Supersymmetry Signals in Leptonic Decays of W and Z Bosons

Total Page:16

File Type:pdf, Size:1020Kb

Supersymmetry Signals in Leptonic Decays of W and Z Bosons PHYSICAL REVIEW D VOLUME 35, NUMBER 3 1 FEBRUARY 1987 Supersymmetry signals in leptonic decays of 8' and Z bosons R. Arnowitt Department of Physics, Northeastern University, Boston, Massachusetts 02115 and Lyman Laboratory of Physics, Harvard University, Cambridge, Massachusetts 02138 Pran Nath Department of Physics, Northeastern University, Boston, Massachusetts 02115 (Received 16 July 1986) It is shown that opposite-sign dilepton events from Z decay represent an excellent signal for su- persymmetry if mrr(Mz/2 in certain kinematic domains where the standard-model background from Z z+r is absent. Excess of monoleptonic events from W 8'y consistent with UA1 cuts is also computed. Comparison with existing data is made. I. INTRODUCTION II. DILEPTON DISTRIBUTIONS Supergravity unified models' are of interest phenome- In calculating the dilepton distributions of Eq. (2) we nologically in that they predict the existence of a number approximately model the UA1 cuts for lepton detection. of low-lying superparticles accessible to present accelera- These include the "kinematic" requirements on the elec- tors or accelerators that will be on line in the near future. tron and muon transverse energy p, „, One of the strongest predictions of supergravity models which possess a light photino (y) is the existence of a W p, )15GeV, ~ri, ~ =2.5, (3a) below W' and a ly- gaugino (W) lying the Z gaugino (Z) ' )3G Ve, & p, ln. l (2. (3b) ing below the Z. Thus the vector-boson decays [where ri= —Intan(|)/2) is the pseudorapidity], as well as W~ W+ y, W~ W+Z, (la) various detection efficiencies. In calculating the number of electrons or muons the UA1 cuts, we have Z W+W passing (lb) neglected the energy dependence in decay matrix ele- are feasible provided the W and Z are not too heavy. ments, but have calculated all branching ratios using the rigorous matrix elements of Ref. 1. In this approximation [In addition, models based on renormalization-group — (RG) breaking of SU(2) x U(1) allow for Z Z(3) we may write for the number of e p events from W de- of the result +Z(3) where Z~3~ is a light superpartner of the axion. cays Z, N,„, Previous work has analyzed the hadronic decays N,~~ =Nz, +, -[I (Z WW)/I (Z e+e )] W,Z qqy into quarks and photinos. Those decays give rise to monojet and dijet events at the CERN SppS Col- x2B(W evy)B(W pvy)(P, „ /P„), (4) lider. Our analysis shows that the UA1 data does not where +, — is the number Z e+e events, rule out W masses mg, =-35-45 GeV, and indeed we find Nz, ' B(W Ivy) = —, is the branching ratio for W leptonic de- models in this mass range with Higgs-boson mixing angles ' + aH 45 consistent with the current UA1 data. cay, P,„ is the fraction of e p pairs from W decay In this Rapid Communication we study the effect of the passing the UA1 cuts, and P„ the fraction of e+e pairs from Z e+e the cuts. [Similar expres- leptonic decays of the W's, W l+ vI+ y. Equation decay passing (lb) then leads to the decays sions hold for the other processes of Eq. (2).] Since in the W leptonic decay the W energy (1Mz/2) is shared between it +PT P P +IIT e e +ItT (2) three particles, one qualitatively expects less than half the electrons to pass the UA I cuts of Eq. (3a), i e., where is the missing transverse energy from the escap- pr — ing v and y. The Z e p channel makes a striking signal for supersymmetry as it is expected to be hadroni- TABLE I. Number of dilepton events arising from Z WW relative to the number of Z e+e events as a function of the cally quiet. The only standard-model background for W mass m~. these decays is Z z+z followed by leptonic decays of the z' s. However~ as discussed below, certain kinematic — z+z domains of e p are forbidden to decays, and so (Gev) f.u even a single event outside the regions forbidden to the z 35 0.072 0.023 0.011 would be evidence for decay of a heavy object such as the 40 0.057 0.019 0.0085 W. We also investigate monoleptonic events arising from 45 0.031 0.118 0.0083 Wy. 1085 Oc 1987 The American Physical Society 1086 R. ARNOWI j I' AND PRAN NATH TABLE II. Number of monolepton events arising from W Wy relative to number of W e v events as a function of 3.0- the W mass m~. (GeV) 35 0.025 0.014 2.0- 40 0.022 0.012 45 0.019 0.0092 which will populate the low-energy side of the W Ivi distribution. (The W WZ channel closes for mg, ~ 37 GeV. ) Assuming again a constant matrix element in the phase-space integral over the UA1 cuts, one has, for the 0 number of W induced leptons, -10 -0.6 -0.2 0 0.2 1.0 ZT COS(ge f ) NI =N~-l, lr(w- wy)/r(w- tv) j — &B(W FIG. 1. Number Z p e p'T arising from Z WW as a Ivy)(P( /PI), (6) — 40-GeV function of Zr cos(p, p„) for a W. where PP is the fraction of leptons arising from W decay passing the UA1 cuts, and PI is the corresponding fraction for leptons from W l v decay. Here the effect is suppressed somewhat since in supersymmetry P,„=0.4. This is indeed confirmed in detailed Monte Carlo calculations. N,„ is enhanced, however, due to I (W Wy)/I (W lv)=0.3-0.4 . the fact I (Z WW)/I (Z e+e ) =4. The ratios The ratios =NI /N~ I„are given in Table II. For the f,„=N,„ /Nz—, +, —,etc. , for the three processes of Eq. fI (2) are given in Table I for W masses in the range con- earlier data, N~ „=172and N~ „„=47.One thus ex- sistent with the UA1 monojet data. For the earlier UA1 pects N, =4 events on the low shoulder of the W ev data of 399 nb ', Nz, +, -=18, and so one expects distribution and N„=2 events. Again these numbers about N,„=1.0 events for a 40-GeV W gaugino. (This should double when the more recent data is included. The number should double when the more recent data is in- earlier data can tolerate about +8 events on the low- cluded. ) In contrast, we estimate for the energy side of the W ev distribution, and so at present roughly— standard-model Z r+ r e p +p'T contribution this effect cannot be detected. With the inclusion of the that N,'„' = 0.5. The supersymmetry contribution thus ap- more recent data, however, the effect is on the edge of be- pears to be somewhat larger than that of the standard ing observable. model. Angle and energy distributions allow one to distinguish the z from W contributions to N,„. Thus the light mass of IV. CONCLUSION the z that all the e — events should be almost implies p Opposite-sign dilepton events from Z decay represents back to back in the transverse plane. The distribution of an excellent signal for W s if the W is sufficiently light for events expected for W's as a function of =cos(p, — ZT p„) the Z WW decay channel to be open. Such events are is given in Fig. 1. About one quarter of the W events lies expected to be hadronically quiet. By choosing the kine- in the first bin —1.0 ~ & —0. overlapping the z con- ZT 9, rnatic region, one can effectively veto the standard-model tribution. The region — 9 & & 0 contains about 50% 0. ZT background from Z z+z without significantly reduc- of the events, while the remaining events have ZT & 0. ing the supersymmetric signal. Furthermore, the z', a Thus there is a clear angular separation of W and z events. fourth sequential lepton with mass m, Mz/2, is The energy distribution gives a less clear separation of the ( distinguish- able from the W, as it couples to the Z with 8'and z. Thus for a z decay the maximum lepton energy strength = 20-25% of the W coupling and hence makes is about Mz/2, while a 40-GeV W yields leptons with ener- only a very small contribution to the dilepton events. Thus ~37 GeV. Thus very energetic leptons would arise gy observation of only a few such dilepton events would be only from z's. strong evidence for the decay of a heavy particle such as the W. Supersymmetry models predict about 1 event/400 nb ' at the CERN collider for W masses in the range con- III. MONOLEPTONIC DISTRIBUTION sistent with UA1 monojet data, which is on the edge of ob- The Wy channel of Eq. (la) will produce monoleptonic servability. With the increased luminosity at the collider events through arising from the antiproton accumulator, however, such events should be detectable by UA1. In addition, an ex- W+ y (l + v&+ y) + y, (5) cess of monoleptonic events from W Wy is predicted, SUPERSYMMETRY SIGNALS IN LEPTONIC DECAYS OF W. 1087 consistent with the current accuracy of the UA1 S'~ ev m~ =40 GeV, with correspondingly smaller N„ data. An increase in statistics, however, could make this and N„„. effect also observable. While dilepton events from 8'decays of the Z are barely ACKNOWLEDGMENTS observable at CERN in the current data sample, they should be copiously produced at the Stanford Linear Col- This work was supported by the National Science Foun- lider (SLC) and CERN LEP if 2mg, & Mz.
Recommended publications
  • 1. Discovery of the W and Z Boson 1983 at CERN Spps Accelerator, √S≈540 Gev, UA-1/2 Experiments 1.1 Boson Production in Pp Interactions
    Experimental tests of the Standard Model • Discovery of the W and Z bosons • Precision tests of the Z sector • Precision tests of the W sector • Electro-weak unification at HERA • Radiative corrections and prediction of the top and Higgs mass • Top discovery at the Tevatron • Higgs searches at the LHC 1. Discovery of the W and Z boson 1983 at CERN SppS accelerator, √s≈540 GeV, UA-1/2 experiments 1.1 Boson production in pp interactions − − p , q p ,q u W u Z ˆ ˆ d s ν u s +,q p , q p → → ν + → → + pp W X pp Z ff X σ (σ ) 10 nb W Z Similar to Drell-Yan: (photon instead of W) 1nb = ≈ sˆ xq xq s mit xq 12.0 2 1.0 nb = ≈ = 2 sˆ xq s .0 014 s 65( GeV ) → Cross section is small ! sˆ M 1 10 100 W ,Z 1.2 UA-1 Detector 1.3 Event signature: pp → Z → ff + X + p p − High-energy lepton pair: 2 2 2 m = (p + + p − ) = M Z ≈ MZ 91 GeV → → ν + 1.4 Event signature: pp W X Missing p T vector Undetected ν − ν Missing momentum p p High-energy lepton – Large transverse momentum p t How can the W mass be reconstructed ? W mass measurement In the W rest frame: In the lab system: • = = MW p pν • W system boosted 2 only along z axis T ≤ MW • p • p distribution is conserved 2 T −1 2 dN 2p M 2 Jacobian Peak: T ⋅ W − 2 ~ pT pT MW 4 dN dp T • Trans.
    [Show full text]
  • Supersymmetry: What? Why? When?
    Contemporary Physics, 2000, volume41, number6, pages359± 367 Supersymmetry:what? why? when? GORDON L. KANE This article is acolloquium-level review of the idea of supersymmetry and why so many physicists expect it to soon be amajor discovery in particle physics. Supersymmetry is the hypothesis, for which there is indirect evidence, that the underlying laws of nature are symmetric between matter particles (fermions) such as electrons and quarks, and force particles (bosons) such as photons and gluons. 1. Introduction (B) In addition, there are anumber of questions we The Standard Model of particle physics [1] is aremarkably hope will be answered: successful description of the basic constituents of matter (i) Can the forces of nature be uni® ed and (quarks and leptons), and of the interactions (weak, simpli® ed so wedo not have four indepen- electromagnetic, and strong) that lead to the structure dent ones? and complexity of our world (when combined with gravity). (ii) Why is the symmetry group of the Standard It is afull relativistic quantum ®eld theory. It is now very Model SU(3) ´SU(2) ´U(1)? well tested and established. Many experiments con® rmits (iii) Why are there three families of quarks and predictions and none disagree with them. leptons? Nevertheless, weexpect the Standard Model to be (iv) Why do the quarks and leptons have the extendedÐ not wrong, but extended, much as Maxwell’s masses they do? equation are extended to be apart of the Standard Model. (v) Can wehave aquantum theory of gravity? There are two sorts of reasons why weexpect the Standard (vi) Why is the cosmological constant much Model to be extended.
    [Show full text]
  • Measurement of the W-Boson Mass in Pp Collisions at √ S = 7 Tev
    EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN) Eur. Phys. J. C 78 (2018) 110 CERN-EP-2016-305 DOI: 10.1140/epjc/s10052-017-5475-4 9th November 2018 Measurementp of the W-boson mass in pp collisions at s = 7 TeV with the ATLAS detector The ATLAS Collaboration A measurement of the mass of the W boson is presented based on proton–proton collision data recorded in 2011 at a centre-of-mass energy of 7 TeV with the ATLAS detector at the LHC, and corresponding to 4.6 fb−1 of integrated luminosity. The selected data sample consists of 7:8 × 106 candidates in the W ! µν channel and 5:9 × 106 candidates in the W ! eν channel. The W-boson mass is obtained from template fits to the reconstructed distributions of the charged lepton transverse momentum and of the W boson transverse mass in the electron and muon decay channels, yielding mW = 80370 ± 7 (stat.) ± 11 (exp. syst.) ± 14 (mod. syst.) MeV = 80370 ± 19 MeV; where the first uncertainty is statistical, the second corresponds to the experimental system- atic uncertainty, and the third to the physics-modelling systematic uncertainty. A meas- arXiv:1701.07240v2 [hep-ex] 7 Nov 2018 + − urement of the mass difference between the W and W bosons yields mW+ − mW− = −29 ± 28 MeV. c 2018 CERN for the benefit of the ATLAS Collaboration. Reproduction of this article or parts of it is allowed as specified in the CC-BY-4.0 license. 1 Introduction The Standard Model (SM) of particle physics describes the electroweak interactions as being mediated by the W boson, the Z boson, and the photon, in a gauge theory based on the SU(2)L × U(1)Y symmetry [1– 3].
    [Show full text]
  • Probing Supergravity Grand Unification in the Brookhaven G-2 Experiment
    PHYSICAL REVIEW D VOLUME 53, NUMBER 3 1 FEBRUARY 1996 Probing supergravity grand unification in the Brookhaven 9 - 2 experiment Utpal Chattopadhyay Department of Physics, flovthe&tem University, Boston, Massachusetts 02115 Pran Nath Department of Physics, Northeastern University, Boston, Massachusetts 0211S and Institute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030 (Received 24 July 1995) A quantitative analysis of a, 3 f(g - 2), within the framework of supergravity grand unification and radiative breaking of the electroweak symmetry is given. It is found that a;“sy is dominated by the chiial interference term from the light chargino exchange, and that this terni carries a signature which correlates strongly with the sign of p. Thus as a rule azusy > 0 for fl > 0 and I$“‘~ < 0 for ti < 0 with very few exceptions when tanp N 1. At the quantitative level it is shown that if the ES21 BNL experiment can reach the expected sensitivity of 4 x lo-” and there is a reduction in the hadronic error by a factor of 4 or more, then the experiment will explore a majority of the parameter space in the mo - mg plane in the region mo < 400 GeV, mg < 700 GeV for tanp > 10 assuming the experiment will not discard the standard model result within its 2~ uncertainty limit. For smaller tanp, the SUSY reach of ES21 will still be considerable. Further, if no effect within the 2~ limit of the standard model v&e is seen, then large tanp scenarios will he severely constrained within the current naturalness criterion, i.e , mo, mp < 1 TeV.
    [Show full text]
  • Particle Physics: Problem Sheet 5 Weak, Electroweak and LHC Physics
    2010 — Subatomic: Particle Physics 1 Particle Physics: Problem Sheet 5 Weak, electroweak and LHC Physics 1. Draw a quark level Feynman diagram for the decay K+ → π+π0. This + is a weak decay. K has strange quark number, Ns = −1. The final state has no strange quarks so Ns = 0. The number of strange quarks can only change when a W boson is exchanged. 2. Write down all possible decay modes of the W − boson into quarks and leptons. What is the strength of each of these vertices? Decay Strength − − W → e ν¯e gW − − W → τ ν¯τ gW − − W → µ ν¯µ gW − W → ¯us gW Vus − W → ¯ud gW Vud − W → ¯ub gW Vub − W → ¯cd gW Vcd − W → ¯cs gW Vcs − W → ¯cb gW Vcb − W → ¯t d gW Vtd − W → ¯t s gW Vts − W → ¯t b gW Vtb 3. By drawing the lowest order Feynman diagrams, show that both charged (W ± exchange) and neutral current (Z0 exchange) contribute to neutrino − − electron scattering: νe + e → νe + e . 2010 — Subatomic: Particle Physics 2 Charged current means exchange of the W ± boson, neutral current means exchange of the Z0 boson. Because we can draw both diagrams, whilst obeying all the conservation laws, it means that both are able to happen. When we observe an electron-neutrino scat- tering event we can never tell, on an event-by-event basis, whether the Z-boson or the W -boson was responsilbe. However by measuring the total cross section and comparing with predictions, we can show that both charged and neutral currents are involved.
    [Show full text]
  • The Discovery of the W and Z Particles
    June 16, 2015 15:44 60 Years of CERN Experiments and Discoveries – 9.75in x 6.5in b2114-ch06 page 137 The Discovery of the W and Z Particles Luigi Di Lella1 and Carlo Rubbia2 1Physics Department, University of Pisa, 56127 Pisa, Italy [email protected] 2GSSI (Gran Sasso Science Institute), 67100 L’Aquila, Italy [email protected] This article describes the scientific achievements that led to the discovery of the weak intermediate vector bosons, W± and Z, from the original proposal to modify an existing high-energy proton accelerator into a proton–antiproton collider and its implementation at CERN, to the design, construction and operation of the detectors which provided the first evidence for the production and decay of these two fundamental particles. 1. Introduction The first experimental evidence in favour of a unified description of the weak and electromagnetic interactions was obtained in 1973, with the observation of neutrino interactions resulting in final states which could only be explained by assuming that the interaction was mediated by the exchange of a massive, electrically neutral virtual particle.1 Within the framework of the Standard Model, these observations provided a determination of the weak mixing angle, θw, which, despite its large experimental uncertainty, allowed the first quantitative prediction for the mass values of the weak bosons, W± and Z. The numerical values so obtained ranged from 60 to 80 GeV for the W mass, and from 75 to 92 GeV for the Z mass, too large to be accessible by any accelerator in operation at that time.
    [Show full text]
  • Particles Meet Cosmology and Strings in Boston
    PASCOS 2004 Particles meet cosmology and strings in Boston PASCOS 2004 is the latest in the symposium series that brings together disciplines from the frontier areas of modern physics. Participants at PASCOS 2004 and the Pran Nath Fest, which were held at Northeastern University, Boston. They include Howard Baer - front row sixth from left - then, moving right, Alfred Bartl, Michael Dine, Bruno Zumino, Pran Nath, Steven Weinberg, Paul Frampton, Mariano Quiros, Richard Arnowitt, MaryKGaillard, Peter Nilles and Michael Vaughn (chair, local organizing committee). The Tenth International Symposium on Particles, Strings and Cos­ redshift surveys suggests that the critical matter density of the uni­ mology took place at Northeastern University, Boston, on 16-22 verse is Qm ~ 0.3, direct dynamical measurements combined with August 2004. Two days of the symposium, 18-19 August, were the estimates of the luminosity density indicate Qm = 0.1-0.2. She devoted to the Pran Nath Fest in celebration of the 65th birthday of suggested that the apparent discrepancy may result from variations Matthews University Distinguished Professor Pran Nath. The PASCOS in the dark-matter fraction with mass and scale. She also suggested symposium is the largest interdisciplinary gathering on the interface that gravitational lensing maps combined with large redshift sur­ of the three disciplines of cosmology, particle physics and string veys promise to measure the dark-matter distribution in the uni­ theory, which have become increasingly entwined in recent years. verse. The microwave background can also provide clues to inflation Topics at PASCOS 2004 included the large-scale structure of the in the early universe.
    [Show full text]
  • Particle Physics Handout 8 the Weak Force
    Subatomic Physics: Particle Physics Handout 8 The Weak Force Weak interactions W and Z interactions at low energy Fermi theory Electroweak theory W and Z bosons at high energy 6 6 SELF-INTERASELF-INTERACTIONSCTIONS hhhljkhsdlkh 1 At this point, QCDhhhljkhsdlkhlooks like a stronger version of QED. At this point, QCD looks like a stronger version of QED. This is true up to a point. However, in practice QCD This is true up to a point. However, in practice QCD behaves very differently to QED. The similarities arise from behaves very differently to QED. The similarities arise from QCD Summarythe fact that both involve the exchange of MASSLESS the fact that both involve the exchange of MASSLESS spin-1 bosons. The big difference is that GLUONS carry spin-1 bosons. The big difference is that GLUONS carry colour “cQuarksharge”. and gluons carry QCD: Quantum Gluonscolour are“c theharg e”. colour charge. GLUONS CAN INTERACT WITH OTHER GLUONS: Chromodymanics is the propagatorGLUONS of theCAN INTERACT WITH OTHER GLUONS: quantum description of strong force Gluons self-interact:g g the strong force. g gg g g Only quarks feel the g g g strong force. g gg g 3 GLUON VERTEX 4 GLUON VERTEX 3 GLUON VERTEX 4 GLUON VERTEX Hadrons can be Electromagnetic coupling constant ! decreasesEXAMPLE: Gluon-Gluon Scattering • EXAMPLE: Gluon-GluondescribedScattering as consisting as a charged particles get further apart. of partons: quarks and •Strong coupling constant !S increases as gluons, which interact + + further apart quarks become. + independently+ Quarks and gluons produced in Colour Confinement collisions hadronise: hadrons are energy required to separate produced.
    [Show full text]
  • Supersymmetry and Its Breaking
    Supersymmetry and its breaking Nathan Seiberg IAS The LHC is around the corner 2 What will the LHC find? • We do not know. • Perhaps nothing Is the standard model wrong? • Only the Higgs particle Most boring. Unnatural. Is the Universe Anthropic? • Additional particles without new concepts Unnatural. Is the Universe Anthropic? • Natural Universe – Technicolor (extra dimensions) – Supersymmetry (SUSY) – new fermionic dimensions • Something we have not thought of 3 I view supersymmetry as the most conservative and most conventional possibility. In the rest of this talk we will describe supersymmetry, will motivate this claim, and will discuss some of the recent developments in this field. 4 Three presentations of supersymmetry • Supersymmetry pairs bosons and fermions – integer spin particles and half integer spin particles. • Supersymmetry is an extension of the Poincare symmetry. • Supersymmetry is an extension of space and time. It describes additional dimensions which are intrinsically quantum mechanical (fermionic). 5 Supersymmetry as an extension of the Poincare symmetry • The Poincare symmetry includes four translations . • One way to present supersymmetry is through adding fermionic symmetries which satisfy Note, these are anti-commutation relations – no obvious classical analog. 6 The spectrum • Normally, translations relate a particle at one point to a particle at a nearby point. • Because of the larger symmetry there must be more particles. relates one particle to another. Every particle has a superpartner. • The symmetry pairs bosons and fermions – integer spin particles and half integer spin particles: 7 Supersymmetry as new quantum fermionic dimensions (more abstract) • In addition to the four classical (bosonic) coordinates , we introduce four fermionic coordinates with spin 1/2.
    [Show full text]
  • Susy 2018.Pdf
    New ideas in Model Building Antonio Delgado University of Notre Dame SUSY2018 Barcelona, July 23-27, 2018 Internatonal Conference on Supersymmetry and Unification of Fundamental Interactons 2018 Internatonal Advisory Commitee Local Organising Commitee Ignatos Antoniadis, CERN Kaoru Hagiwara, KEK Martne Bosman, IFAE Lluïsa Mir, IFAE Csaba Balazs, Monash University Tao Han, Pitsburgh University Pilar Casado, UAB/IFAE Andrés Pacheco Pagés, IFAE/PIC Wim de Boer, KIT, Karlsruhe Gordon L. Kane, Michigan State University José Ramón Espinosa, ICREA/IFAE Alex Pomarol, UAB/IFAE Marcela Carena, Fermilab and Chicago University Dimitri Kazakov, JINR, Dubna Enrique Fernández, UAB/IFAE Oriol Pujolàs, IFAE Mirjam Cvetc, Pennsylvania State University Jihn E. Kim, Seoul Natonal University Sebastán Grinstein, ICREA/IFAE Mariano Quirós, IFAE, co-Chair Athanasios Dedes, Ioannina University Pyungwon Ko, KIAS, Seoul Aurelio Juste, ICREA/IFAE Javier Rico, IFAE Keith Dienes, Arizona State University Paul G. Langacker, IAS, Princeton Ilya Korolkov, IFAE Imma Riu, IFAE Herbi Dreiner, University of Bonn Joseph D. Lykken, Fermilab Mario Martnez, ICREA/IFAE, co-Chair Sebastán Grinschpun, IFAE John Ellis, King’s College UK & CERN Rabindra N. Mohapatra, University of Maryland Ramon Miquel, ICREA/IFAE Jonathan L. Feng, UC Irvine Pran Nath, Northeastern University Gian F. Giudice, CERN Apostolos Pilafsis, Manchester University Rohini M Godbole, CHEP, IISc, Bangalore Fernando Quevedo, ICTP Manoranjan Guchait, TIFR, Mumbai Graham G. Ross, University of Oxford John Gunion, UC Davis Sandip Trivedi, TIFR, Mumbai Pre-SUSY School July 17-20, 2018 susy2018.ifae.es Universitat Autònoma de Barcelona Organised by Supported by GOBIERNO MINISTERIO DE ESPAÑA DE ECONOMÍA, INDUSTRIA Y COMPETITIVIDAD Institut de Física d’Altes Energies Epicycles over epicycles Epicycles over epicycles Turtles over turtles • More seriously I am going to give my personal view on the status of Model Building.
    [Show full text]
  • 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).
    [Show full text]
  • Probing Supergravity Unified Theories at the Large Hadron Collider
    PROBING SUPERGRAVITY UNIFIED THEORIES AT THE LARGE HADRON COLLIDER A dissertation presented by Zuowei Liu to The Department of Physics In partial fulfilment of the requirements for the degree of Doctor of Philosophy in the field of arXiv:0808.3157v1 [hep-ph] 22 Aug 2008 Physics Northeastern University Boston, Massachusetts August, 2008 1 c Zuowei Liu, 2008 ALL RIGHTS RESERVED 2 PROBING SUPERGRAVITY UNIFIED THEORIES AT THE LARGE HADRON COLLIDER by Zuowei Liu ABSTRACT OF DISSERTATION Submitted in partial fulfillment of the requirement for the degree of Doctor of Philosophy in Physics in the Graduate School of Arts and Sciences of Northeastern University, August, 2008 3 Abstract The discovery of supersymmetry is one of the major goals of the current exper- iments at the Tevatron and in proposed experiments at the Large Hadron Collider (LHC). However when sparticles are produced the signatures of their production will to a significant degree depend on their hierarchical mass patterns. Here we investigate hierarchical mass patterns for the four lightest sparticles within one of the leading candidate theories - the SUGRA model. Specifically we analyze the hierarchies for the four lightest sparticles for the mSUGRA as well as for a general class of super- gravity unified models including nonuniversalities in the soft breaking sector. It is shown that out of nearly 104 possibilities of sparticle mass hierarchies, only a small number survives the rigorous constraints of radiative electroweak symmetry break- ing, relic density and other experimental constraints. The signature space of these mass patterns at the LHC is investigated using a large set of final states including multi-leptonic states, hadronically decaying τs, tagged b jets and other hadronic jets.
    [Show full text]