to highlight the ways in which information has been organized, and to sketch the outlines of the standard model and its possible extensions. Classification of Particles The particles that have been identified in high-energy experiments fall into dis- tinct classes. There are the leptons (see Electron, Leptons, Neutrino, Muonium), 1 all of which have spin 2 . They may be charged or neutral. The charged lep- tons have electromagnetic as well as weak interactions; the neutral ones only interact weakly. There are three well-defined lepton pairs, the electron (e−) and − the electron neutrino (νe), the muon (µ ) and the muon neutrino (νµ), and the (much heavier) charged lepton, the tau (τ), and its tau neutrino (ντ ). These particles all have antiparticles, in accordance with the predictions of relativistic quantum mechanics (see CPT Theorem).