Exploring the Nature of the Universe
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Higgs Bosons and Supersymmetry
Higgs bosons and Supersymmetry 1. The Higgs mechanism in the Standard Model | The story so far | The SM Higgs boson at the LHC | Problems with the SM Higgs boson 2. Supersymmetry | Surpassing Poincar´e | Supersymmetry motivations | The MSSM 3. Conclusions & Summary D.J. Miller, Edinburgh, July 2, 2004 page 1 of 25 1. Electroweak Symmetry Breaking in the Standard Model 1. Electroweak Symmetry Breaking in the Standard Model Observation: Weak nuclear force mediated by W and Z bosons • M = 80:423 0:039GeV M = 91:1876 0:0021GeV W Z W couples only to left{handed fermions • Fermions have non-zero masses • Theory: We would like to describe electroweak physics by an SU(2) U(1) gauge theory. L ⊗ Y Left{handed fermions are SU(2) doublets Chiral theory ) right{handed fermions are SU(2) singlets f There are two problems with this, both concerning mass: gauge symmetry massless gauge bosons • SU(2) forbids m)( ¯ + ¯ ) terms massless fermions • L L R R L ) D.J. Miller, Edinburgh, July 2, 2004 page 2 of 25 1. Electroweak Symmetry Breaking in the Standard Model Higgs Mechanism Introduce new SU(2) doublet scalar field (φ) with potential V (φ) = λ φ 4 µ2 φ 2 j j − j j Minimum of the potential is not at zero 1 0 µ2 φ = with v = h i p2 v r λ Electroweak symmetry is broken Interactions with scalar field provide: Gauge boson masses • 1 1 2 2 MW = gv MZ = g + g0 v 2 2q Fermion masses • Y ¯ φ m = Y v=p2 f R L −! f f 4 degrees of freedom., 3 become longitudinal components of W and Z, one left over the Higgs boson D.J. -
1 Standard Model: Successes and Problems
Searching for new particles at the Large Hadron Collider James Hirschauer (Fermi National Accelerator Laboratory) Sambamurti Memorial Lecture : August 7, 2017 Our current theory of the most fundamental laws of physics, known as the standard model (SM), works very well to explain many aspects of nature. Most recently, the Higgs boson, predicted to exist in the late 1960s, was discovered by the CMS and ATLAS collaborations at the Large Hadron Collider at CERN in 2012 [1] marking the first observation of the full spectrum of predicted SM particles. Despite the great success of this theory, there are several aspects of nature for which the SM description is completely lacking or unsatisfactory, including the identity of the astronomically observed dark matter and the mass of newly discovered Higgs boson. These and other apparent limitations of the SM motivate the search for new phenomena beyond the SM either directly at the LHC or indirectly with lower energy, high precision experiments. In these proceedings, the successes and some of the shortcomings of the SM are described, followed by a description of the methods and status of the search for new phenomena at the LHC, with some focus on supersymmetry (SUSY) [2], a specific theory of physics beyond the standard model (BSM). 1 Standard model: successes and problems The standard model of particle physics describes the interactions of fundamental matter particles (quarks and leptons) via the fundamental forces (mediated by the force carrying particles: the photon, gluon, and weak bosons). The Higgs boson, also a fundamental SM particle, plays a central role in the mechanism that determines the masses of the photon and weak bosons, as well as the rest of the standard model particles. -
A Young Physicist's Guide to the Higgs Boson
A Young Physicist’s Guide to the Higgs Boson Tel Aviv University Future Scientists – CERN Tour Presented by Stephen Sekula Associate Professor of Experimental Particle Physics SMU, Dallas, TX Programme ● You have a problem in your theory: (why do you need the Higgs Particle?) ● How to Make a Higgs Particle (One-at-a-Time) ● How to See a Higgs Particle (Without fooling yourself too much) ● A View from the Shadows: What are the New Questions? (An Epilogue) Stephen J. Sekula - SMU 2/44 You Have a Problem in Your Theory Credit for the ideas/example in this section goes to Prof. Daniel Stolarski (Carleton University) The Usual Explanation Usual Statement: “You need the Higgs Particle to explain mass.” 2 F=ma F=G m1 m2 /r Most of the mass of matter lies in the nucleus of the atom, and most of the mass of the nucleus arises from “binding energy” - the strength of the force that holds particles together to form nuclei imparts mass-energy to the nucleus (ala E = mc2). Corrected Statement: “You need the Higgs Particle to explain fundamental mass.” (e.g. the electron’s mass) E2=m2 c4+ p2 c2→( p=0)→ E=mc2 Stephen J. Sekula - SMU 4/44 Yes, the Higgs is important for mass, but let’s try this... ● No doubt, the Higgs particle plays a role in fundamental mass (I will come back to this point) ● But, as students who’ve been exposed to introductory physics (mechanics, electricity and magnetism) and some modern physics topics (quantum mechanics and special relativity) you are more familiar with.. -
KAONIC and OTHER EXOTIC ATOMS 243 Atoms Got Underway in Earnest with the Invention and Application of Semiconductor Detectors
Copyright 1975. All rights reserved KAONIC AND OTHER :.:5562 EXOTIC ATOMS Ryoichi Seki California State University, Northridge, California 91324 Clyde E. Wiegand Lawrence Berkeley Laboratory, University of California, Berkeley, California 94720 CONTENTS 1 INTRODUCTION................................................ 241 2 BASIC CHARACTERISTICS OF EXOTIC ATOMS. .. 245 3 EXPERIMENTAL FINDINGS. .. 248 3.1 X-Ray Intensities.. .. .. .. .. .. .. .. .. .. .. 248 248 3.1.1 Kaonic.atoms....................................... .. 3.1.2 Sigmonic atoms.. 250 . .. 3.1.3 Antiprotonic atoms. 250 . .. 3.2 Level Shifts and Widths. 250 . .. 256 3.3 Particle Properties Derivedfrom Exotic Atoms. 3.3.1 Mass.. 257 . .. 258 3.3.2 Magnetic moment.. 259 3.3.3 Polarizability....................................... .. 3.4 Atomic Phenomena Directly Related to Nuclear Properties. 260 '. .. 260 3.4.1 Nuclear quadrupole moment..... ............... .. 260 3.4.2 Dynamical quadrupole (E2) mixing. .. 261 3.5 Products from Nuclear Absorption of K-, �-, and p. 3. 5. 1 Particles observed in nuclear emulsions and bubble chambers.. 261 . 264 3.5.2 Nuclear y rays.. 4 THEORETICAL UNDERSTANDING. .. .. .. .. .. .. .. .. .. 265 . 4.1 Atomic Capture and Cascade.. 266 Annu. Rev. Nucl. Sci. 1975.25:241-281. Downloaded from www.annualreviews.org Atomic capture.. 266 Access provided by Pennsylvania State University on 02/13/15. For personal use only. 4.1.1 .. .. .. .. .. 267 4.1.2 Atomic cascade.. 268 4.2 Strong Interactions with Nuclei.. 269 4.2.1 K --nucleus optical potential.. - . 4.2.2 p- and � -nucleus optical potential. 276 27 4.3 Two- and One-Nucleon Absorption Products. .. .. .. .. .. .. .. 7 . .. 278 5 CONCLUDING REMARKS. 1 INTRODUCTION In this article we attempt to tell what is known about kaonie, sigmonic, and anti protonic atoms. -
New Physics of Strong Interaction and Dark Universe
universe Review New Physics of Strong Interaction and Dark Universe Vitaly Beylin 1 , Maxim Khlopov 1,2,3,* , Vladimir Kuksa 1 and Nikolay Volchanskiy 1,4 1 Institute of Physics, Southern Federal University, Stachki 194, 344090 Rostov on Don, Russia; [email protected] (V.B.); [email protected] (V.K.); [email protected] (N.V.) 2 CNRS, Astroparticule et Cosmologie, Université de Paris, F-75013 Paris, France 3 National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 31 Kashirskoe Chaussee, 115409 Moscow, Russia 4 Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie 6, 141980 Dubna, Russia * Correspondence: [email protected]; Tel.:+33-676380567 Received: 18 September 2020; Accepted: 21 October 2020; Published: 26 October 2020 Abstract: The history of dark universe physics can be traced from processes in the very early universe to the modern dominance of dark matter and energy. Here, we review the possible nontrivial role of strong interactions in cosmological effects of new physics. In the case of ordinary QCD interaction, the existence of new stable colored particles such as new stable quarks leads to new exotic forms of matter, some of which can be candidates for dark matter. New QCD-like strong interactions lead to new stable composite candidates bound by QCD-like confinement. We put special emphasis on the effects of interaction between new stable hadrons and ordinary matter, formation of anomalous forms of cosmic rays and exotic forms of matter, like stable fractionally charged particles. The possible correlation of these effects with high energy neutrino and cosmic ray signatures opens the way to study new physics of strong interactions by its indirect multi-messenger astrophysical probes. -
MIT at the Large Hadron Collider—Illuminating the High-Energy Frontier
Mit at the large hadron collider—Illuminating the high-energy frontier 40 ) roland | klute mit physics annual 2010 gunther roland and Markus Klute ver the last few decades, teams of physicists and engineers O all over the globe have worked on the components for one of the most complex machines ever built: the Large Hadron Collider (LHC) at the CERN laboratory in Geneva, Switzerland. Collaborations of thousands of scientists have assembled the giant particle detectors used to examine collisions of protons and nuclei at energies never before achieved in a labo- ratory. After initial tests proved successful in late 2009, the LHC physics program was launched in March 2010. Now the race is on to fulfill the LHC’s paradoxical mission: to complete the Stan- dard Model of particle physics by detecting its last missing piece, the Higgs boson, and to discover the building blocks of a more complete theory of nature to finally replace the Standard Model. The MIT team working on the Compact Muon Solenoid (CMS) experiment at the LHC stands at the forefront of this new era of particle and nuclear physics. The High Energy Frontier Our current understanding of the fundamental interactions of nature is encap- sulated in the Standard Model of particle physics. In this theory, the multitude of subatomic particles is explained in terms of just two kinds of basic building blocks: quarks, which form protons and neutrons, and leptons, including the electron and its heavier cousins. From the three basic interactions described by the Standard Model—the strong, electroweak and gravitational forces—arise much of our understanding of the world around us, from the formation of matter in the early universe, to the energy production in the Sun, and the stability of atoms and mit physics annual 2010 roland | klute ( 41 figure 1 A photograph of the interior, central molecules. -
Introduction to Supersymmetry
Introduction to Supersymmetry Pre-SUSY Summer School Corpus Christi, Texas May 15-18, 2019 Stephen P. Martin Northern Illinois University [email protected] 1 Topics: Why: Motivation for supersymmetry (SUSY) • What: SUSY Lagrangians, SUSY breaking and the Minimal • Supersymmetric Standard Model, superpartner decays Who: Sorry, not covered. • For some more details and a slightly better attempt at proper referencing: A supersymmetry primer, hep-ph/9709356, version 7, January 2016 • TASI 2011 lectures notes: two-component fermion notation and • supersymmetry, arXiv:1205.4076. If you find corrections, please do let me know! 2 Lecture 1: Motivation and Introduction to Supersymmetry Motivation: The Hierarchy Problem • Supermultiplets • Particle content of the Minimal Supersymmetric Standard Model • (MSSM) Need for “soft” breaking of supersymmetry • The Wess-Zumino Model • 3 People have cited many reasons why extensions of the Standard Model might involve supersymmetry (SUSY). Some of them are: A possible cold dark matter particle • A light Higgs boson, M = 125 GeV • h Unification of gauge couplings • Mathematical elegance, beauty • ⋆ “What does that even mean? No such thing!” – Some modern pundits ⋆ “We beg to differ.” – Einstein, Dirac, . However, for me, the single compelling reason is: The Hierarchy Problem • 4 An analogy: Coulomb self-energy correction to the electron’s mass A point-like electron would have an infinite classical electrostatic energy. Instead, suppose the electron is a solid sphere of uniform charge density and radius R. An undergraduate problem gives: 3e2 ∆ECoulomb = 20πǫ0R 2 Interpreting this as a correction ∆me = ∆ECoulomb/c to the electron mass: 15 0.86 10− meters m = m + (1 MeV/c2) × . -
Observation of Global Hyperon Polarization in Ultrarelativistic Heavy-Ion Collisions
Available online at www.sciencedirect.com Nuclear Physics A 967 (2017) 760–763 www.elsevier.com/locate/nuclphysa Observation of Global Hyperon Polarization in Ultrarelativistic Heavy-Ion Collisions Isaac Upsal for the STAR Collaboration1 Ohio State University, 191 W. Woodruff Ave., Columbus, OH 43210 Abstract Collisions between heavy nuclei at ultra-relativistic energies form a color-deconfined state of matter known as the quark-gluon plasma. This state is well described by hydrodynamics, and non-central collisions are expected to produce a fluid characterized by strong vorticity in the presence of strong external magnetic fields. The STAR Collaboration at Brookhaven National Laboratory’s√ Relativistic Heavy Ion Collider (RHIC) has measured collisions between gold nuclei at center of mass energies sNN = 7.7 − 200 GeV. We report the first observation of globally polarized Λ and Λ hyperons, aligned with the angular momentum of the colliding system. These measurements provide important information on partonic spin-orbit coupling, the vorticity of the quark-gluon plasma, and the magnetic field generated in the collision. 1. Introduction Collisions of nuclei at ultra-relativistic energies create a system of deconfined colored quarks and glu- ons, called the quark-gluon plasma (QGP). The large angular momentum (∼104−5) present in non-central collisions may produce a polarized QGP, in which quarks are polarized through spin-orbit coupling in QCD [1, 2, 3]. The polarization would be transmitted to hadrons in the final state and could be detectable through global hyperon polarization. Global hyperon polarization refers to the phenomenon in which the spin of Λ (and Λ) hyperons is corre- lated with the net angular momentum of the QGP which is perpendicular to the reaction plane, spanned by pbeam and b, where b is the impact parameter vector of the collision and pbeam is the beam momentum. -
Light Higgs Production in Hyperon Decay
Light Higgs Production in Hyperon Decay Xiao-Gang He∗ Department of Physics and Center for Theoretical Sciences, National Taiwan University, Taipei. Jusak Tandean† Department of Mathematics/Physics/Computer Science, University of La Verne, La Verne, CA 91750, USA G. Valencia‡ Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA (Dated: July 8, 2018) Abstract A recent HyperCP observation of three events in the decay Σ+ pµ+µ− is suggestive of a new particle → with mass 214.3 MeV. In order to confront models that contain a light Higgs boson with this observation, it is necessary to know the Higgs production rate in hyperon decay. The contribution to this rate from penguin-like two-quark operators has been considered before and found to be too large. We point out that there are additional four-quark contributions to this rate that could be comparable in size to the two-quark contributions, and that could bring the total rate to the observed level in some models. To this effect we implement the low-energy theorems that dictate the couplings of light Higgs bosons to hyperons at leading order in chiral perturbation theory. We consider the cases of scalar and pseudoscalar Higgs bosons in the standard model and in its two-Higgs-doublet extensions to illustrate the challenges posed by existing experimental constraints and suggest possible avenues for models to satisfy them. arXiv:hep-ph/0610274v3 16 Apr 2008 ∗Electronic address: [email protected] †Electronic address: [email protected] ‡Electronic address: [email protected] 1 I. INTRODUCTION Three events for the decay mode Σ+ pµ+µ− with a dimuon invariant mass of 214.3 0.5 MeV → ± have been recently observed by the HyperCP Collaboration [1]. -
Exotic Atom Production with Upcs Joint EF07 and EF06 Discussion
Exotic atom production with UPCs Joint EF07 and EF06 discussion: UPC physics with ion beams Tuesday Oct 13, 2020 C.A. Bertulani Texas A&M University-Commerce Gerhard Baur Mark Ellermann Fernando Navarra 1 Pair Production with Atomic Capture Bertulani, Baur, Phys. Rep. 163, 299 (1988) Brazilian J. Phys. 18, 559 (1988) '" = + = → (= + '0) + = + '" Ingredients: 1. Perturbation theory 2. Sommerfeld-Maue wavefunction (e+) 2%& ./( 6 " 012+34 Ψ" = ()* ' 1 + 8 3 9 : 2", 4 < ' + − 1 27" =? &" = v" 3. Bound state wavefunction (e-) ./( =>? @ 6 4 Ψ = 1 + =? 8 3 '0 BCD E F 0 % 2 A 2 Pair Production with Capture 33$ '( ) 1 !~ , ,./0 ln 4 − 2.051 10 *+ - − 1 Baur, Bertulani, NPA 505, 835 (1989) Luminosity: 8 = 8: exp −>? LHC, Pb+Pb à >~ 2 hours EF Mainly K-shell capture, with ~ 20% capture in higher atomic orbitals. Antihydrogen production: Baur, PLB 311, 343 (1993) Munger, Brodsky, Schmidt, PRD 49, 3228 (1994) 3 1996 Baur et al, PLB 368, 251 (1996) 4 First Production of AntiHydrogen Baur et al., PLB 368, 251 (1996) Fermilab 1998: Blanford et al, PRL 80, 3037 (1998) 11 events as predicted Bertulani, Baur, PRD 58, 034005 (1998) 5 Antihydrogen • $96 trillion dollars per gram of antihydrogen (most expensive material to produce) • CERN Antiproton Decelerator (AD) + atom trap • ALPHA experiment CERN: 1S ßà 2S transition à H same as H! within 200 ppt Moretti et al., Nature 419, 456 (2002) à no CPT violation à no “source” for baryon asymmetry • Hbar and anti-gravity: Amole et al., Nature Com. 4, 1785 (2013) à ± ($! gravitational)/($! inertial) mass < 75 à not conclusive • No antideuterium, antitritium, or antihelium atoms have ever been produced. -
Arxiv:2104.06076V2 [Nucl-Ex] 19 Apr 2021 Related to This field
Fundamental physics at the strangeness frontier at DAΦNE. Outline of a proposal for future measurements. C. Curceanu, C. Guaraldo, A. Scordo, D. Sirghi, Laboratori Nazionali di Frascati INFN, Via E. Fermi 54, Frascati, Italy K. Piscicchia Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy C. Amsler, J. Zmeskal Stefan Meyer Institute of the Austrian Academy of Sciences (SMI), Wien, Austria D. Bosnar Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia S. Eidelman Budker Institute of Nuclear Physics (SB RAS), Novosibirsk and Lebedev Physical Institute (RAS), Moscow, Russia H. Ohnishi, Y. Sada Research Center for Electron Photon Science, Tohoku University, Sendai, Japan The DAΦNE collider at INFN-LNF is a unique source of low-energy kaons, which was used by the DEAR, SIDDHARTA and AMADEUS collaborations for unique measurements of kaonic atoms and kaon-nuclei interactions. Presently, the SIDDHARTA-2 collaboration is underway to measure the kaonic deuterium exotic atom. With this document we outline a proposal for fundamental physics at the strangeness frontier for future measurements of kaonic atoms and kaon-nuclei interactions at DAΦNE, which is intended to stimulate discussions within the broad scientific community performing research directly or indirectly arXiv:2104.06076v2 [nucl-ex] 19 Apr 2021 related to this field. PACS numbers: 13.75.Jz, 36.10.-k, 36.10.Gv, 14.40.-n, 25.80.Nv, 29.30.-h, 29.90.+r, 87.64.Gb, 07.85.Fv, 29.40.-n, 29.40.Gx, 29.40.Wk 1. Introduction The DAΦNE collider at INFN-LNF1,2 is a unique source of strangeness (kaons) in the world: it delivers low-momentum (< 140 MeV/c) nearly monochromatic charged kaons, generated by the decay of the φ resonance formed in electron-positron annihilation. -
Mass Generation Via the Higgs Boson and the Quark Condensate of the QCD Vacuum
Pramana – J. Phys. (2016) 87: 44 c Indian Academy of Sciences DOI 10.1007/s12043-016-1256-0 Mass generation via the Higgs boson and the quark condensate of the QCD vacuum MARTIN SCHUMACHER II. Physikalisches Institut der Universität Göttingen, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany E-mail: [email protected] Published online 24 August 2016 Abstract. The Higgs boson, recently discovered with a mass of 125.7 GeV is known to mediate the masses of elementary particles, but only 2% of the mass of the nucleon. Extending a previous investigation (Schumacher, Ann. Phys. (Berlin) 526, 215 (2014)) and including the strange-quark sector, hadron masses are derived from the quark condensate of the QCD vacuum and from the effects of the Higgs boson. These calculations include the π meson, the nucleon and the scalar mesons σ(600), κ(800), a0(980), f0(980) and f0(1370). The predicted second σ meson, σ (1344) =|ss¯, is investigated and identified with the f0(1370) meson. An outlook is given on the hyperons , 0,± and 0,−. Keywords. Higgs boson; sigma meson; mass generation; quark condensate. PACS Nos 12.15.y; 12.38.Lg; 13.60.Fz; 14.20.Jn 1. Introduction adds a small additional part to the total constituent- quark mass leading to mu = 331 MeV and md = In the Standard Model, the masses of elementary parti- 335 MeV for the up- and down-quark, respectively [9]. cles arise from the Higgs field acting on the originally These constituent quarks are the building blocks of the massless particles. When applied to the visible matter nucleon in a similar way as the nucleons are in the case of the Universe, this explanation remains unsatisfac- of nuclei.