DOCSLIB.ORG

The Equation of State and the Sphaleron Rate in the Standard Model

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
The Equation of State and the Sphaleron Rate in the Standard Model The equation of state and the sphaleron rate in the Standard Model Kari Rummukainen University of Helsinki and Helsinki Institute of Physics D'Onofrio, Rummukainen, Tranberg arXiv:1404.3565 D'Onofrio, Rummukainen, arXiv:1508.07161 Big Bang and the little bangs, CERN 8/2016 K. Rummukainen (Helsinki) SM equation of state 1 / 25 The \Bump" The \bump" has ceased to be (. or is it just resting?) the Standard Model rules (still) K. Rummukainen (Helsinki) SM equation of state 2 / 25 Phase transitions in the Standard Model No phase transitions in the Standard Model (at µ = 0) I QCD and EW \phase transitions" are cross-overs Many BSM models have a first order EW phase transition 7! I EW baryogenesis (Kainulainen) I Gravitational waves (Weir) K. Rummukainen (Helsinki) SM equation of state 3 / 25 In this talk: Precision results of EW: I Pseudocritical temperature I Equation of state - \softness", width of the cross-over I Sphaleron rate Why study these? I it's the Standard. I Background to cosmological applications, e.g. leptogenesis I Precision properties of physics K. Rummukainen (Helsinki) SM equation of state 4 / 25 Phase diagram of the electroweak SM After lots of activity on and off the lattice: > ! No phase transition at all, smooth \cross-over" for mHiggs∼72 GeV 130 symmetric phase 120 [Kajantie,Laine,K.R.,Shaposhnikov,Tsypin 95{98] 110 2nd order endpoint /GeV c T 100 see also 1st order transition [Csikor,Fodor, Heitger] 90 [G¨urtler,Ilgenfritz,Schiller,Strecha] broken Higgs phase 80 50 60 70 80 90 mH/GeV K. Rummukainen (Helsinki) SM equation of state 5 / 25 Overall EOS [Laine, Schr¨oder2006] 0.4 12 10 0.3 8 4 6 p / T w m = 150 GeV 0.2 2 4 H c m = 200 GeV s H 1/3 2 0.1 0 1 2 3 4 5 6 1 2 3 4 5 6 10 10 10 10 10 10 10 10 10 10 10 10 T / MeV T / MeV Perturbation theory + Lattice QCD + Hadron RG Here EW transition featureless K. Rummukainen (Helsinki) SM equation of state 6 / 25 Equation of state and the pseudocritical temperature K. Rummukainen (Helsinki) SM equation of state 7 / 25 3d effective theory Tool for perturbative and lattice computations Modes p > g 2T are perturbative (at weak coupling): can be integrated out in stages: 1. p>∼T : fermions, non-zero Matsubara frequencies ! 3d theory (dimensional reduction) 1/ T 2. Electric modes p ∼ gT 2 Obtain a \magnetic theory" for modes p<∼g T . Fully contains the non-perturbative thermal physics. K. Rummukainen (Helsinki) SM equation of state 8 / 25 3d effective theory Physics at T = 0 4D SM action: - Fix physics perturbatively £ (αS (MW ), GF , MH , MW , MZ , Mtop) £ £ £ Integration over scales T and gT (at 2{loop level) £ £ £ 3D continuum effective theory 2{loop countertermsB B in lattice perturbation theory BN 3D lattice theory K. Rummukainen (Helsinki) SM equation of state 9 / 25 0.394 3d effective Lagrangian: 0.3935 /T 2 3 0.393 g 1 1 0.3925 L = F aF a + B B + 0.3 4 ij ij 4 ij ij 0 y 2 y y 2 (Di φ) Di φ + m3φ φ + λ3(φ φ) y -0.3 -0.6 SU(2) + U(1) gauge + Higgs 0.295 Parameters: x 0.29 2 2 0.285 g3 ∼ gW T 2 0.3105 x ≡ λ3=g3 2 4 z 0.31 y ≡ m3=g3 02 2 0.3095 z ≡ g3 =g3 140 150 160 170 T/GeV K. Rummukainen (Helsinki) SM equation of state 10 / 25 Calculating the EOS Developed by Laine and Meyer 2015 Higgs mass parameter ν and T are the only dimensionful parameters For dimensional reasons: p(T ) p µ¯ ν2(¯µ) p (¯µ, ν2(¯µ); g 2(¯µ)) = R ; ; g 2(¯µ) − 0R T 4 T 4 T T 2 T 4 µ¯: MS scale, p0R: zero-temperature pressure g 2(¯µ): all dimensionless couplings in the SM Interaction measure: d p(T ) ∆ = T dT T 4 @(p =T 4) 2ν2[Z hφyφi ] 4p = − R − m 4d R + 0R @ ln(¯µ/T ) T 4 T 4 ≡ ∆1 + ∆2 + ∆3 hφyφi Applying 3d effective theory:∆ = ∆A + ∆B 3D 2 2 2 T K. Rummukainen (Helsinki) SM equation of state 11 / 25 Calculating the EOS y A B hφ φi3D Thus, ∆ = ∆1 + ∆3 + ∆2 + δ2 T 6 All ∆i 's computed perturbatively, uncertainty O(g ) [Laine, Meyer] y On the other hand, hφ φi3D can be perturbatively computed in the symmetric phase and in the broken phase 2 4 Expansions fail near m =g3 ≡ y ∼ 0 { i.e. just at the cross-over ) Non-perturbative evaluation of hφyφi needed ) Lattice simulations Using thermodynamic identities, other quantities can be obtained: p, e, heat capacity CV , speed of sound cs ... Laine and Meyer did the analysis, but using poor quality lattice data (provided by me et al.). ) Revisit with new simulations K. Rummukainen (Helsinki) SM equation of state 12 / 25 Higgs field expectation value 0.6 Red dots: 3D lattice 0.5 (continuum limit) Green bands: 0.4 I Broken phase: 2-loop Coleman-Weinberg [Kajantie et 0.3 >/T φ + al 95] φ < I Symmetric phase: 3-loop 0.2 [Laine and Meyer 2015] Agreement remarkably good 0.1 away from the cross-over P.T. does not converge near the 0 cross-over 140 145 150 155 160 165 170 T/GeV K. Rummukainen (Helsinki) SM equation of state 13 / 25 Higgs susceptibility & pseudocritical temperature 10 β=6 8 β=9 β=16 φ 6 + Define pseudocritical T : maximum φ χ location of the hφyφi susceptibility 4 χφyφ: 2 Tc = 159:6 ± 0:1 ± 1:5 GeV 0 140 145 150 155 160 165 170 1st error: lattice errors T/GeV 2nd error: estimate of the 10 systematic uncertainty in 3d action 8 φ + φ χ 6 Right: continuum extrapolation of χ 4 2 156 157 158 159 160 161 162 T/GeV K. Rummukainen (Helsinki) SM equation of state 14 / 25 Interaction measure 0.7 Convert hφyφi to interaction measure ∆ = ( − 3p)=T 4 4 Band: lattice errors + variation 0.65 µ¯ = (0:5 ::: 2)πT . - 3p)/T ε ( Non-trivial feature between broken phase (low T ) and symmetric phase 0.6 (high T ) behaviour Width of the cross-over region ∼ 2 ::: 3 GeV 140 145 150 155 160 165 170 T/GeV K. Rummukainen (Helsinki) SM equation of state 15 / 25 Pressure and energy density 34.6 Pressure: 4 34.4 e/T Z T 0 p(T ) p(T0) 0 ∆(T ) 4 − 4 = dT 0 1% T T T 34.2 0 T0 4 Use reference temperature , 3p/T 4 34 T0 = 140 GeV, e/T 4 pert. pressure p(T0)=T0 = 11:173 33.8 [Laine, Schr¨oder2006] 4 3p/T Energy density e = ∆ + 3p 33.6 p(T0) has ∼ 1% uncertainty ! 140 145 150 155 160 165 170 uncertainty for e and p T/GeV K. Rummukainen (Helsinki) SM equation of state 16 / 25 More thermodynamics 0.334 142 1/3 0.332 141 0.33 140 2 3 c s /T V 0.328 C 139 0.326 w 138 0.324 137 140 145 150 155 160 165 170 140 145 150 155 160 165 170 T/GeV T/GeV 0 Heat capacity CV = e (T ) 2 0 0 Speed of sound: cs = p =e EOS parameter w = p=e Cross-over well defined, but very soft! K. Rummukainen (Helsinki) SM equation of state 17 / 25 Masses 3 2 Higgs and W screening masses Effective cos θWeinberg 0,8 1.1 m =9 H βG m =16 H βG m 3 β =9 0,6 W G 1 m 3 =16 W βG 0,4 γ 0.9 A m/T 0,2 0.8 cos2 θW 0 0.7 140 145 150 155 160 165 170 140 145 150 155 160 165 170 T/GeV T/GeV K. Rummukainen (Helsinki) SM equation of state 18 / 25 Sphaleron rate K. Rummukainen (Helsinki) SM equation of state 19 / 25 Background Anomaly: baryon number B and gauge topology are connected: Z t Z 3 µν ~ ∆B = ∆L = 3∆NCS = 2 dt dVF Fµν 32π 0 Baryogenesis Rate in thermal equilibrium: h(∆N (t))2i Γ = lim CS V ;t!1 Vt 5 4 In the symmetric phase, Γ / αW T [Arnold, Son, Yaffe 97] 5 4 or rather Γ / αW log(1/αW )T [B¨odeker 98] In the broken phase the rate is exponentially suppressed Turning off of the rate is important for some baryogenesis scenarios K. Rummukainen (Helsinki) SM equation of state 20 / 25 Calculation of the sphaleron rate Non-perturbative ) real-time lattice simulations Several methods: Classical EOM [Ambjorn, Krasnitz 95; + many] I UV modes (HTL) make result lattice spacing depednent [Arnold 97] Classical + HTL effective theories [Moore, Hu, Muller 97; Bodeker, Moore, K.R 99] I More control over UV modes, no continuum limit I Used also in studies of plasma instabilities in HIC B¨odeker method: [B¨odeker 98], heat bath version [Moore 98] 2 I Fully dissipative evolution of soft (g T ) modes X Exact to leading log order log(1=g 2), 9 continuum limit, very simple to use I Same \action" and cont. limit as in 3D thermo simulation 9 lot of lattice results in pure gauge, few in broken EW phase. Here: physical Higgs mass K. Rummukainen (Helsinki) SM equation of state 21 / 25 Evolution of NCS Symmetric T = 152GeV, broken T = 145GeV, deeply broken T = 140GeV (with mH = 113GeV) [D'Onofrio et al 12] 12 1 60 10 0.8 8 0.6 CS CS CS 40 0.4 6 0.2 0 4 20 -0.2 2 -0.4 Chern-Simons number N Chern-Simons number N Chern-Simons number N -0.6 0 0 -0.8 -2 -1 -20 5 5 5 5 5 0.0 5.0×104 1.0×105 1.5×105 2.0×105 0 1×10 2×10 3×10 4×10 5×10 0 1×105 2×105 3×105 4×105 5×105 Measurements Measurements Measurements 1 0 10 1.4 1.2 0.8 -1 10 1 0.6 0.8 -2 10 0.6 0.4 Normalized distribution Normalized distribution 0.4 normalized distribution (log) -3 10 0.2 0.2 -4 0 0 10 0 0.2 0.4 0.6 0.8 1 0 0.2 0.4 0.6 0.8 1 0 0.2 0.4 0.6 0.8 1 Chern-Simons number N Chern-Simons number N CS CS Chern-Simons number NCS K.
Load more

Recommended publications
  • Baryogen, a Monte Carlo Generator for Sphaleron-Like Transitions in Proton-Proton Collisions
    Prepared for submission to JHEP BaryoGEN, a Monte Carlo Generator for Sphaleron-Like Transitions in Proton-Proton Collisions Cameron Bravo1 and Jay Hauser Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA E-mail: [email protected] Abstract: Sphaleron and instanton solutions of the Standard Model provide violation of baryon and lepton numbers and could lead to spectacular events at the LHC or future colliders. Certain models of new physics can also lead to sphaleron-like vacuum transitions. This nonperturbative physics could be relevant to the generation of the matter-antimatter asymmetry of the universe. We have developed BaryoGEN, an event generator that facili- tates the exploration of sphaleron-like transitions in proton-proton collisions with minimal assumptions. BaryoGEN outputs standard Les Houches Event files that can be processed by PYTHIA, and the code is publicly available. We also discuss various approaches to experimental searches for such transitions in proton-proton collisions. arXiv:1805.02786v3 [hep-ph] 21 Jul 2018 1Corresponding author. Contents 1 Introduction1 2 Physics Content2 2.1 Fermionic Content of Transitions2 2.2 Incoming Partons and Cancellations3 2.3 Color Flow5 2.4 Simulation Results6 3 Using the Generator6 4 Conclusions8 1 Introduction The class of solutions of gauge field theories to which the sphaleron belongs were first proposed in 1976 by ’t Hooft [1]. These solutions are nonperturbative, so the cross-sections for processes mediated by the sphaleron cannot be calculated perturbatively, e.g. by using Feynman diagrams. The solutions are high-energy but are unstable and decay immediately. The electroweak (EW) sphaleron was first described in 1984 [2].
    [Show full text]
  • Neutrino CPV Phase and Leptogenesis
    Neutrino CPV phase and Leptogenesis Andrew, Brandon, Erika, Larry, Varuna, Wing The Question How can the CP-violating phase in the neutrino mixing matrix, delta, possibly be related to leptogenesis? Can you make a model where this is transparent and has testable predictions? 2 What is it? ● Experiments have observed an asymmetry in the number of baryons versus anti-baryons in the universe ● Leptogenesis – The process of generating baryogenesis through lepton asymmetry ● This lepton asymmetry is converted into a baryon asymmetry by the sphaleron process ● Leptogenesis is a mechanism that attempts to explain the observed asymmetry – Many different models of Leptogenesis exist – We only consider Leptogenesis with Type I Seesaw 3 Sakharov Conditions Three conditions for dynamically generated baryon asymmetry: I. Baryon (and lepton) Number Violation II. C and CP Symmetry Violation III. Interactions out of Thermal Equilibrium 4 Seesaw Mechanism ● Introduce three right-handed heavy neutrinos, NRi with the following Lagrangian: ● The Majorana mass matrix M is diagonal, the Yukawa matrix may be complex, and the Higgs will give a Majorana mass term to the neutrinos after symmetry breaking ● This gives a mass to the light neutrinos: ● For 0.1 eV light neutrinos and taking λ at the GeV scale, that gives a heavy mass scale of 1010 GeV 5 Seesaw Mechanism ● Self energy diagram N showing flavor change at high energy νf νf’ ● The interaction can be described by: H ● Self energy diagram at low energy νf νf’ with the heavy fields integrated out ● Creates an effective point interaction that can be described by: 6 Seesaw Mechanism ● Relating the high and low energy interactions, we can write the following: ● Where R is orthogonal but may be complex (Casas-Ibarra parametrization); it reshuffles and re-phases the flavors.
    [Show full text]
  • Balancing Asymmetric Dark Matter with Baryon Asymmetry by Sphaleron Transitions †
    Proceeding Paper Balancing Asymmetric Dark Matter with Baryon Asymmetry by Sphaleron Transitions † Arnab Chaudhuri 1,* and Maxim Khlopov 2,3,4 1 Department of Physics and Astronomy, Novosibirsk State University, Novosibirsk, 630090 Novosibirsk Oblast, Russia 2 Institute of Physics, Southern Federal University, 344006 Rostov on Don, Russia; [email protected] 3 Astroparticule et Cosmologie, Université de Paris, CNRS, F-75013 Paris, France 4 National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 115409 Moscow, Russia * Correspondence: [email protected] † Presented at the 1st Electronic Conference on Universe, 22–28 February 2021; Available online: https://ecu2021.sciforum.net/. Abstract: The effect of the electroweak sphaleron transition in balance between baryon excess and and the excess of stable quarks of 4th generation is studied in this paper. Considering the non-violation of SU(2) symmetry and the conservation of electroweak and new charges and quantum numbers of the new family, it makes possible sphaleron transitions between baryons, leptons and 4th family of leptons and quarks. In this paper, we have tried to established a possible definite relationship between the value and sign of the 4th family excess relative to baryon asymmetry. If U-type quarks are the lightest quarks of the 4th family and sphaleron transitions provide excessive U¯ antiquarks, asymmetric dark matter in the form of dark atom bound state of (U¯ U¯ U¯ ) with primordial He nuclei is balanced with baryon asymmetry. Keywords: electroweak phase transition; 4th generation; early universe Citation: Chaudhuri, A.; Khlopov, M. Balancing Asymmetric Dark Matter with Baryon Asymmetry by 1. Introduction Sphaleron Transitions.
    [Show full text]
  • Arxiv:1806.08204V2 [Hep-Ph] 7 Nov 2018
    DO-TH 18/12 CP3-Origins-2018-022 DNRF90 Scalar Dark Matter, GUT baryogenesis and Radiative neutrino mass Wei-Chih Huang∗ CP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark , Fakult¨atf¨urPhysik, Technische Universit¨atDortmund, 44221 Dortmund, Germany Heinrich P¨asy and Sinan Zeißnerz Fakult¨atf¨urPhysik, Technische Universit¨atDortmund, 44221 Dortmund, Germany Abstract We investigate an interesting correlation among dark matter phenomenology, neutrino mass generation and GUT baryogenesis, based on the scotogenic model. The model contains additional right-handed neutrinos N and a second Higgs doublet Φ, both of which are odd under an imposed Z2 symmetry. The neutral component of Φ, i.e. the lightest of the Z2-odd particles, is the dark matter candidate. Due to a Yukawa coupling involving Φ, N and the Standard Model leptons, the lepton asymmetry is converted into the dark matter asymmetry so that a non-vanishing B L − asymmetry can arise from (B L)-conserving GUT baryogenesis, leading to a nonzero baryon − asymmetry after the sphalerons decouple. On the other hand, Φ can also generate neutrino masses radiatively. In other words, the existence of Φ as the dark matter candidate resuscitates GUT baryogenesis and realizes neutrino masses. arXiv:1806.08204v2 [hep-ph] 7 Nov 2018 ∗Electronic address: [email protected] yElectronic address: [email protected] zElectronic address: [email protected] 1 I. INTRODUCTION The origin of the observed baryon asymmetry can not be accounted for within the Standard Model (SM) and is one of the unresolved issues in particle physics and cosmology.
    [Show full text]
  • Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √S = 13 Tev
    Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √s = 13 TeV The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Sirunyan, A. M. et al. “Search for Black Holes and Sphalerons in High-Multiplicity Final States in Proton-Proton Collisions at √s = 13 TeV.” Journal of High Energy Physics 2018, 11 (November 2018): 42 © 2018 The Author(s) As Published https://doi.org/10.1007/JHEP11(2018)042 Publisher Springer Nature Version Final published version Citable link http://hdl.handle.net/1721.1/119253 Terms of Use Creative Commons Attribution 4.0 International License Detailed Terms http://creativecommons.org/licenses/by/4.0/ Published for SISSA by Springer Received: May 15, 2018 Revised: August 28, 2018 Accepted: October 27, 2018 Published: November 7, 2018 Search for black holes and sphalerons in high-multiplicity final states in proton-proton collisions JHEP11(2018)042 p at s = 13 TeV The CMS collaboration E-mail: [email protected] Abstract: A search in energetic, high-multiplicity final states for evidence of physics beyond the standard model, such as black holes, string balls, and electroweak sphalerons, is presented. The data sample corresponds to an integrated luminosity of 35.9 fb−1 collected with the CMS experiment at the LHC in proton-proton collisions at a center-of-mass energy of 13 TeV in 2016. Standard model backgrounds, dominated by multijet production, are determined from control regions in data without any reliance on simulation.
    [Show full text]
  • Arxiv:Hep-Ph/9603208V2 10 Apr 1996 Ac ,1996 1, March INR-913/96 CERN-TH/96-13 5, No Anni 166, 75Th Volume Sakharov’S Nauk, of Fiz
    CERN-TH/96-13 INR-913/96 hep-ph/9603208 March 1, 1996 ELECTROWEAK BARYON NUMBER NON-CONSERVATION IN THE EARLY UNIVERSE AND IN HIGH ENERGY COLLISIONS V. A. Rubakova,1 and M. E. Shaposhnikovb,a,2 a Institute for Nuclear Research of the Russian Academy of Sciences, 60-th October Anniversary Prospect 7a, Moscow 117312, Russia bTheory Division, CERN, CH-1211 Geneva 23, Switzerland Abstract We review recent progress in the study of the anomalous baryon number non-conservation at high temperatures and in high energy collisions. Recent results on high temperature phase transitions are described, and applications to electroweak baryogenesis are considered. The current status of the problem of electroweak instanton-like processes at high energies is outlined. This paper is written on the occasion of Sakharov’s 75th anniversary and will appear in the memorial volume of Uspekhi (Usp. Fiz. Nauk, volume 166, No 5, May 1996). arXiv:hep-ph/9603208v2 10 Apr 1996 CERN-TH/96-13 INR-913/96 March 1, 1996 [email protected] [email protected] Contents 1 Introduction 2 2 Basics of anomalous non-conservation of fermion quantum numbers 4 3 Baryon asymmetry: preliminaries 8 4 Sphaleron rate at finite temperatures 11 4.1 Qualitativediscussion. ...... 11 4.2 TheGreen’sfunctionapproach . ..... 14 4.3 The relation to the “probability flux” formulae . ........... 17 4.4 Quantumversusclassicalrate . ...... 18 4.5 Thesphaleronrateinthebrokenphase . ....... 20 4.6 Real time numerical simulations . ....... 21 4.7 Strongsphalerons................................ ... 23 4.8 Concludingremarks............................... ... 23 5 Phase transitions in gauge theories 24 5.1 Equilibrium approximation . ...... 25 5.2 Simpleestimates ................................
    [Show full text]
  • Sphalerons in the Standard Model with a Real Higgs Singlet
    UM-P-94/102 RCHEP-94/27 Sphalerons in the Standard Model with a real Higgs singlet J. Choi Research Centre for High Energy Physics, School of Physics, University of Melbourne, Parkville, Victoria 3052, Australia Abstract Sphaleron energies within the standard model with a real Higgs singlet added on are calculated. The coupled non-linear equations of motion are numerically solved and the sphaleron energy evaluated for a set of parameters in the Higgs potential. I find a small difference in the sphaleron energy compared to the standard model. A slightly stronger constraint on the strength of the first order phase transition thus results for this model. 1 Introduction If the baryon asymmetry of the universe was generated at the electroweak phase transition, arXiv:hep-ph/9409360v2 21 Sep 1994 as many models are now speculating [1], it is important that the rate of baryon violation be determined more accurately. This rate in the broken symmetry phase is directly related to the energy of the sphaleron configuration in the model, because the sphaleron energy sets the height of the energy barrier between the topologically inequivalent vacua, and baryon violation occurs whenever such a vacuum transition takes place. To preserve any baryon asymmetry created at the phase transition the baryon violation rate must be suppressed in the broken phase and this imposes a constraint on the sphaleron energy at the phase transition. Hence it is important to calculate the sphaleron energy within each model 1 being considered. It is in any case interesting to know the explicit form of the sphaleron configuration in extensions of the Standard Model.
    [Show full text]
  • Sphaleron Induced Transitions at the HE- and HL-LHC HL/HE-LHC Workshop June, 18Th, 2018
    Sphaleron induced transitions at the HE- and HL-LHC HL/HE-LHC Workshop June, 18th, 2018 Simone Amoroso Dasha Shatco 1 Sphalerons Non-Abelian gauge theories have non trivial vacuum structures with an infinite number of ground states differing by topological charges (Chern-Simons number) These solutions are not described in ordinary perturbation theory In the EWK sector of the Standard Model transitions between different vacua, “Sphalerons”, violate Baryon and Lepton number The energy of the sphaleron barrier height in the SM is known explicitly: Being a source of B+L violation Sphalerons they can originate baryogenesys However with a Higgs mass of 125 GeV SM sphalerons cannot explain the matter-antimatter asymmetry in the universe (2nd order phase transition) 2 Sphalerons transitions At low energy tunnelling processes are exponentially suppressed 4⇡ 150 σ e− ↵W 10− Inst ⇠ ⇠ But it has been argued that at high enough energies, the system can pass over the energy barrier avoiding the suppression (0307034) This opens the unique possibility of studying such processes at high energy hadron colliders An ΔN=-1 qq scattering would look like: The sphaleron rate is expected to grow exponentially with the number of additional accompanying gauge bosons Typical expected multiplicities from approximate results are: 3 Phenomenology Studies for sphaleron production in pp collisions where first done at the beginning of the 90ies, in view of the SSC (0212099) Cross-section estimated in the “instanton approximation”, valid for E << Esph predicted to increase
    [Show full text]
  • How to Observe the QCD Instanton/Sphaleron Processes at Hadron Colliders?
    How to observe the QCD instanton/sphaleron processes at hadron colliders? Edward Shuryak and Ismail Zahed Center of Nuclear Theory, Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA Abstract The instanton/sphaleron processes involve gauge fields with changing topology, including a nonzero variation of the Chern-Simons number ∆N = 1. In QCD such processes lead to the production of 2N ∆N units CS ± f CS of the axial charge, proportional to the number of light quark flavors Nf = 3, for u; d; s. In the electroweak theory such processes lead to the production of 12 fermions, with ∆B = ∆L = 3 units of baryon and lepton ± number. While this is all known for a long time, and is one of the pillars of the nonperturbative theory of the QCD vacuum, in this paper we discuss what we call a \reclined tunneling", in which external forces are added to the tunneling processes and create certain gluonic objects with positive invariant mass. The idea to observe these objects experimentally at hadronic colliders have been proposed before, but insofar without success. Motivated by the recent CERN workshop on the topic, we review these ideas. We put forward our own suggestions, in particular to utilize a double-diffractive (Pomeron-Pomeron) collisions to this goal, which we believe maximizes the entrance factor and minimizes the backgrounds. We consider clusters of small (M = 3 10 GeV), medium (M = 10 30 GeV) and high M 100 GeV invariant masses, subsequently. − − ∼ Among the proposed signals are specific flavor combination of channels, originating from well-defined 6-, 8- and 10-quark-antiquark operators, as well as correlation of quark chiralities to be potentially detected via Λ hyperon decays.
    [Show full text]
  • Balancing Asymmetric Dark Matter with Baryon Asymmetry and Dilution of Frozen Dark Matter by Sphaleron Transition
    universe Article Balancing Asymmetric Dark Matter with Baryon Asymmetry and Dilution of Frozen Dark Matter by Sphaleron Transition Arnab Chaudhuri 1,* and Maxim Yu. Khlopov 2,3,4 1 Department of Physics and Astronomy, Novosibirsk State University, Pirogova 2, 630090 Novosibirsk, Russia 2 CNRS, Astroparticule et Cosmologie, Université de Paris, F-75013 Paris, France; [email protected] 3 Institute of Physics, Southern Federal University, 344090 Rostov on Don, Russia 4 Center for Cosmopartilce Physics “Cosmion”, National Research Nuclear University “MEPhI” (Moscow Engineering Physics Institute), 115409 Moscow, Russia * Correspondence: [email protected] Abstract: In this paper, we study the effect of electroweak sphaleron transition and electroweak phase transition (EWPT) in balancing the baryon excess and the excess stable quarks of the 4th generation. Sphaleron transitions between baryons, leptons and the 4th family of leptons and quarks establish a definite relationship between the value and sign of the 4th family excess and baryon asymmetry. This relationship provides an excess of stable U¯ antiquarks, forming dark atoms—the bound state of (U¯ U¯ U¯ ) the anti-quark cluster and primordial helium nucleus. If EWPT is of the second order and the mass of U quark is about 3.5 TeV, then dark atoms can explain the observed dark matter density. In passing by, we show the small, yet negligible dilution in the pre-existing dark matter density, due to the sphaleron transition. Keywords: electroweak phase transition; 4th generation; early universe Citation: Chaudhuri, A.; Khlopov, M.Y. Balancing Asymmetric Dark Matter with Baryon Asymmetry and Dilution of Frozen Dark Matter by 1.
    [Show full text]
  • How Diffusion Works for Electroweak Baryogenesis – and What We Learn for Leptogenesis
    How Diffusion Works for Electroweak Baryogenesis – and what we Learn for Leptogenesis Björn Garbrecht Department of Physics University of Wisconsin–Madison Low Energy Precision Electroweak Physics in the LHC Era INT, University of Washington, Seattle, October 7th 2008 Based on Daniel J. H. Chung, BG, Michael J. Ramsey-Musolf, Sean Tulin, arXiv:0808.1144 [hep-ph] Daniel J.H. Chung, BG, Sean Tulin, arXiv:0807.2283 [hep-ph] Seattle, 10/07/08 Björn Garbrecht – UW-Madison 1/44 Outline 1 Introduction and Overview Diffusion and Chemical Equilibration in 2 Electroweak Baryogenesis 3 The Effect of the Sparticle Mass Spectrum on the Conversion of B–L to B Seattle, 10/07/08 Björn Garbrecht – UW-Madison 2/44 1 Introduction & Overview Seattle, 10/07/08 Björn Garbrecht – UW-Madison 3/44 [Kuzmin, Rubakov, Shaposhnikov (1985); McLerran, Shaposhnikov, Turok, Voloshin Electroweak Baryogenesis (1990), Cohen, Kaplan, Nelson (1990)] strong first order phase transition not with Standard Model weak sphaleron active B C broken phase Eq CP weak sphaleron inactive symmetric phase Seattle, 10/07/08 Björn Garbrecht – UW-Madison 4/44 What Happens at the Wall Generation of Higgsino density from CP- violating local (?) source Diffusion & chemical equilibration ahead of the wall Strong damping due to the non-zero Higgs VEV in the broken phase Seattle, 10/07/08 Björn Garbrecht – UW-Madison 5/44 [Cohen, Kaplan, Nelson (1994), Diffusion Equation for EWBG Huet, Nelson (1995)] inelastic relaxation in local (?) CP- scatterings broken phase violating source The densities denote charge densities (particle density minus antiparticle density). We denote the particular charge densities by the symbol representing the particles, e.g.
    [Show full text]
  • Baryogenesis
    CP Violation, Baryon violation, RPV in SUSY, Mesino Oscillations, and Baryogenesis David McKeen and AEN, arXiv:1512.05359 Akshay Ghalsasi, David McKeen, AEN., arXiv:1508.05392 (Thursday: Kyle Aitken, David McKeen, AEN, Thomas Neder, arXiv:1708.01259) (See also Seyda Ipek, David McKeen, AEN., arXiv:1407.8193 Seyda Ipek, John March-Russell, arXiv:1604.00009) Neutron-Antineutron Oscillations: Appearance, Disappearance, and Baryogenesis October 24, 2017 CP V beyond the Standard Model • Needed to produce early universe asymmetry of 10-8 between quarks and anti-quarks? (baryogenesis) • Effects of CKM phase in early universe highly suppressed by small mixing angles and mass differences. non standard CPV • or • non standard enhancement of standard CPV 2 Baryon Violation • SM: Anomalous effect in weak interactions (“Sphalerons”) rapid violation of B, L at T> ~ 100 GeV (weak transition), negligible B violation at low T (tunneling) • Sphalerons conserve B-L • Baryogenesis: • produce net B-L at high T (e.g. leptogenesis) • electroweak baryogenesis (no BSM B or L violation needed) • post sphaleron baryogenesis (requires B violation at low energy which does not allow proton decay) 3 Why ‘post sphaleron’ baryogenesis is compelling • Consistent with wide range of cosmology/inflation models. • No high temperature required (solves a lot of cosmological issues, e.g. gravitino over production) • Electroweak baryogenesis requires 1st order weak transition, CPV in Higgs sector—very constrained by electric dipole moment of electron, mass of Higgs. 4 Consequence
    [Show full text]