DOCSLIB.ORG

Neutrino Physics: Experiments

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Neutrino Physics: Experiments Neutrino physics: experiments The dark side of the Universe, ISAPP, MPIK Heidelberg, May 29/30, 2019 ν νe µ Christian Weinheimer Institut für Kernphysik, Westfälische Wilhelms-Universität Münster weinheimer@uni-muenster.de ν τ A reminder: Neutrinos in the Standard Model of Particle Physics Prof. Dr. Takaaki Kajita Neutrino oscillations: experiments with atmospheric, solar, accelerator and reactor neutrinos Neutrino masses: - cosmology and astrophysics - neutrinoless double β decay - direct neutrino mass experiments Search for sterile neutrinos Coherent neutrino nucleus elastic scattering Prof. Dr. Arthur B. McDonald Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 1 Experimental proof n of neutrinos ν e p e+ 1956: Cowan and Reines: Poltergeist experiment strong νe source: nuclear power reactor: 6 fission (from fission products), E 9 MeV νe ν energy gain / fission: 200 MeV 1 GW thermal power 2 1020 ν/s + Detection reaction: inverse β decay: νe + p n + e (threshold: 1.8 MeV) Signature:a) n: thermalisation by elastic scattering, capture on Cd γ 's b) e+: annihilation 2 γ 's (511 keV) spatial and time-delayed coincidence (nearly background free) measured cross section: (1.1 ± 0.3) 10-43 cm2 figure: Schmitz: Neutrinophysics, Teubner (in good agreement with Fermi`s theory for V-A) Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 2 ν's in the electroweak Standard Model: U(1)SU(2) 12 fundamental fermions 6 left-handed weak isospin dublets: pure weak isospin dublets weak S. Glashow isospin dublets 9 right-handed weak isospin singulets: (no νR in SM) massive leptons in charged S. Weinberg weak currents (CC): - lepton: For masseless particles (ν in SM): P(H = 1) = (1 -v/c))/2 P = -v/c σ Long c ΨL , ΨR have helicity H = -1 p - anti lepton: P(H = 1) = (1 v/c)/2 σ P = v/c A. Salam c p Long ΨR , ΨL have helicity H = +1 Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 3 Lagrangian: Interaction part l (d) ν (u) W + W - ν (u) l (d) weak charged current (CC) ν,l, u,d, .. Z 0 ν,l, u,d, .. weak neutral current (NC) l, u,d, .. γ l, u,d, .. em neutral current coupling to electromagnetic current e.m. as in QED:g sin = e Jµ θW o θW = 28.7 coupling of weak interaction coupling of em. interaction, 2“ 2 but there is a term „mW (mZ ) in the denominator of the propagator, see later Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 4 Weakness of weak interaction Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 5 ν cross sections σ s figure: Schmitz: Neutrinophysics, Teubner -fermion scattering cross sections: s = m 2 + 2E m s E ν σ f ν f ν Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 6 LEP: determination of number of neutrino generations LEP: e- + e+ Z0 (γ) e- + e+, µ- + µ+, τ-+ τ+, e l u + u, b i s i d + d, v s + s, c + c, b + b, νe + νe, e l ν + ν , b µ µ i s i + , v ντ ντ n ???? i figure: PDG Exp: full width: Γ = 2495(2) MeV invisible width: Γinvisible = 499(2) MeV partial width = 167.1 MeV N = 2.99 ν Γν ν Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 7 Angular distribution of neutrino-fermion scattering Neutrino-fermion scattering: no angular dependence: y distribution is flat for νl scattering ! Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 8 Angular distribution of antineutrino-fermion scattering Antineutrino-fermion scattering (neglect NC): angular dependence: distribution y distribution is not flat for νl scattering ! Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 9 Christian Weinheimer Christian distributionand y the for for helicitydeducearguements we From Experiment Sea quarkSea fraction expect: expect: ν Average: Average: q = q : ν q with with and but q ν (x) in nucleon is about nucleon 15% is in (x) q = q and (anti)neutrino-nucleon scattering σ ν tot q : ISAPP Heidelberg May 29/30, 2019 May 29/30, Heidelberg ISAPP Deep inelastic inelastic Deep 10 figures: Perkins: Introduction to High Energy Physics, Cambridge Neutrino sources and energy spectra figure: Schmitz: Neutrinophysics, Teubner Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 11 Summary of neutrinos in the Standard Model of particle physics ● ν's are left-handed, charged fermions in CC reactions (W exchange) are also left-handed charged fermion coupling to the Z0 is more complicated (since the Z0 is a superposition of the „hypercharge photon B“ and the W3) ● ν's are massless, since there is no right-handed neutrino to construct a „Dirac mass term“ = - m ΨL ΨR – m ΨR ΨL L ● ν's have very small cross section (due to the large masses of W and Z) Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 12 Neutrino physics: experiments The dark side of the Universe, ISAPP, MPIK Heidelberg, May 29/30, 2019 ν νe µ Christian Weinheimer Institut für Kernphysik, Westfälische Wilhelms-Universität Münster weinheimer@uni-muenster.de ν τ A reminder: Neutrinos in the Standard Model of Particle Physics Prof. Dr. Takaaki Kajita Neutrino oscillations: experiments with atmospheric, solar, accelerator and reactor neutrinos Neutrino masses: - cosmology and astrophysics - neutrinoless double β decay - direct neutrino mass experiments Search for sterile neutrinos Coherent neutrino nucleus elastic scattering Prof. Dr. Arthur B. McDonald Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 13 Atmospheric neutrino anomaly: too few muon neutrinos Interaction of cosmic rays (p,α, ..) in outer atmosphere: π, K,... + + + π µ νµ + e + νµ + νe - - + π µ νµ e- + + νµ νe + / 2 νµ νµ νe νe n o i t a t c e ν e p x e e ν / t / n µ e ν + m i µ r ν e p x e Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 14 Kamioka Nucleon Decay Experiment: KamiokaNDE (II) 3000 t water Cherenov detector to search for proton decay (→ GUT) 16m high, 16m diameter 1000 38cm PMTs at the surface If a charged particle moves faster than speed of light in the medium, polarisation does not follow: → Emission of Cherenkov-light into a cone: cosθ = 1/βn o (→ 42 for H20 assuming β=v/c → 1) → ring structure at wall covered by PMTs Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 15 Atmospheric neutrinos in a water Cherenkov detector Cherenkov cone gives: ● energy ● direction (-) ν ● electron/muon differentiation: muons: sharp ring l+/- electrons: washed-out ring (multiple scattering, em shower) (Super-)Kamiokande Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 16 Physics results of KamiokaNDE II No observation of proton decay → main mission failed but KamiokaNDE II performed extremely well, e.g. - Discovery (together with IMB) of neutrinos from SN1987a → Nobel prize 2002 to Masatoshi Koshiba - confirmation of nuclear burning in the sun by observing solar neutrinos - atmospheric neutrino anomaly: wrong muon neutrinos/electron neutrino ratio & wrong angular distribution Y. Fukuda et al., Phys. Lett. B 335 (1994) 237 → decision to build Super-Kamiokande Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 17 Super-Kamiokande: Start of data taking in April 1996 water Cherenkov detector H20: 50 000 t 40 m high, 40 m 11146 PMTs a 50 cm 1 km overburden in Kamioka Mine, Japan Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 18 Super-Kamiokande's first result at Int. Conf. Neutrino 1998 at Takayama Nobel prize 2015 to Takaaki Kajita Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 19 Angular distribution of and at SK νe νµ θ ν p, α, .. L Expectation no neutrino oscillation Fit νµ → ντ Oszillation R. Wendell – Neutrino 2014 Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 20 Angular distribution of and at SK νe νµ Clear deficit of muon neutrinos coming from below, θ (i.e. muon neutrino which travelled a long distance) ν p, α, .. Measurement is compatible to neutrino oscillation: L (detector is nearly blind for ν ) νµ ντ τ „Neutrino oscillation“ with parameters (Δm2 2 ×10-3 eV2. sin2(2θ) 1) Expectation no neutrino oscillation Fit νµ → ντ Oszillation R. Wendell – Neutrino 2014 Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 21 Angular distribution of and at SK νe νµ All data sets and analyses (FC, PC, up-going θ µ, NC enhanced): ν compatible with p, α, .. ν ν oscillation L µ τ (Δm2 2 ×10-3 eV2. sin2(2θ) 1) Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 22 Angular distribution of and at SK νe νµ θ Question to think about: ν What is the connection of the expected multi-GeV p, α, .. angular distributions of atmospheric neutrinos L with the red sky at sun rise or sun set ? Expectation no neutrino oscillation Fit νµ → ντ Oszillation R. Wendell – Neutrino 2014 Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 23 Neutrino (vacuum) oscillations 1) non-trivial unitary ν mixing matrix U between neutrino flavour states ( ) and mass states ( ): νe νµ ντ ν1 ν2 ν3 d d g s mixin d 3 state 2) a flavour state propagates as a coherent sum of mass states m(νi) if the m(νi) differ neutrino oscillation ν U 1 U * - + µ1 τ1 ντ τ nt + µ ν perime W U 2 U * slit ex µ2 τ2 Triple ν ν + µ U 3 U * W µ3 τ3 creation of a detection of a νµ propagation as coherent ντ via weak interaction superposition of mass states via weak interaction Formula is correct, P but correct derivation (να νβ) needs wave packages or QFT (see E. Akhmedov) Christian Weinheimer ISAPP Heidelberg May 29/30, 2019 24 Neutrino (vacuum) oscillations 2 Flavor case: Probability for an oscillation sin2(2 ) from to (and back) for Θ να νβ an amplitude value of 2 average E/L sin (2θ) = 0.2 in units of the y oscillation length L .
Load more

Recommended publications
  • Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond Alessandra Edda Baas University of Massachusetts Amherst
    University of Massachusetts Amherst ScholarWorks@UMass Amherst Masters Theses 1911 - February 2014 2010 Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond Alessandra Edda Baas University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.umass.edu/theses Part of the Physics Commons Baas, Alessandra Edda, "Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond" (2010). Masters Theses 1911 - February 2014. 503. Retrieved from https://scholarworks.umass.edu/theses/503 This thesis is brought to you for free and open access by ScholarWorks@UMass Amherst. It has been accepted for inclusion in Masters Theses 1911 - February 2014 by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact scholarworks@library.umass.edu. THEORETICAL AND EXPERIMENTAL ASPECTS OF THE HIGGS MECHANISM IN THE STANDARD MODEL AND BEYOND A Thesis Presented by ALESSANDRA EDDA BAAS Submitted to the Graduate School of the University of Massachusetts Amherst in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE September 2010 Department of Physics © Copyright by Alessandra Edda Baas 2010 All Rights Reserved THEORETICAL AND EXPERIMENTAL ASPECTS OF THE HIGGS MECHANISM IN THE STANDARD MODEL AND BEYOND A Thesis Presented by ALESSANDRA EDDA BAAS Approved as to style and content by: Eugene Golowich, Chair Benjamin Brau, Member Donald Candela, Department Chair Department of Physics To my loving parents. ACKNOWLEDGMENTS Writing a Thesis is never possible without the help of many people. The greatest gratitude goes to my supervisor, Prof. Eugene Golowich who gave my the opportunity of working with him this year.
    [Show full text]
  • Physics at the Tevatron
    Top Physics at Hadron Colliders Sandra Leone INFN Pisa Gottingen HASCO School 2018 1 Outline . Motivations for studying top . A brief history t . Top production and decay b ucds . Identification of final states . Cross section measurements . Mass determination . Single top production . Study of top properties 2 Motivations for Studying Top . Only known fermion with a mass at the natural electroweak scale. Similar mass to tungsten atomic # 74, 35 times heavier than b quark. Why is Top so heavy? Is top involved in EWSB? -1/2 (Does (2 2 GF) Mtop mean anything?) Special role in precision electroweak physics? Is top, or the third generation, special? . New physics BSM may appear in production (e.g. topcolor) or in decay (e.g. Charged Higgs). b t ucds 3 Pre-history of the Top quark 1964 Quarks (u,d,s) were postulated by Gell-Mann and Zweig, and discovered in 1968 (in electron – proton scattering using a 20 GeV electron beam from the Stanford Linear Accelerator) 1973: M. Kobayashi and T. Maskawa predict the existence of a third generation of quarks to accommodate the observed violation of CP invariance in K0 decays. 1974: Discovery of the J/ψ and the fourth (GIM) “charm” quark at both BNL and SLAC, and the τ lepton (also at SLAC), with the τ providing major support for a third generation of fermions. 1975: Haim Harari names the quarks of the third generation "top" and "bottom" to match the "up" and "down" quarks of the first generation, reflecting their "spin up" and "spin down" membership in a new weak-isospin doublet that also restores the numerical quark/ lepton symmetry of the current version of the standard model.
    [Show full text]
  • Electro-Weak Interactions
    Electro-weak interactions Marcello Fanti Physics Dept. | University of Milan M. Fanti (Physics Dep., UniMi) Fundamental Interactions 1 / 36 The ElectroWeak model M. Fanti (Physics Dep., UniMi) Fundamental Interactions 2 / 36 Electromagnetic vs weak interaction Electromagnetic interactions mediated by a photon, treat left/right fermions in the same way g M = [¯u (eγµ)u ] − µν [¯u (eγν)u ] 3 1 q2 4 2 1 − γ5 Weak charged interactions only apply to left-handed component: = L 2 Fermi theory (effective low-energy theory): GF µ 5 ν 5 M = p u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 Complete theory with a vector boson W mediator: g 1 − γ5 g g 1 − γ5 p µ µν p ν M = u¯3 γ u1 − 2 2 u¯4 γ u2 2 2 q − MW 2 2 2 g µ 5 ν 5 −−−! u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 2 low q 8 MW p 2 2 g −5 −2 ) GF = | and from weak decays GF = (1:1663787 ± 0:0000006) · 10 GeV 8 MW M. Fanti (Physics Dep., UniMi) Fundamental Interactions 3 / 36 Experimental facts e e Electromagnetic interactions γ Conserves charge along fermion lines ¡ Perfectly left/right symmetric e e Long-range interaction electromagnetic µ ) neutral mass-less mediator field A (the photon, γ) currents eL νL Weak charged current interactions Produces charge variation in the fermions, ∆Q = ±1 W ± Acts only on left-handed component, !! ¡ L u Short-range interaction L dL ) charged massive mediator field (W ±)µ weak charged − − − currents E.g.
    [Show full text]
  • Neutrino Masses-How to Add Them to the Standard Model
    he Oscillating Neutrino The Oscillating Neutrino of spatial coordinates) has the property of interchanging the two states eR and eL. Neutrino Masses What about the neutrino? The right-handed neutrino has never been observed, How to add them to the Standard Model and it is not known whether that particle state and the left-handed antineutrino c exist. In the Standard Model, the field ne , which would create those states, is not Stuart Raby and Richard Slansky included. Instead, the neutrino is associated with only two types of ripples (particle states) and is defined by a single field ne: n annihilates a left-handed electron neutrino n or creates a right-handed he Standard Model includes a set of particles—the quarks and leptons e eL electron antineutrino n . —and their interactions. The quarks and leptons are spin-1/2 particles, or weR fermions. They fall into three families that differ only in the masses of the T The left-handed electron neutrino has fermion number N = +1, and the right- member particles. The origin of those masses is one of the greatest unsolved handed electron antineutrino has fermion number N = 21. This description of the mysteries of particle physics. The greatest success of the Standard Model is the neutrino is not invariant under the parity operation. Parity interchanges left-handed description of the forces of nature in terms of local symmetries. The three families and right-handed particles, but we just said that, in the Standard Model, the right- of quarks and leptons transform identically under these local symmetries, and thus handed neutrino does not exist.
    [Show full text]
  • GRAND UNIFIED THEORIES Paul Langacker Department of Physics
    GRAND UNIFIED THEORIES Paul Langacker Department of Physics, University of Pennsylvania Philadelphia, Pennsylvania, 19104-3859, U.S.A. I. Introduction One of the most exciting advances in particle physics in recent years has been the develcpment of grand unified theories l of the strong, weak, and electro­ magnetic interactions. In this talk I discuss the present status of these theo­ 2 ries and of thei.r observational and experimenta1 implications. In section 11,1 briefly review the standard Su c x SU x U model of the 3 2 l strong and electroweak interactions. Although phenomenologically successful, the standard model leaves many questions unanswered. Some of these questions are ad­ dressed by grand unified theories, which are defined and discussed in Section III. 2 The Georgi-Glashow SU mode1 is described, as are theories based on larger groups 5 such as SOlO' E , or S016. It is emphasized that there are many possible grand 6 unified theories and that it is an experimental problem not onlv to test the basic ideas but to discriminate between models. Therefore, the experimental implications are described in Section IV. The topics discussed include: (a) the predictions for coupling constants, such as 2 sin sw, and for the neutral current strength parameter p. A large class of models involving an Su c x SU x U invariant desert are extremely successful in these 3 2 l predictions, while grand unified theories incorporating a low energy left-right symmetric weak interaction subgroup are most likely ruled out. (b) Predictions for baryon number violating processes, such as proton decay or neutron-antineutnon 3 oscillations.
    [Show full text]
  • Graviweak Unification
    Gravi-Weak Unification Fabrizio Nestia, Roberto Percaccib a Universit`adell’Aquila & INFN, LNGS, I-67010, L’Aquila, Italy b SISSA, via Beirut 4, I-34014 Trieste, Italy INFN, Sezione di Trieste, Italy June 22, 2007 Abstract The coupling of chiral fermions to gravity makes use only of the selfdual SU(2) subalgebra of the (complexified) SO(3, 1) algebra. It is possible to identify the antiselfdual subalgebra with the SU(2)L isospin group that appears in the Standard Model, or with its right-handed counterpart SU(2)R that appears in some extensions. Based on this observation, we describe a form of unification of the gravitational and weak interactions. We also discuss models with fermions of both chiralities, the inclusion strong interactions, and the way in which these unified models of gravitational and gauge interactions avoid conflict with the Coleman-Mandula theorem. 1 Approaches to unification In particle physics, the word “unification” is used in a narrow sense to describe the following situation. One starts with two set of phenomena described by gauge theories with gauge groups G1 and G2. A unified description of the two sets of phenomena is given by a gauge theory with a gauge group G containing G1 and G2 as commuting subgroups. In the symmetric phase of the unified theory, the two sets of phenomena are indistinguishable. The subgroups G1 and G2, and hence the distinction between arXiv:0706.3307v2 [hep-th] 5 Jul 2007 the two sets of phenomena, are selected by the vacuum expectation value (VEV) of an “order parameter”, which is usually a multiplet of scalar fields.
    [Show full text]
  • Field Theory and the Standard Model
    Field theory and the Standard Model W. Buchmüller and C. Lüdeling Deutsches Elektronen-Synchrotron DESY, 22607 Hamburg, Germany Abstract We give a short introduction to the Standard Model and the underlying con- cepts of quantum field theory. 1 Introduction In these lectures we shall give a short introduction to the Standard Model of particle physics with empha- sis on the electroweak theory and the Higgs sector, and we shall also attempt to explain the underlying concepts of quantum field theory. The Standard Model of particle physics has the following key features: – As a theory of elementary particles, it incorporates relativity and quantum mechanics, and therefore it is based on quantum field theory. – Its predictive power rests on the regularization of divergent quantum corrections and the renormal- ization procedure which introduces scale-dependent `running couplings'. – Electromagnetic, weak, strong and also gravitational interactions are all related to local symmetries and described by Abelian and non-Abelian gauge theories. – The masses of all particles are generated by two mechanisms: confinement and spontaneous sym- metry breaking. In the following chapters we shall explain these points one by one. Finally, instead of a summary, we briefly recall the history of `The making of the Standard Model' [1]. From the theoretical perspective, the Standard Model has a simple and elegant structure: it is a chiral gauge theory. Spelling out the details reveals a rich phenomenology which can account for strong and electroweak interactions, confinement and spontaneous symmetry breaking, hadronic and leptonic flavour physics etc. [2, 3]. The study of all these aspects has kept theorists and experimenters busy for three decades.
    [Show full text]
  • Electroweak Unification and the W and Z Bosons
    Particle Physics Dr. Alexander Mitov Handout 13 : Electroweak Unification and the W and Z Bosons Dr. A. Mitov Particle Physics 463 Boson Polarization States « In this handout we are going to consider the decays of W and Z bosons, for this we will need to consider the polarization. Here simply quote results although the justification is given in Appendices I and II « A real (i.e. not virtual) massless spin-1 boson can exist in two transverse polarization states, a massive spin-1 boson also can be longitudinally polarized « Boson wave-functions are written in terms of the polarization four-vector « For a spin-1 boson travelling along the z-axis, the polarization four vectors are: transverse longitudinal transverse Longitudinal polarization isn’t present for on-shell massless particles, the photon can exist in two helicity states (LH and RH circularly polarized light) Dr. A. Mitov Particle Physics 464 W-Boson Decay «To calculate the W-Boson decay rate first consider « Want matrix element for : Incoming W-boson : Out-going electron : Out-going : Vertex factor : Note, no propagator « This can be written in terms of the four-vector scalar product of the W-boson polarization and the weak charged current with Dr. A. Mitov Particle Physics 465 W-Decay : The Lepton Current « First consider the lepton current « Work in Centre-of-Mass frame with « In the ultra-relativistic limit only LH particles and RH anti-particles participate in the weak interaction so Note: Chiral projection operator, “Helicity conservation”, e.g. e.g. see p.131 or p.294 see p.133 or p.295 Dr.
    [Show full text]
  • The Algebra of Grand Unified Theories
    The Algebra of Grand Unified Theories John Baez and John Huerta Department of Mathematics University of California Riverside, CA 92521 USA March 21, 2009 1 Introduction The Standard Model of particle physics is one of the greatest triumphs of physics. This theory is our best attempt to describe all the particles and all the forces of nature... except gravity. It does a great job of fitting exper- iments we can do in the lab. But physicists are dissatisfied with it. There are three main reasons. First, it leaves out gravity: that force is described by Einstein's theory of general relativity, which has not yet been reconciled with the Standard Model. Second, astronomical observations suggest that there may be forms of matter not covered by the Standard Model|most notably, `dark matter'. And third, the Standard Model is complicated and seemingly arbitrary. This goes against the cherished notion that the laws of nature, when deeply understood, are simple and beautiful. For the modern theoretical physicist, looking beyond the Standard Model has been an endeavor both exciting and frustrating. Most modern attempts are based on string theory. There are also other interesting approaches, such as loop quantum gravity and theories based on noncommutative ge- ometry. But back in the mid 1970's, before any of these currently popular approaches came to prominence, physicists pursued a program called `grand unification’. This sought to unify the forces and particles of the Standard Model using the mathematics of Lie groups, Lie algebras, and their repre- sentations. Ideas from this era remain influential, because grand unification is still one of the most fascinating attempts to find order and beauty lurking within the Standard Model.
    [Show full text]
  • Unification in Particle Physics
    Examensarbete 15 hp Juni 2016 Unification in Particle Physics Henrik Jansson Kandidatprogrammet i Fysik Department of Physics and Astronomy Unification in Particle Physics Henrik Jansson A thesis presented for the degree of Bachelor of Science Department of Physics and Astronomy Uppsala University, Sweden June 2016 To my girls Unification in Particle Physics Abstract During the twentieth century, particle physics developed into a cornerstone of modern physics, culminating in the Standard Model. Even though this theory has proved to be of extraordinary power, it is still incomplete in several respects. It is our aim in this bachelor thesis to discuss some possible theories beyond the Standard Model, the main focus being on Grand Unified Theories, while also taking a look at attempts of further unification via discrete family symmetry. At the heart of all these theories lies the concept of local gauge invariance, which is introduced as a fundamental principle, followed by an overview of the Standard Model itself. No theory has so far managed to unify all elementary particles and their interactions, but some interesting features are highlighted. We also give a hint at some possible paths to go in the future in the quest for a unification in particle physics. Sammanfattning Under 1900-talet utvecklades partikelfysiken till en av de fundamentala teorierna inom fysiken, och kom att sammanfattas i den s.k. Standardmodellen. Aven¨ om denna modell r¨ont excep- tionella framg˚angervad g¨allerbeskrivningen av elementarpartiklar och deras v¨axelverkan, ¨ar den fortfarande ofullst¨andigp˚aflera s¨att.Syftet med denna kandidatuppsats ¨aratt diskutera m¨ojligateorier bortom Standardmodellen s˚asomStorf¨orenandeTeorier och diskreta famil- jesymmetrier vars avsikt ¨aratt koppla samman de tre familjerna av fermioner i Standard- modellen.
    [Show full text]
  • Neutrino Physics, Rev
    Neutrino Physics aPaul Langacker1, bJens Erler2, and bEduardo Peinado3 aDepartment of Physics, University of Pennsylvania, Philadelphia, PA 19104, USA bInstituto de F´ısica, Universidad Nacional Aut´onoma de M´exico, 01000 M´exico D.F., M´exico Abstract The theoretical and experimental bases of neutrino mass and mixing are reviewed. A brief chronological evolution of the weak interactions, the electroweak Standard Model, and neutrinos is presented. Dirac and Majorana mass terms are explained as well as models such as the seesaw mechanism. Schemes for two, three and four neutrino mixings are presented. 11th Mexican School of Particles and Fields arXiv:hep-ph/0506257v1 24 Jun 2005 August 2004 1E-mail: pgl@electroweak.hep.upenn.edu 2E-mail: erler@fisica.unam.mx 3E-mail: epeinado@nirvana.fisica.uson.mx Contents 1 The Fermi Theory 1 2 Intermediate Vector Bosons (IVB) and SU(2)W × U(1)Y 3 3 Aspects of the SU(2)W × U(1)Y Theory 4 3.1 TheWeakChargedCurrent .......................... 7 3.2 TheWeakNeutralCurrent. 8 4 Neutrino Preliminaries 9 4.1 WeylSpinors .................................. 10 4.2 ActiveandSterileNeutrinos . ... 10 5 Neutrino Mass Models 11 5.1 FermionMasses................................. 11 5.2 DiracMass ................................... 11 5.3 MajoranaMass ................................. 12 5.4 Mixedmodels .................................. 13 5.5 SpecialCases .................................. 14 5.6 ExtensiontoThreeFamilies . .. 15 5.7 ModelsofNeutrinoMass. .. .. .. 17 6 Laboratory and Astrophysical Constraints on Neutrino Counting and Mass 18 6.1 LaboratoryLimits ............................... 18 6.2 CosmologicalConstraints. ... 19 6.3 NeutrinoOscillations . .. 20 7 Atmospheric Neutrinos 21 8 Solar Neutrinos 22 9 Neutrino Oscillation Patterns 25 9.1 ThreeNeutrinoPatterns . 25 9.2 FourNeutrinoPatterns. 26 10 Conclusions 27 i 1 The Fermi Theory The history of the weak interactions dates back to the discovery of radioactivity by Bec- querel in 1896 [1].
    [Show full text]
  • Electroweak Unification and the W and Z Bosons Prof
    Particle Physics Michaelmas Term 2009 Prof Mark Thomson Handout 13 : Electroweak Unification and the W and Z Bosons Prof. M.A. Thomson Michaelmas 2009 451 Boson Polarization States , In this handout we are going to consider the decays of W and Z bosons, for this we will need to consider the polarization. Here simply quote results although the justification is given in Appendices A and B , A real (i.e. not virtual) massless spin-1 boson can exist in two transverse polarization states, a massive spin-1 boson also can be longitudinally polarized , Boson wave-functions are written in terms of the polarization four-vector , For a spin-1 boson travelling along the z-axis, the polarization four vectors are: transverse longitudinal transverse Longitudinal polarization isn’t present for on-shell massless particles, the photon can exist in two helicity states (LH and RH circularly polarized light) Prof. M.A. Thomson Michaelmas 2009 452 W-Boson Decay ,To calculate the W-Boson decay rate first consider , Want matrix element for : Incoming W-boson : Out-going electron : Out-going : Vertex factor : Note, no propagator , This can be written in terms of the four-vector scalar product of the W-boson polarization and the weak charged current with Prof. M.A. Thomson Michaelmas 2009 453 W-Decay : The Lepton Current , First consider the lepton current , Work in Centre-of-Mass frame with , In the ultra-relativistic limit only LH particles and RH anti-particles participate in the weak interaction so Note: Chiral projection operator, “Helicity conservation”, e.g. e.g. see p.131 or p.294 see p.133 or p.295 Prof.
    [Show full text]