New Heavy Resonances: from the Electroweak to the Planck Scale
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Searches for Electroweak Production of Supersymmetric Gauginos and Sleptons and R-Parity Violating and Long-Lived Signatures with the ATLAS Detector
Searches for electroweak production of supersymmetric gauginos and sleptons and R-parity violating and long-lived signatures with the ATLAS detector Ruo yu Shang University of Illinois at Urbana-Champaign (for the ATLAS collaboration) Supersymmetry (SUSY) • Standard model does not answer: What is dark matter? Why is the mass of Higgs not at Planck scale? • SUSY states the existence of the super partners whose spin differing by 1/2. • A solution to cancel the quantum corrections and restore the Higgs mass. • Also provides a potential candidate to dark matter with a stable WIMP! 2 Search for SUSY at LHC squark gluino 1. Gluino, stop, higgsino are the most important ones to the problem of Higgs mass. 2. Standard search for gluino/squark (top- right plots) usually includes • large jet multiplicity • missing energy ɆT carried away by lightest SUSY particle (LSP) • See next talk by Dr. Vakhtang TSISKARIDZE. 3. Dozens of analyses have extensively excluded gluino mass up to ~2 TeV. Still no sign of SUSY. 4. What are we missing? 3 This talk • Alternative searches to probe supersymmetry. 1. Search for electroweak SUSY 2. Search for R-parity violating SUSY. 3. Search for long-lived particles. 4 Search for electroweak SUSY Look for strong interaction 1. Perhaps gluino mass is beyond LHC energy scale. gluino ↓ 2. Let’s try to find gauginos! multi-jets 3. For electroweak productions we look for Look for electroweak interaction • leptons (e/μ/τ) from chargino/neutralino decay. EW gaugino • ɆT carried away by LSP. ↓ multi-leptons 5 https://cds.cern.ch/record/2267406 Neutralino/chargino via WZ decay 2� 3� 2� SR ɆT [GeV] • Models assume gauginos decay to W/Z + LSP. -
The Nobel Prize in Physics 1999
The Nobel Prize in Physics 1999 The last Nobel Prize of the Millenium in Physics has been awarded jointly to Professor Gerardus ’t Hooft of the University of Utrecht in Holland and his thesis advisor Professor Emeritus Martinus J.G. Veltman of Holland. According to the Academy’s citation, the Nobel Prize has been awarded for ’elucidating the quantum structure of electroweak interaction in Physics’. It further goes on to say that they have placed particle physics theory on a firmer mathematical foundation. In this short note, we will try to understand both these aspects of the award. The work for which they have been awarded the Nobel Prize was done in 1971. However, the precise predictions of properties of particles that were made possible as a result of their work, were tested to a very high degree of accuracy only in this last decade. To understand the full significance of this Nobel Prize, we will have to summarise briefly the developement of our current theoretical framework about the basic constituents of matter and the forces which hold them together. In fact the path can be partially traced in a chain of Nobel prizes starting from one in 1965 to S. Tomonaga, J. Schwinger and R. Feynman, to the one to S.L. Glashow, A. Salam and S. Weinberg in 1979, and then to C. Rubia and Simon van der Meer in 1984 ending with the current one. In the article on ‘Search for a final theory of matter’ in this issue, Prof. Ashoke Sen has described the ‘Standard Model (SM)’ of particle physics, wherein he has listed all the elementary particles according to the SM. -
Cosmological Relaxation of the Electroweak Scale
Selected for a Viewpoint in Physics week ending PRL 115, 221801 (2015) PHYSICAL REVIEW LETTERS 27 NOVEMBER 2015 Cosmological Relaxation of the Electroweak Scale Peter W. Graham,1 David E. Kaplan,1,2,3,4 and Surjeet Rajendran3 1Stanford Institute for Theoretical Physics, Department of Physics, Stanford University, Stanford, California 94305, USA 2Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA 3Berkeley Center for Theoretical Physics, Department of Physics, University of California, Berkeley, California 94720, USA 4Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa 277-8583, Japan (Received 22 June 2015; published 23 November 2015) A new class of solutions to the electroweak hierarchy problem is presented that does not require either weak-scale dynamics or anthropics. Dynamical evolution during the early Universe drives the Higgs boson mass to a value much smaller than the cutoff. The simplest model has the particle content of the standard model plus a QCD axion and an inflation sector. The highest cutoff achieved in any technically natural model is 108 GeV. DOI: 10.1103/PhysRevLett.115.221801 PACS numbers: 12.60.Fr Introduction.—In the 1970s, Wilson [1] had discovered Our models only make the weak scale technically natural that a fine-tuning seemed to be required of any field theory [9], and we have not yet attempted to UV complete them which completed the standard model Higgs sector, unless for a fully natural theory, though there are promising its new dynamics appeared at the scale of the Higgs mass. -
10. Electroweak Model and Constraints on New Physics
1 10. Electroweak Model and Constraints on New Physics 10. Electroweak Model and Constraints on New Physics Revised March 2020 by J. Erler (IF-UNAM; U. of Mainz) and A. Freitas (Pittsburg U.). 10.1 Introduction ....................................... 1 10.2 Renormalization and radiative corrections....................... 3 10.2.1 The Fermi constant ................................ 3 10.2.2 The electromagnetic coupling........................... 3 10.2.3 Quark masses.................................... 5 10.2.4 The weak mixing angle .............................. 6 10.2.5 Radiative corrections................................ 8 10.3 Low energy electroweak observables .......................... 9 10.3.1 Neutrino scattering................................. 9 10.3.2 Parity violating lepton scattering......................... 12 10.3.3 Atomic parity violation .............................. 13 10.4 Precision flavor physics ................................. 15 10.4.1 The τ lifetime.................................... 15 10.4.2 The muon anomalous magnetic moment..................... 17 10.5 Physics of the massive electroweak bosons....................... 18 10.5.1 Electroweak physics off the Z pole........................ 19 10.5.2 Z pole physics ................................... 21 10.5.3 W and Z decays .................................. 25 10.6 Global fit results..................................... 26 10.7 Constraints on new physics............................... 30 10.1 Introduction The standard model of the electroweak interactions (SM) [1–4] is based on the gauge group i SU(2)×U(1), with gauge bosons Wµ, i = 1, 2, 3, and Bµ for the SU(2) and U(1) factors, respectively, and the corresponding gauge coupling constants g and g0. The left-handed fermion fields of the th νi ui 0 P i fermion family transform as doublets Ψi = − and d0 under SU(2), where d ≡ Vij dj, `i i i j and V is the Cabibbo-Kobayashi-Maskawa mixing [5,6] matrix1. -
Structure of Matter
STRUCTURE OF MATTER Discoveries and Mysteries Part 2 Rolf Landua CERN Particles Fields Electromagnetic Weak Strong 1895 - e Brownian Radio- 190 Photon motion activity 1 1905 0 Atom 191 Special relativity 0 Nucleus Quantum mechanics 192 p+ Wave / particle 0 Fermions / Bosons 193 Spin + n Fermi Beta- e Yukawa Antimatter Decay 0 π 194 μ - exchange 0 π 195 P, C, CP τ- QED violation p- 0 Particle zoo 196 νe W bosons Higgs 2 0 u d s EW unification νμ 197 GUT QCD c Colour 1975 0 τ- STANDARD MODEL SUSY 198 b ντ Superstrings g 0 W Z 199 3 generations 0 t 2000 ν mass 201 0 WEAK INTERACTION p n Electron (“Beta”) Z Z+1 Henri Becquerel (1900): Beta-radiation = electrons Two-body reaction? But electron energy/momentum is continuous: two-body two-body momentum energy W. Pauli (1930) postulate: - there is a third particle involved + + - neutral - very small or zero mass p n e 휈 - “Neutrino” (Fermi) FERMI THEORY (1934) p n Point-like interaction e 휈 Enrico Fermi W = Overlap of the four wave functions x Universal constant G -5 2 G ~ 10 / M p = “Fermi constant” FERMI: PREDICTION ABOUT NEUTRINO INTERACTIONS p n E = 1 MeV: σ = 10-43 cm2 휈 e (Range: 1020 cm ~ 100 l.yr) time Reines, Cowan (1956): Neutrino ‘beam’ from reactor Reactions prove existence of neutrinos and then ….. THE PREDICTION FAILED !! σ ‘Unitarity limit’ > 100 % probability E2 ~ 300 GeV GLASGOW REFORMULATES FERMI THEORY (1958) p n S. Glashow W(eak) boson Very short range interaction e 휈 If mass of W boson ~ 100 GeV : theory o.k. -
Lepton Flavor at the Electroweak Scale
Lepton flavor at the electroweak scale: A complete A4 model Martin Holthausen1(a), Manfred Lindner2(a) and Michael A. Schmidt3(b) (a) Max-Planck Institut f¨urKernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany (b) ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Melbourne, Victoria 3010, Australia Abstract Apparent regularities in fermion masses and mixings are often associated with physics at a high flavor scale, especially in the context of discrete flavor symmetries. One of the main reasons for that is that the correct vacuum alignment requires usually some high scale mechanism to be phenomenologically acceptable. Contrary to this expectation, we present in this paper a renormalizable radiative neutrino mass model with an A4 flavor symmetry in the lepton sector, which is broken at the electroweak scale. For that we use a novel way to achieve the VEV alignment via an extended symmetry in the flavon potential proposed before by two of the authors. We discuss various phenomenological consequences for the lepton sector and show how the remnants of the flavor symmetry suppress large lepton flavor violating processes. The model naturally includes a dark matter candidate, whose phenomenology we outline. Finally, we sketch possible extensions to the quark sector and discuss its implications for the LHC, especially how an enhanced diphoton rate for the resonance at 125 GeV can be explained within this model. arXiv:1211.5143v2 [hep-ph] 5 Feb 2013 [email protected] [email protected] [email protected] 1 Introduction Much progress has been achieved in the field of particle physics during the last year. -
Composite Higgs Models with “The Works”
Composite Higgs models with \the works" James Barnard with Tony Gherghetta, Tirtha Sankar Ray, Andrew Spray and Callum Jones With the recent discovery of the Higgs boson, all elementary particles predicted by the Standard Model have now been observed. But particle physicists remain troubled by several problems. The hierarchy problem Why is the Higgs mass only 126 GeV? Quantum effects naively 16 suggest that mh & 10 GeV would be more natural. Flavour hierarchies Why is the top quark so much heavier than the electron? Dark matter What are the particles that make up most of the matter in the universe? Gauge coupling unification The three gauge couplings in the SM nearly unify, hinting towards a grand unified theory, but they don't quite meet. It feels like we might be missing something. With the recent discovery of the Higgs boson, all elementary particles predicted by the Standard Model have now been observed. However, there is a long history of things that looked like elementary particles turning out not to be Atoms Nuclei Hadrons Splitting the atom Can we really be sure we have reached the end of the line? Perhaps some of the particles in the SM are actually composite. Compositeness in the SM also provides the pieces we are missing The hierarchy problem If the Higgs is composite it is shielded from quantum effects above the compositeness scale. Flavour hierarchies Compositeness in the fermion sector naturally gives mt me . Dark matter Many theories predict other composite states that are stabilised by global symmetries, just like the proton in the SM. -
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. -
ELECTROWEAK PHYSICS Theory for the Experimentalist
ELECTROWEAK PHYSICS Theory for the experimentalist Chris Hays Oxford University CONTENTS Introduction vii 1 The geometry of forces 1 1.1 The fiber bundle of the universe 2 1.2 Spacetime metric 3 1.3 Connections 5 1.4 Curvature 6 1.5 Principle of least action 7 1.6 Conservation laws 9 2 Path integrals and fields 11 2.1 Non-relativistic path integral 12 2.2 Perturbation theory 13 2.2.1 Green’s functions 14 2.3 Path integral of a scalar field 15 2.3.1 Free-field transition amplitude 16 2.3.2 Interacting-field transition amplitude 17 2.4 Path integral of a fermion field 18 2.5 Path integral of a gauge field 19 2.5.1 Free-field generating functional 21 3 The Higgs mechanism 23 iii iv CONTENTS 3.1 Self-interacting scalar field theory 23 3.1.1 Real scalar field 23 3.1.2 Complex scalar field 24 3.2 Gauged scalar field theory 25 3.2.1 U(1)-charged scalar field 25 3.2.2 SU(2)-charged scalar field 26 3.2.3 Propagators after symmetry breaking 27 4 The Electroweak theory 29 4.1 The Electroweak Lagrangian 29 4.2 Electroweak symmetry breaking 30 4.2.1 Scalar field Lagrangian 31 4.2.2 Fermion field Lagrangian 33 4.3 Electroweak propagators 34 5 Cross sections and Feynman diagrams 37 5.1 Scattering matrix 37 5.2 Cross sections and lifetimes 38 5.3 Feynman rules 40 6 Scalar renormalization 47 6.1 Renormalized Lagrangian 47 6.2 Regularization 49 6.2.1 Propagator loop corrections 49 6.2.2 Vertex loop correction 50 6.3 The renormalization group 51 7 QED renormalization 55 7.1 QED divergences 55 7.2 Fermion self energy 56 7.3 Vacuum polarization 57 7.4 Vertex correction 61 -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
Arxiv:0905.3187V2 [Hep-Ph] 7 Jul 2009 Cie Ataryo Xeietlifrain the Information
Unanswered Questions in the Electroweak Theory Chris Quigg∗ Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, Illinois 60510 USA Institut f¨ur Theoretische Teilchenphysik, Universit¨at Karlsruhe, D-76128 Karlsruhe, Germany Theory Group, Physics Department, CERN, CH-1211 Geneva 23, Switzerland This article is devoted to the status of the electroweak theory on the eve of experimentation at CERN’s Large Hadron Collider. A compact summary of the logic and structure of the electroweak theory precedes an examination of what experimental tests have established so far. The outstanding unconfirmed prediction of the electroweak theory is the existence of the Higgs boson, a weakly interacting spin-zero particle that is the agent of electroweak symmetry breaking, the giver of mass to the weak gauge bosons, the quarks, and the leptons. General arguments imply that the Higgs boson or other new physics is required on the TeV energy scale. Indirect constraints from global analyses of electroweak measurements suggest that the mass of the standard-model Higgs boson is less than 200 GeV. Once its mass is assumed, the properties of the Higgs boson follow from the electroweak theory, and these inform the search for the Higgs boson. Alternative mechanisms for electroweak symmetry breaking are reviewed, and the importance of electroweak symmetry breaking is illuminated by considering a world without a specific mechanism to hide the electroweak symmetry. For all its triumphs, the electroweak theory has many shortcomings. It does not make specific predictions for the masses of the quarks and leptons or for the mixing among different flavors. It leaves unexplained how the Higgs-boson mass could remain below 1 TeV in the face of quantum corrections that tend to lift it toward the Planck scale or a unification scale. -
The Minimal Fermionic Model of Electroweak Baryogenesis
The minimal fermionic model of electroweak baryogenesis Daniel Egana-Ugrinovic C. N. Yang Institute for Theoretical Physics, Stony Brook, NY 11794 Abstract We present the minimal model of electroweak baryogenesis induced by fermions. The model consists of an extension of the Standard Model with one electroweak singlet fermion and one pair of vector like doublet fermions with renormalizable couplings to the Higgs. A strong first order phase transition is radiatively induced by the singlet- doublet fermions, while the origin of the baryon asymmetry is due to asymmetric reflection of the same set of fermions on the expanding electroweak bubble wall. The singlet-doublet fermions are stabilized at the electroweak scale by chiral symmetries and the Higgs potential is stabilized by threshold corrections coming from a multi-TeV ultraviolet completion which does not play any significant role in the phase transition. We work in terms of background symmetry invariants and perform an analytic semi- classical calculation of the baryon asymmetry, showing that the model may effectively generate the observed baryon asymmetry for percent level values of the unique invari- ant CP violating phase of the singlet-doublet sector. We include a detailed study of electron electric dipole moment and electroweak precision limits, and for one typical benchmark scenario we also recast existing collider constraints, showing that the model arXiv:1707.02306v1 [hep-ph] 7 Jul 2017 is consistent with all current experimental data. We point out that fermion induced electroweak baryogenesis has irreducible phenomenology at the 13 TeV LHC since the new fermions must be at the electroweak scale, have electroweak quantum numbers and couple strongly with the Higgs.