Search for Higgs Boson Decays to a Meson and a Photon

Total Page:16

File Type:pdf, Size:1020Kb

Search for Higgs Boson Decays to a Meson and a Photon Search for Higgs boson decays to a meson and a photon Konstantinos Nikolopoulos University of Birmingham on behalf of the ATLAS and CMS Collaborations Precision Workshop - Rencontres du Vietnam ATLAS experiment at CERN 26 September 2016, Quy Nhon, Vietnam This project has received funding from the European Union’s 7th Framework Programme for research, technological development and demonstration under grant agreement no 334034 (EWSB) Higgs Mechanism: Scalar Couplings Structure Higgs-fermion interactions: YukawaBosonic sector:couplings + V EWSB gives mass to W , W −, Z bosons H • Higgs interactions to vector bosons: defined by symmetryHiggs breaking couplings proportional to m2 gHV V • W /Z Higgs interactions to fermions: ad-hoc hierarchical Yukawa couplings∝mf 2m2 g = V V HVV v Higgs Mechanism: Scalar Couplings Structure Fermionic sector: Bosonic sector: f + V EWSB gives mass to W , W −, Z bosons H After introducting Higgs field, can add • H • Higgs couplings proportional to m2 gHV V gHff¯ Yukawa terms to Lagrangian • W /Z 2 m Higgs couplings proportional to fermion mass 2 2mV f • 2mV ghV V = V ghff¯ = f¯ gHVV = υ υ mf v gHf f¯ = Yf = v Fermionic sector: v is Higgs field vacuum expectation value f • After introducting Higgs field, can add Loops (e.g. γ,gluon)sensitivetoBSMphysics H • Yukawa couplings not imposed• by fundamental principle gHff¯ Yukawa terms to Lagrangian Higgs couplings Enhanced proportional Yukawa to fermion couplings mass in BSM scenarios • 4of39 ¯ [Phys. Rev. D80, 076002, Phys. Lett. B665 (2008) 79, Phys.Rev. D90 (2014) 115022,…] f mf Unitarityg ¯ = Y = bounds (through EFT) for fermion mass Hf f f v generation scale (1st/2nd generation) v is Higgs field vacuum expectation value • Loops (e.g. γ,gluon)sensitivetoBSMphysics • υ3 ⇤ <20 TeV 4of39 ⇠ smf [Phys. Rev. Lett. 59, 2405 (1987); Phys.Rev. D71 (2005) 093009] K. Nikolopoulos / Quy Nhon, 26 Sep 2016 / Search for Higgs boson decays to a meson and a photon 2 Higgs-fermion interactions: The story so far 4.5(3.4)σ ATLAS-CONF-2015-044 JHEP 1504 (2015) 117 Progress in Higgs boson properties: mass known to 0.19% bosonic decays measured to ~20-30% In fermion sector, different picture: 3.2(3.5)σ τ-lepton: direct evidence by ATLAS and CMS for h→ττ e,µ: no evidence→non-universality t-quark: no firm evidence for ttH; indirect evidence b-quark: no evidence for h→bb in LHC; mild excesses c-quark: no direct evidence, loose bounds from h→bb u/d/s-quarks: no direct searches available JHEP 1405 (2014) 104 K. Nikolopoulos / Quy Nhon, 26 Sep 2016 / Search for Higgs boson decays to a meson and a photon 3 We take m =125.9 0.4 GeV, and we obtain Γ(H γγ)=9.565 10−6 GeV from H ± → × the values of the Higgs-boson total width and branching fraction to γγ in Refs. [11, 12]. We estimate the uncertainties in the indirect amplitude along the lines that were suggested in footnote 2 of Ref. [8]. In Γ(H γγ), we take the uncertainty from uncalculated higher- → order corrections to be 1%, and the uncertainties that arise from the uncertainties in the top-quark mass mt and the W -boson mass mW to be 0.022% and 0.024%, respectively. We take the uncertainties in theExclusive leptonic decay widths Decays to be 2.5% for h the→J/ψQandγ 1.3% for h→Qγ decays:the a Υclean. We probe estimate on the Yukawa uncertainties couplings in the of indirect 1st and amplitude 2nd generation from uncalculated quarks mass Q is a vector meson or quarkonium2 2 state corrections to be mV /mH . We have not included the effects of the uncertainty in mH , as it Two contributions: direct and indirect amplitude is expected that that uncertainty will be significantly reduced in Run II of the LHC. Direct amplitude: provides sensitivity to Yukawa couplings The uncertainties in the direct amplitude arise primarily from the uncertainties in φ0, Indirect amplitude: larger contribution than direct amplitude 0 2 FIG. 1: The Feynman diagrams2 for the direct amplitude2 for H V + γ4 at order αs.Theshaded Destructive interferencev , and uncalculated corrections of order αs,orderαsv ,andorder→ v . We estimate the ⟨ ⟩ blob represents the quarkonium wave function. The momenta that are adjacent to the heavy-quark order-α2 correction to be 2%, the order-α v2 correction to be 5% for the J/ψ and 1.5% for s “Direct” contributionlines are defined in the text.s “Indirect” contribution the Υ,andtheorder-v4 correction to be 9% for the J/ψ and 1% for the Υ. The uncertainties Small angular separation of decay products in the direct amplitude that arise from the uncertainties in mc and mb are 0.6% in the case of the J/ψ and 0.1% in the case of the Υ, and so they are negligible in comparison withthe other uncertainties in the direct amplitude. Our results for the widths are7 meson decay 2 −10 Γ(H J/ψ + γ)= (11.9 0.2) (1.04 0.14)κc 10 GeV, (53a) products → FIG. 2: The Feynman± diagram− for the indirect± amplitude for×H V + γ.Thehatchedcircle Phys.Rev.2 →D90 (2014) 11, 113010 Higgs Γ[H Υ(1S)+γ]=!(3.33 0.03) (3.49 0.15)κ! 10−10 GeV, (53b) → represents top-quark! ± or W -boson− loops, and± the shaded!b blob× represents the quarkonium wave function. ExclusiveΓ[H Υ decays(2S)+γ ]=lead!(2 to.18 distinct0.03) experimental(2.48 0.11)κ !2 signatures10−10 GeV, (53c) → ! ± − ± b! × In the direct process, the Higgs boson decays into a heavy quark-antiquark (QQ¯) pair, photon High-pT isolated •quarkonium recoiling against 2 −10 Γ[H Υ(3S)+γ]=!(1.83 0.02) (2.15 0.10)κb! 10 GeV. (53d) high-pT→ isolated photonone of! which radiates± a photon− before± forming a quarkonium! × with the other element of the! pair. ! The SM values for the widths (κQ! =1)are ! K. Nikolopoulos / Quy Nhon, 26 Sep 2016 / Search for Higgs bosonIn the decaysindirect to process a meson, the Higgs and bosona photon decays through a top-quark loop or a vector-4 • ∗ ∗ boson loop to a γ and a γ (virtual+0.05 photon).− The8 γ then decays into a vector quarko- ΓSM(H J/ψ + γ)=1.17−0.05 10 GeV, (54a) nium.→ × Γ [H Υ(1S)+γ]=2.56+7.30 10−12 GeV, (54b) SMThe Feynman→ diagrams for the direct−2.56 and× indirect processes are shown in Figs. 1 and 2, Γ respectively.[H Υ(2 ItS is)+ the quantumγ]=8 interference.46+7.79 between10−12 theseGeV two, processes that provides phase(54c) SM → −5.35 × 3 Γ [H Υ(3S)+γ]=10.25+7.33 10−12 GeV. (54d) SM → −5.45 × 7 We do not include results for the ψ(2S) because a value for v2 [ψ(2S)] does not exist in the literature ⟨ ⟩ and because it is likely that v2 for the ψ(2S) is so large that the theoretical uncertainties in the width would be very large. 18 and κb ∆Υ(1S) = (0.948 0.040) + i(0.130 0.019) eff +0.0184 0.0015i, ± ± κγγ − ! " κb ∆Υ(2S) = (1.014 0.054) + i(0.141 0.022) eff +0.0207 0.0015i, (43) ± ± κγγ − # $ κb ∆Υ(3S) = (1.052 0.060) + i(0.148 0.025) eff +0.0221 0.0015i. ± ± κγγ − ! " Approximate expressions forκ ¯ρ0 ,¯κω andκ ¯φ have been given in (22) and (23). The constant terms in the above results show the tiny power-suppressed corrections. Only for the Υ(nS) states they reach the level of percent. Our complete expressionsfortheCP-oddcoefficients ∆˜ V are also given in Appendix E. It is a good approximation to only keep the direct contributions in these terms, which are likely to give rise to the dominant effects. Their coefficients are the same as in the expressions above, but withκ ¯q replaced by κ˜¯q and κb replaced byκ ˜b. It is interesting to compare our result for the quantities ∆V with corresponding expressions obtained by other authors. From [10] one can extract ∆ρ0 =(0.095 0.020) (2¯κu +¯κd)/3, ∆ =(0.092 0.021) (2¯κ +¯κ )and∆ =(0.130 0.027)¯κ , while from± [32] one can obtain ω ± u d φ ± s ∆ =(0.392 0.053)¯κ , ∆ =(1.048 0.046)κ , ∆ =(1.138 0.053)κ and ∆ = J/ψ ± c Υ(1S) ± b Υ(2S) ± b Υ(3S) (1.175 0.056)κb. These values are systematically higher than ours due to the fact that these authors± have not (or not fully) included QCD radiative corrections and RG evolution effects in the direct contributions. For the Υ(nS) states it is important to keep the small imaginary parts of the direct contributions, since in theExclusive SM the real parts alm Decaysost perfectly cancel h→ inQ theγ combinations 1 ∆V in (37). The result for ∆ω obtained in [10] misses the contribution from ω φ mixing and− contains a sign mistake in front ofκ ¯ . Note also that our predictions for the Substantial− recent% interest% from the theory communityd regarding branching ratio estimatesvector∆V parameters mesons, and we %feasibility: of find light% mesons are significantly more accurate than those obtained in [10]. 6 Br(h J/ψγ)=(2.95 0.07f 0.06direct 0.14h γγ) 10− , → ± J/ψ ± ± → · 4Phenomenologicalresults+1.75 9 Br(h Υ(1S) γ)=(4.61 0.06fΥ(1S) 1.21 direct 0.22h γγ) 10− , → ± − ± → · (45) We begin by quoting our benchmark results for the+0.75h V γ branching fractions9 in the SM.
Recommended publications
  • Mass Shift of Σ-Meson in Nuclear Matter
    Mass shift of σ-Meson in Nuclear Matter J. R. Morones-Ibarra, Mónica Menchaca Maciel, Ayax Santos-Guevara, and Felipe Robledo Padilla. Facultad de Ciencias Físico-Matemáticas, Universidad Autónoma de Nuevo León, Ciudad Universitaria, San Nicolás de los Garza, Nuevo León, 66450, México. Facultad de Ingeniería y Arquitectura, Universidad Regiomontana, 15 de Mayo 567, Monterrey, N.L., 64000, México. April 6, 2010 Abstract The propagation of sigma meson in nuclear matter is studied in the Walecka model, assuming that the sigma couples to a pair of nucleon-antinucleon states and to particle-hole states, including the in medium effect of sigma-omega mixing. We have also considered, by completeness, the coupling of sigma to two virtual pions. We have found that the sigma meson mass decreases respect to its value in vacuum and that the contribution of the sigma omega mixing effect on the mass shift is relatively small. Keywords: scalar mesons, hadrons in dense matter, spectral function, dense nuclear matter. PACS:14.40;14.40Cs;13.75.Lb;21.65.+f 1. INTRODUCTION The study of matter under extreme conditions of density and temperature, has become a very important issue due to the fact that it prepares to understand the physics for some interesting subjects like, the conditions in the early universe, the physics of processes in stellar evolution and in heavy ion collision. Particularly, the study of properties of mesons in hot and dense matter is important to understand which could be the signature for detecting the Quark-Gluon Plasma (QGP) state in heavy ion collision, and to get information about the signal of the presence of QGP and also to know which symmetries are restored [1].
    [Show full text]
  • Phenomenology of Gev-Scale Heavy Neutral Leptons Arxiv:1805.08567
    Prepared for submission to JHEP INR-TH-2018-014 Phenomenology of GeV-scale Heavy Neutral Leptons Kyrylo Bondarenko,1 Alexey Boyarsky,1 Dmitry Gorbunov,2;3 Oleg Ruchayskiy4 1Intituut-Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands 2Institute for Nuclear Research of the Russian Academy of Sciences, Moscow 117312, Russia 3Moscow Institute of Physics and Technology, Dolgoprudny 141700, Russia 4Discovery Center, Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, DK- 2100 Copenhagen, Denmark E-mail: [email protected], [email protected], [email protected], [email protected] Abstract: We review and revise phenomenology of the GeV-scale heavy neutral leptons (HNLs). We extend the previous analyses by including more channels of HNLs production and decay and provide with more refined treatment, including QCD corrections for the HNLs of masses (1) GeV. We summarize the relevance O of individual production and decay channels for different masses, resolving a few discrepancies in the literature. Our final results are directly suitable for sensitivity studies of particle physics experiments (ranging from proton beam-dump to the LHC) aiming at searches for heavy neutral leptons. arXiv:1805.08567v3 [hep-ph] 9 Nov 2018 ArXiv ePrint: 1805.08567 Contents 1 Introduction: heavy neutral leptons1 1.1 General introduction to heavy neutral leptons2 2 HNL production in proton fixed target experiments3 2.1 Production from hadrons3 2.1.1 Production from light unflavored and strange mesons5 2.1.2
    [Show full text]
  • A Quark-Meson Coupling Model for Nuclear and Neutron Matter
    Adelaide University ADPT February A quarkmeson coupling mo del for nuclear and neutron matter K Saito Physics Division Tohoku College of Pharmacy Sendai Japan and y A W Thomas Department of Physics and Mathematical Physics University of Adelaide South Australia Australia March Abstract nucl-th/9403015 18 Mar 1994 An explicit quark mo del based on a mean eld description of nonoverlapping nucleon bags b ound by the selfconsistent exchange of ! and mesons is used to investigate the prop erties of b oth nuclear and neutron matter We establish a clear understanding of the relationship b etween this mo del which incorp orates the internal structure of the nucleon and QHD Finally we use the mo del to study the density dep endence of the quark condensate inmedium Corresp ondence to Dr K Saito email ksaitonuclphystohokuacjp y email athomasphysicsadelaideeduau Recently there has b een considerable interest in relativistic calculations of innite nuclear matter as well as dense neutron matter A relativistic treatment is of course essential if one aims to deal with the prop erties of dense matter including the equation of state EOS The simplest relativistic mo del for hadronic matter is the Walecka mo del often called Quantum Hadro dynamics ie QHDI which consists of structureless nucleons interacting through the exchange of the meson and the time comp onent of the meson in the meaneld approximation MFA Later Serot and Walecka extended the mo del to incorp orate the isovector mesons and QHDI I and used it to discuss systems like
    [Show full text]
  • Quark Diagram Analysis of Bottom Meson Decays Emitting Pseudoscalar and Vector Mesons
    Quark Diagram Analysis of Bottom Meson Decays Emitting Pseudoscalar and Vector Mesons Maninder Kaur†, Supreet Pal Singh and R. C. Verma Department of Physics, Punjabi University, Patiala – 147002, India. e-mail: [email protected], [email protected] and [email protected] Abstract This paper presents the two body weak nonleptonic decays of B mesons emitting pseudoscalar (P) and vector (V) mesons within the framework of the diagrammatic approach at flavor SU(3) symmetry level. Using the decay amplitudes, we are able to relate the branching fractions of B PV decays induced by both b c and b u transitions, which are found to be well consistent with the measured data. We also make predictions for some decays, which can be tested in future experiments. PACS No.:13.25.Hw, 11.30.Hv, 14.40.Nd †Corresponding author: [email protected] 1. Introduction At present, several groups at Fermi lab, Cornell, CERN, DESY, KEK and Beijing Electron Collider etc. are working to ensure wide knowledge of the heavy flavor physics. In future, a large quantity of new and accurate data on decays of the heavy flavor hadrons is expected which calls for their theoretical analysis. Being heavy, bottom hadrons have several channels for their decays, categorized as leptonic, semi-leptonic and hadronic decays [1-2]. The b quark is especially interesting in this respect as it has W-mediated transitions to both first generation (u) and second generation (c) quarks. Standard model provides satisfactory explanation of the leptonic and semileptonic decays but weak hadronic decays confronts serious problem as these decays experience strong interactions interferences [3-6].
    [Show full text]
  • 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.
    [Show full text]
  • D MESON PRODUCTION in E+E ANNIHILATION* Petros-Afentoulis Rapidis Stanford Linear Accelerator Center Stanford University Stanfor
    SLAC-220 UC-34d (E) D MESON PRODUCTION IN e+e ANNIHILATION* Petros-Afentoulis Rapidis Stanford Linear Accelerator Center Stanford University Stanford, California 94305 June 1979 Prepared for the Department of Energy under contract number DE-AC03-76SF00515 Printed in the United States of America . Available from National Technical Information Service, U .S . Department of Commerce, 5285 Port Royal Road, Springfield, VA 22161 . Price : Printed Copy $6 .50 ; Microfiche $3 .00 . * Ph .D . dissertation . ABSTRACT The production of D mesons in e+e annihilation for the center-of- mass energy range 3 .7 to 7 .0 GeV has been studied with the MARK :I magnetic detector at the Stanford Positron Electron Accelerating Rings facility . We observed a resonance in the total cross-section for hadron production in e+e annihilation at an energy just above the threshold for charm production. This resonance,which we name I", has a mass of 3772 ± 6 MeV/c 2 , a total width of 28 ± 5 MeV/c 2 , a partial width to electron pairs of 345 ± 85 eV/c 2 , and decays almost exclusively into DD pairs . The •" provides a rich source of background-free and kinematically well defined D mesons for study . From the study of D mesons produced in the decay of the *" we have determined the masses of the D ° and D+ mesons to be 1863 .3 ± 0 .9 MeV/c 2 and 1868 .3 ± 0 .9 MeV/c 2 respectively . We also determined the branching fractions for D ° decay to K-7r+ , K°ir+e and K 1r+ur ir+ to be (2 .2 ± 0 .6)%, (4 .0 ± 1 .3)%, and (3 .2 ± 1 .1)% and the r+i+ + branching fractions for D + decay to K°7+ and K to be (1 .5 0 .6)1 and (3 .9 '~ 1 .0)% .
    [Show full text]
  • Chapter 16 Constituent Quark Model
    Chapter 16 Constituent Quark Model 1 Quarks are fundamental spin- 2 particles from which all hadrons are made up. Baryons consist of three quarks, whereas mesons consist of a quark and an anti-quark. There are six 2 types of quarks called “flavours”. The electric charges of the quarks take the value + 3 or 1 (in units of the magnitude of the electron charge). − 3 2 Symbol Flavour Electric charge (e) Isospin I3 Mass Gev /c 2 1 1 u up + 3 2 + 2 0.33 1 1 1 ≈ d down 3 2 2 0.33 − 2 − ≈ c charm + 3 0 0 1.5 1 ≈ s strange 3 0 0 0.5 − 2 ≈ t top + 3 0 0 172 1 ≈ b bottom 0 0 4.5 − 3 ≈ These quarks all have antiparticles which have the same mass but opposite I3, electric charge and flavour (e.g. anti-strange, anti-charm, etc.) 16.1 Hadrons from u,d quarks and anti-quarks Baryons: 2 Baryon Quark content Spin Isospin I3 Mass Mev /c 1 1 1 p uud 2 2 + 2 938 n udd 1 1 1 940 2 2 − 2 ++ 3 3 3 ∆ uuu 2 2 + 2 1230 + 3 3 1 ∆ uud 2 2 + 2 1230 0 3 3 1 ∆ udd 2 2 2 1230 3 3 − 3 ∆− ddd 1230 2 2 − 2 113 1 1 3 Three spin- 2 quarks can give a total spin of either 2 or 2 and these are the spins of the • baryons (for these ‘low-mass’ particles the orbital angular momentum of the quarks is zero - excited states of quarks with non-zero orbital angular momenta are also possible and in these cases the determination of the spins of the baryons is more complicated).
    [Show full text]
  • 8. Quark Model of Hadrons Particle and Nuclear Physics
    8. Quark Model of Hadrons Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 8. Quark Model of Hadrons 1 In this section... Hadron wavefunctions and parity Light mesons Light baryons Charmonium Bottomonium Dr. Tina Potter 8. Quark Model of Hadrons 2 The Quark Model of Hadrons Evidence for quarks The magnetic moments of proton and neutron are not µN = e~=2mp and 0 respectively ) not point-like Electron-proton scattering at high q2 deviates from Rutherford scattering ) proton has substructure Hadron jets are observed in e+e− and pp collisions Symmetries (patterns) in masses and properties of hadron states, \quarky" periodic table ) sub-structure Steps in R = σ(e+e− ! hadrons)/σ(e+e− ! µ+µ−) Observation of cc¯ and bb¯ bound states and much, much more... Here, we will first consider the wave-functions for hadrons formed from light quarks (u, d, s) and deduce some of their static properties (mass and magnetic moments). Then we will go on to discuss the heavy quarks (c, b). We will cover the t quark later... Dr. Tina Potter 8. Quark Model of Hadrons 3 Hadron Wavefunctions Quarks are always confined in hadrons (i.e. colourless states) Mesons Baryons Spin 0, 1, ... Spin 1/2, 3/2, ... Treat quarks as identical fermions with states labelled with spatial, spin, flavour and colour. = space flavour spin colour All hadrons are colour singlets, i.e. net colour zero qq¯ 1 Mesons = p (rr¯+ gg¯ + bb¯) colour 3 qqq 1 Baryons = p (rgb + gbr + brg − grb − rbg − bgr) colour 6 Dr. Tina Potter 8.
    [Show full text]
  • Dark Matter Searches for Monoenergetic Neutrinos Arising from Stopped Meson Decay in the Sun
    UH511-1249-15 CETUP2015-020 Prepared for submission to JCAP Dark Matter Searches for Monoenergetic Neutrinos Arising from Stopped Meson Decay in the Sun Carsten Rotta Seongjin Ina Jason Kumarb David Yaylalic;d aDepartment of Physics, Sungkyunkwan University, Suwon 440-746, Korea bDepartment of Physics & Astronomy, University of Hawai'i, Honolulu, HI 96822, USA cDepartment of Physics, University of Arizona, Tucson, AZ 85721, USA dDepartment of Physics, University of Maryland, College Park, MD 20742, USA E-mail: [email protected], [email protected], [email protected], [email protected] Abstract. Dark matter can be gravitationally captured by the Sun after scattering off solar nuclei. Annihilations of the dark matter trapped and accumulated in the centre of the Sun could result in one of the most detectable and recognizable signals for dark mat- ter. Searches for high-energy neutrinos produced in the decay of annihilation products have yielded extremely competitive constraints on the spin-dependent scattering cross sections of dark matter with nuclei. Recently, the low energy neutrino signal arising from dark-matter annihilation to quarks which then hadronize and shower has been suggested as a competitive and complementary search strategy. These high-multiplicity hadronic showers give rise to a large amount of pions which will come to rest in the Sun and decay, leading to a unique sub- GeV neutrino signal. We here improve on previous works by considering the monoenergetic neutrino signal arising from both pion and kaon decay. We consider searches at liquid scin- arXiv:1510.00170v2 [hep-ph] 25 Nov 2015 tillation, liquid argon, and water Cherenkov detectors and find very competitive sensitivities for few-GeV dark matter masses.
    [Show full text]
  • LIGHT UNFLAVORED MESONS (S = C = B = 0) for I =1(Π, B, Ρ, A): Ud, (Uu Dd)/√2, Du; − for I =0(Η, Η′, H, H′, Ω, Φ, F , F ′): C1(U U + D D) + C2(S S)
    Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, 030001 (2018) and 2019 update LIGHT UNFLAVORED MESONS (S = C = B = 0) For I =1(π, b, ρ, a): ud, (uu dd)/√2, du; − for I =0(η, η′, h, h′, ω, φ, f , f ′): c1(u u + d d) + c2(s s) ± G P π I (J )=1−(0−) Mass m = 139.57061 0.00024 MeV (S = 1.6) ± 8 Mean life τ = (2.6033 0.0005) 10− s (S=1.2) cτ = 7.8045 m ± × [a] π± ℓ± ν γ form factors ± → ± FV = 0.0254 0.0017 F = 0.0119 ± 0.0001 A ± FV slope parameter a = 0.10 0.06 +0.009 ± R = 0.059 0.008 − π− modes are charge conjugates of the modes below. For decay limits to particles which are not established, see the section on Searches for Axions and Other Very Light Bosons. p + π DECAY MODES Fraction (Γi /Γ) Confidence level (MeV/c) µ+ ν [b] (99.98770 0.00004) % 30 µ ± µ+ ν γ [c] ( 2.00 0.25 ) 10 4 30 µ ± × − e+ ν [b] ( 1.230 0.004 ) 10 4 70 e ± × − e+ ν γ [c] ( 7.39 0.05 ) 10 7 70 e ± × − e+ ν π0 ( 1.036 0.006 ) 10 8 4 e ± × − e+ ν e+ e ( 3.2 0.5 ) 10 9 70 e − ± × − e+ ν ν ν < 5 10 6 90% 70 e × − Lepton Family number (LF) or Lepton number (L) violating modes µ+ ν L [d] < 1.5 10 3 90% 30 e × − µ+ ν LF [d] < 8.0 10 3 90% 30 e × − µ e+ e+ ν LF < 1.6 10 6 90% 30 − × − 0 G PC + π I (J )=1−(0 − ) Mass m = 134.9770 0.0005 MeV (S = 1.1) ± mπ mπ0 = 4.5936 0.0005 MeV ± − ± 17 Mean life τ = (8.52 0.18) 10− s (S=1.2) cτ = 25.5 nm ± × HTTP://PDG.LBL.GOV Page1 Created: 5/22/2019 10:04 Citation: M.
    [Show full text]
  • The Quark Model
    Lecture The Quark model WS2018/19: ‚Physics of Strongly Interacting Matter‘ 1 Quark model The quark model is a classification scheme for hadrons in terms of their valence quarks — the quarks and antiquarks which give rise to the quantum numbers of the hadrons. The quark model in its modern form was developed by Murray Gell-Mann - american physicist who received the 1969 Nobel Prize in physics for his work on the theory of elementary particles. * QM - independently proposed by George Zweig 1929 .Hadrons are not ‚fundamental‘, but they are built from ‚valence quarks‘, i.e. quarks and antiquarks, which give the quantum numbers of the hadrons | Baryon | qqq | Meson | qq q= quarks, q – antiquarks 2 Quark quantum numbers The quark quantum numbers: . flavor (6): u (up-), d (down-), s (strange-), c (charm-), t (top-), b(bottom-) quarks anti-flavor for anti-quarks q: u, d, s, c, t, b . charge: Q = -1/3, +2/3 (u: 2/3, d: -1/3, s: -1/3, c: 2/3, t: 2/3, b: -1/3 ) . baryon number: B=1/3 - as baryons are made out of three quarks . spin: s=1/2 - quarks are the fermions! . strangeness: Ss 1, Ss 1, Sq 0 for q u, d, c,t,b (and q) charm: . Cc 1, Cc 1, Cq 0 for q u, d, s,t,b (and q) . bottomness: Βb 1, Bb 1, Bq 0 for q u, d, s,c,t (and q) . topness: Tt 1, Tt 1, Tq 0 for q u, d, s,c,b (and q) 3 Quark quantum numbers The quark quantum numbers: hypercharge: Y = B + S + C + B + T (1) (= baryon charge + strangeness + charm + bottomness +topness) .
    [Show full text]
  • The Periodic Table of Elementary Particles
    The Masses of elementary particles and hadrons Ding-Yu Chung The masses of elementary particles and hadrons can be calculated from the periodic table of elementary particles. The periodic table is derived from dimensional hierarchy for the seven extra spatial dimensions. As a molecule is the composite of atoms with chemical bonds, a hadron is the composite of elementary particles with hadronic bonds. The masses of elementary particles and hadrons can be calculated using the periodic table with only four known constants: the number of the extra spatial dimensions in the superstring, the mass of electron, the mass of Z°, and αe. The calculated masses are in good agreement with the observed values. For examples, the calculated masses for the top quark, neutron, and pion are 176.5 GeV, 939.54MeV, and 135.01MeV in excellent agreement with the observed masses, 176 ± 13 GeV, 939.57 MeV, and 134.98 MeV, respectively. The masses of 110 hadrons are calculated. The overall average difference between the calculated masses and the observed masses for all hadrons is 0.29 MeV. The periodic table of elementary particles provides the most comprehensive explanation and calculation for the masses of elementary particles and hadrons. PACS number(s): 11.25.Sq, 11.30.Pb, 12.10.Kt, 12.40.Yx Keywords: string field theory, supersymmetry, mass relations, hadron mass models and calculations 1 1. Introduction The mass hierarchy of elementary particles is one of the most difficult problems in particle physics. There are various approaches to solve the problem. In this paper, the approach is to use a periodic table.
    [Show full text]