Nicola Neri on Behalf of the Lhcb Collaboration Presenting Also Result from Atlas and CMS

Total Page:16

File Type:pdf, Size:1020Kb

Nicola Neri on Behalf of the Lhcb Collaboration Presenting Also Result from Atlas and CMS Production and decay of heavy flavour baryons Nicola Neri on behalf of the LHCb collaboration presenting also result from Atlas and CMS INFN - Sezione di Milano FPCP 2015 25-29 May 2015 - Nagoya, Japan Outline ‣ Introduction to b-baryon physics ‣ Experimental results ‣ Conclusions Nicola Neri 2 Production and decay of HF baryons - FPCP 2015 Introduction to b-baryon physics Nicola Neri 3 Production and decay of HF baryons - FPCP 2015 Physics motivations ‣ At LHC b-baryons are produced in unprecedented quantities ➝ opens a new field in flavour physics for precision measurements 0 - Most precise measurement of |Vub| using ⇤ b pµ−⌫¯µ decays [arXiv:1504.01568] ! - Mass, lifetimes and branching ratios measurements ‣ b-baryon physics is a relatively unexplored territory: - search for physics beyond the Standard Model (SM) in rare decays and CP violation - useful QCD laboratory in different energy regime with respect to light baryons. Experimental anchor point for QCD models Nicola Neri 4 Production and decay of HF baryons - FPCP 2015 Beautiful baryons ‣ Baryons are fermions composed by 3 quarks ‣ State function antisymmetric under exchange of equal-mass quarks qqq = color space, spin, flavour | iA | iA ⇥ | iS ‣ SU(4) multiplets for baryons made of (u,d,s,b) observed quarks - B= bottomness, Y=hypercharge, I3= Isospin z-component - SU(4) symmetry heavily broken - large b-quark mass - particles in SU(4) multiplets have same spin and parity Nicola Neri 5 Production and decay of HF baryons - FPCP 2015 b-baryons states q2 s, ` S, J ‣ b-baryons ( bq 1 q 2 ) as QCD L = ` + `0 `0 laboratory: q1 - m b m q 1 q 2 simplified dynamics b ground state p + + - b quark in the limit m b j =0 , 1 j = L + s (L = 0) !1(m 4.8GeV) effective static colour field b ⇠ - heavy baryon properties determined by dynamics of diquark system in b- quark color field - Ground state baryons ( L = 0) with spin-parity J P =1 / 2 + , 3 /2+ characterised by the spin-party of p + + the diquark system j =0 , 1 1 + 3 + J P = (J P = not shown) 2 2 Nicola Neri 6 Production and decay of HF baryons - FPCP 2015 b-baryon rare decays 0 ⇤ pµ−⌫¯ ‣ Access to |Vub| CKM element, b ! µ form factors f ( ⇤ b p ) determined by Lattice! QCD. Experimentally very challenging, Vub achieved unprecedented See Greg Ciazerek talk for precision more details 3 V =(3.27 0.23) 10− | ub| ± ⇥ arXiv:1504.01568, submitted to Nature 0 + ‣ Angular analysis of b-baryon ⇤b ⇤µ µ− flavour-changing neutral current ! decays, e.g. b s transitions, is sensitive to physics! beyond Standard Model (SM) arXiv:1503.07138, submitted to JHEP See Christian Linn talk for more details Nicola Neri 7 Production and decay of HF baryons - FPCP 2015 Experimental results Nicola Neri 8 Production and decay of HF baryons - FPCP 2015 b-baryon production ‣ Production cross-section strongly depends on pT of b-hadron : f 0 /fd - different b-quark fragmentation function ratio ⇤ b measured at 0 0 LEP and at LHC, where f ⇤ 0 = P ( b ⇤ b ) and fd = P (b Bd) b ! ! f 0 /fd - measurement of ⇤ b vs pT of b-quark is cleaner to interpret. Expected a slow dependence in that case arXiv:1505.02771 JHEP 08, 143 (2014) PRD85, 032008 (2012) Note: LEP average not included in the fit. LHCb measurements are not independent Nicola Neri 9 Production and decay of HF baryons - FPCP 2015 Production kinematic dependence 0 + 0 + ‣ Use clean ⇤ ⇤ ⇡ − (45K) , B D ⇡ − (106K) exclusive b c ! decays to measure! dependance of f 0 /f d on b-hadron ⇤b kinematics, e.g. pT, pseudorapidity η. ‣ Measure where and x = pT , ⌘ Data sample 1fb-1 at 7 TeV - JHEP08(2014)143 0 + 3.05 < ⌘ < 3.2 0 + ⇤b ⇤c ⇡− B D ⇡− 3.05 < ⌘ < 3.2 ! ! Nicola Neri 10 Production and decay of HF baryons - FPCP 2015 Production kinematic dependence f 0 /fd ‣ Absolute value of ⇤ b from LHCb semileptonic analysis Phys. Rev. D 85 (2012) 032008 - obtain most precise branching ratio measurement of b-baryon to date (8% precision) 0 + stat. syst. semileptonic (B D ⇡−) JHEP08(2014)143 analysis B ! Exponential dependence vs pT Linear dependence vs η Nicola Neri 11 Production and decay of HF baryons - FPCP 2015 0 ⇤ b production cross-section 0 ‣ Measurement of differential production cross-section for ⇤ b 0 + using ⇤ J/ ⇤ decays with J/ µ µ−, ⇤ p⇡− b ! ! ! PLB 714 (2012) 136–157 ‣ pT distribution falls faster than measured b-mesons spectra and than predicted spectra from NLO MC POWHEG and leading-order MC PYTHYA 0 0 ‣ Cross-section ratio σ ( ⇤ b ) / σ ( ⇤ b ) consistent with 1 and constant vs pT, and rapidity |y| Nicola Neri 12 Production and decay of HF baryons - FPCP 2015 0 Observation of ⌅b⇤ ‣ New resonant state compatible with 0 3 + ⌅⇤ (usb) J P = ,j =1 b 2 ‣ Signal reconstruction involves three 21 signal events significance >5σ secondary vertices, ⌅ b− , ⌅ − , ⇤ and a dimuon pair 00 ‣ Theory predicts m ( ⌅ ) m ( ⌅ − ) <m ⇡+ b − b 00 + no strong decay ⌅ b ⌅ b− ⇡ consistent with experimental! results p ⇡− PRL 108, 252002 (2012) 0 ⇤ ⇡− ⌅b− δm = m(⌅⇤ ) m(⌅−) m + = 14.84 0.74 0.28 MeV b − b − ⇡ ± ± µ− 108 14 + 0 µ J/ ± m(⌅⇤ ) = 5945.0 0.7 0.3 2.7(PDG) MeV b ± ± ± ⌅− 0 ⌅− + Γ(⌅b⇤ )=2.1 0.74 MeV b ⇡ ± 0 ⌅b⇤ Nicola Neri 13 Production and decay of HF baryons - FPCP 2015 Two new ⌅ b− baryon resonances 1 + 0 (dsb) J P = ,j =1 ‣ Study ⌅ b ⇡ s− mass spectrum: 2 ⌅b0 2 3 + new resonances consistent with ( dsb ) J P = ,j =1 ⌅b⇤ 2 121 12 ± 237 24 ± -1 0 0 3fb data at 7-8 TeV - PRL 114, 062004 (2015) δm = m(⌅ ⇡−) m(⌅ ) m b − b − ⇡− Nicola Neri 14 Production and decay of HF baryons - FPCP 2015 ⌅ b− helicity angle distributions ‣ Flat distribution if J=1/2 or J>1/2 but zero longitudinal polarisation ‣ Cannot determine J value. However, data are consistent with quark model predictions J=1/2 and J=3/2 (if not or weakly polarised) PRL 114, 062004 (2015) 0 ⌅⇤ ⌅b− b ⇡− a =0.89 0.11 a =0.88 0.11 ± + ± ⌅c ✓ Helicity angle definition h 0 ⇡− (0, ) ⌅b ⇤ − ⇡− ⌅b Nicola Neri 15 Production and decay of HF baryons - FPCP 2015 0 ⌅ b lifetime and mass measurements 3fb-1 data at 7-8 TeV - PRL 113, 032001 (2014) ‣ Measure lifetime relative to ⇤ 0 and mass difference m ( ⌅ 0 ) m ( ⇤ 0 ) b b − b 0 + + + 0 + + + ⇤ ⇤ ⇡−, ⇤ pK−⇡ ⌅ ⌅ ⇡−, ⌅ pK−⇡ b ! c c ! b ! c c ! (180.5 0.5) 103 3775 71 ± ⇥ ± ‣ Ratio of efficiency corrected yields vs time (1/⌧⇤0 1/⌧⌅0 )t N 0 (t)/N 0 (t)=e b − b ⌅b ⇤b Lifetime ratio from a fit using exponential function Nicola Neri 16 Production and decay of HF baryons - FPCP 2015 0 ⌅ b lifetime and mass measurements PRL 113, 032001 (2014) 0 ⇤b lifetime measurements ⌧⇤0 =1.479 0.009 0.010 ps b ± ± PLB, 734, (2014) 122 ‣ Measure ⌧⇤0 =1.449 0.036 0.017 ps b ± ± first measurement PRD 87, 032002 (2013) ⌧⇤0 =1.503 0.052 0.031 ps b ± ± JHEP 07 (2013) 163 0 0 2 ‣ Measure m ( ⌅ b ) m ( ⇤ b ) = 172 . 44 0 .39 0.17 MeV/c − x4± precision± improvement 0 ‣ Measure relative production rate ⇤ b mass measurements m⇤0 = 5619.36 0.26 MeV b ± PRL 112, 202001 (2014) m⇤0 = 5619.7 0.7 1.1 MeV assuming naive Cabibbo factors b ± ± PRD 87, 032002 (2013) obtain f(⌅0)/f(⇤0) 0.2 b b ⇡ Nicola Neri 17 Production and decay of HF baryons - FPCP 2015 lifetime and mass measurements ⌅b− 3fb-1 data at 7-8 TeV - PRL 113, 242002 (2014) 0 0 ‣ Measure lifetime relative to ⇤ and mass difference m ( ⌅ − ) m(⇤ ) b b − b 0 + + + 0 0 + ⇤ ⇤ ⇡−, ⇤ pK−⇡ ⌅− ⌅ ⇡−, ⌅ pK−K−⇡ b ! c c ! b ! c c ! (220.5 0.5) 103 1799 46 ± ⇥ ± Nicola Neri 18 Production and decay of HF baryons - FPCP 2015 ⌅ − lifetime and mass results b PRL 113, 242002 (2014) Ratio of efficiency vs decay time Ratio of efficiency corrected yields vs decay time ‣ Measure x2 precision improvement 0 ‣ Using LHCb results relative to ⌅ b we obtain ‣ Results consistent with predictions from heavy quark expansion (HQE) Nicola Neri 19 Production and decay of HF baryons - FPCP 2015 0 Observation of ⇤ J/ p ⇡ − decay b ! - Large interference between tree and penguin amplitudes. 0 JHEP07(2014)103 Measure relative BR wrt ⇤ J/ pK − and search for CPV b ! 3 3 V V λ VtbVtd λ ( Vus = λ) / cb cd ⇠ / ⇠ | | 0 0 ⇤ J/ p⇡− 2102 61 ⇤b J/ pK−11179 109 b ! ± ! ± Nicola Neri 20 Production and decay of HF baryons - FPCP 2015 Search for CP violation ∆A 3fb-1 data at 7-8 TeV ‣ Measurement of CP cancel production and proton JHEP07(2014)103 reconstruction asymmetries 0 0 0 + (⇤ J/ ph−)= (⇤ J/ ph−)+ (⇤ ) (h )+ (p) Araw b ! ACP b ! Aprod b − Areco Areco 0 0 ∆A = (⇤ J/ p⇡−) (⇤ J/ pK−) CP Araw b ! − Araw b ! 0 0 + + = (⇤ J/ p⇡−) (⇤ J/ pK−)+ (⇡ ) (K ) ACP b ! − ACP b ! Areco − Areco 0 0 (5.7 2.4 1.2)% 2.2σ from zero raw(B J/ K⇤ )=( 1.10 0.32 0.0.6)% ± ± ⇡ A ! − ± ± ‣ No indications of large local CP asymmetries in Dalitz plane ‣ Rich resonant structure in m ( p ⇡ − ) , no evidence for exotics in m(J/ p),m(J ⇡−) ‣ BR compatible with expected value 0.08: CKM x phase space factor Nicola Neri 21 Production and decay of HF baryons - FPCP 2015 0 (0) Search for ⇤ b ⇤ ⌘ decays ! arXiV:1505.03295 ‣ b-baryons decays to final states with ⌘ , ⌘ 0 not yet Submitted to JHEP observed.
Recommended publications
  • Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays
    Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays !Resonances !Heavy Meson and Baryons !Decays and Quantum numbers !CKM matrix 1 Announcements •No lecture on Friday. •Remaining lectures: •Tuesday 13 March •Friday 16 March •Tuesday 20 March •Friday 23 March •Tuesday 27 March •Friday 30 March •Tuesday 3 April •Remaining Tutorials: •Monday 26 March •Monday 2 April 2 From Friday: Mesons and Baryons Summary • Quarks are confined to colourless bound states, collectively known as hadrons: " mesons: quark and anti-quark. Bosons (s=0, 1) with a symmetric colour wavefunction. " baryons: three quarks. Fermions (s=1/2, 3/2) with antisymmetric colour wavefunction. " anti-baryons: three anti-quarks. • Lightest mesons & baryons described by isospin (I, I3), strangeness (S) and hypercharge Y " isospin I=! for u and d quarks; (isospin combined as for spin) " I3=+! (isospin up) for up quarks; I3="! (isospin down) for down quarks " S=+1 for strange quarks (additive quantum number) " hypercharge Y = S + B • Hadrons display SU(3) flavour symmetry between u d and s quarks. Used to predict the allowed meson and baryon states. • As baryons are fermions, the overall wavefunction must be anti-symmetric. The wavefunction is product of colour, flavour, spin and spatial parts: ! = "c "f "S "L an odd number of these must be anti-symmetric. • consequences: no uuu, ddd or sss baryons with total spin J=# (S=#, L=0) • Residual strong force interactions between colourless hadrons propagated by mesons. 3 Resonances • Hadrons which decay due to the strong force have very short lifetime # ~ 10"24 s • Evidence for the existence of these states are resonances in the experimental data Γ2/4 σ = σ • Shape is Breit-Wigner distribution: max (E M)2 + Γ2/4 14 41.
    [Show full text]
  • 10 Progressing Beyond the Standard Models
    i i “proc16” — 2016/12/12 — 10:17 — page 177 — #193 i i BLED WORKSHOPS Proceedings to the 19th Workshop IN PHYSICS What Comes Beyond ::: (p. 177) VOL. 17, NO. 2 Bled, Slovenia, July 11–19, 2016 10 Progressing Beyond the Standard Models B.A. Robson ? The Australian National University, Canberra, ACT 2601, Australia Abstract. The Standard Model of particle physics (SMPP) has enjoyed considerable success in describing a whole range of phenomena in particle physics. However, the model is con- sidered incomplete because it provides little understanding of other empirical observations such as the existence of three generations of leptons and quarks, which apart from mass have similar properties. This paper examines the basic assumptions upon which the SMPP is built and compares these with the assumptions of an alternative model, the Generation Model (GM). The GM provides agreement with the SMPP for those phenomena which the SMPP is able to describe, but it is shown that the assumptions inherent in the GM allow progress beyond the SMPP. In particular the GM leads to new paradigms for both mass and gravity. The new theory for gravity provides an understanding of both dark matter and dark energy, representing progress beyond the Standard Model of Cosmology (SMC). Povzetek. Standardni Model elektrosibkeˇ in barvne interakcije zelo uspesnoˇ opiseˇ veliko pojavov v fiziki osnovnih delcev. Model imajo kljub temu za nepopoln, ker ne pojasni vrste empiricnihˇ dejstev, kot je obstoj treh generacij leptonov in kvarkov, ki imajo, razen razlicnihˇ mas, zelo podobne lastnosti. V prispevku obravnavamo osnovne predpostavke, na katerih so zgradili ta model in jih primerjamo s predpostavkami alternativnega modela, generacijskega modela.
    [Show full text]
  • The Flavour Puzzle, Discreet Family Symmetries
    The flavour puzzle, discreet family symmetries 27. 10. 2017 Marek Zrałek Particle Physics and Field Theory Department University of Silesia Outline 1. Some remarks about the history of the flavour problem. 2. Flavour in the Standard Model. 3. Current meaning of the flavour problem? 4. Discrete family symmetries for lepton. 4.1. Abelian symmetries, texture zeros. 4.2. Non-abelian symmetries in the Standard Model and beyond 5. Summary. 1. Some remarks about the history of the flavour problem The flavour problem (History began with the leptons) I.I. Rabi Who ordered that? Discovered by Anderson and Neddermayer, 1936 - Why there is such a duplication in nature? - Is the muon an excited state of the electron? - Great saga of the µ → e γ decay, (Hincks and Pontecorvo, 1948) − − - Muon decay µ → e ν ν , (Tiomno ,Wheeler (1949) and others) - Looking for muon – electron conversion process (Paris, Lagarrigue, Payrou, 1952) Neutrinos and charged leptons Electron neutrino e− 1956r ν e 1897r n p Muon neutrinos 1962r Tau neutrinos − 1936r ν µ µ 2000r n − ντ τ 1977r p n p (Later the same things happen for quark sector) Eightfold Way Murray Gell-Mann and Yuval Ne’eman (1964) Quark Model Murray Gell-Mann and George Zweig (1964) „Young man, if I could remember the names of these particles, I „Had I foreseen that, I would would have been a botanist”, have gone into botany”, Enrico Fermi to advise his student Leon Wofgang Pauli Lederman Flavour - property (quantum numbers) that distinguishes Six flavours of different members in the two groups, quarks and
    [Show full text]
  • Lecture 5: Quarks & Leptons, Mesons & Baryons
    Physics 3: Particle Physics Lecture 5: Quarks & Leptons, Mesons & Baryons February 25th 2008 Leptons • Quantum Numbers Quarks • Quantum Numbers • Isospin • Quark Model and a little History • Baryons, Mesons and colour charge 1 Leptons − − − • Six leptons: e µ τ νe νµ ντ + + + • Six anti-leptons: e µ τ νe̅ νµ̅ ντ̅ • Four quantum numbers used to characterise leptons: • Electron number, Le, muon number, Lµ, tau number Lτ • Total Lepton number: L= Le + Lµ + Lτ • Le, Lµ, Lτ & L are conserved in all interactions Lepton Le Lµ Lτ Q(e) electron e− +1 0 0 1 Think of Le, Lµ and Lτ like − muon µ− 0 +1 0 1 electric charge: − tau τ − 0 0 +1 1 They have to be conserved − • electron neutrino νe +1 0 0 0 at every vertex. muon neutrino νµ 0 +1 0 0 • They are conserved in every tau neutrino ντ 0 0 +1 0 decay and scattering anti-electron e+ 1 0 0 +1 anti-muon µ+ −0 1 0 +1 anti-tau τ + 0 −0 1 +1 Parity: intrinsic quantum number. − electron anti-neutrino ν¯e 1 0 0 0 π=+1 for lepton − muon anti-neutrino ν¯µ 0 1 0 0 π=−1 for anti-leptons tau anti-neutrino ν¯ 0 −0 1 0 τ − 2 Introduction to Quarks • Six quarks: d u s c t b Parity: intrinsic quantum number • Six anti-quarks: d ̅ u ̅ s ̅ c ̅ t ̅ b̅ π=+1 for quarks π=−1 for anti-quarks • Lots of quantum numbers used to describe quarks: • Baryon Number, B - (total number of quarks)/3 • B=+1/3 for quarks, B=−1/3 for anti-quarks • Strangness: S, Charm: C, Bottomness: B, Topness: T - number of s, c, b, t • S=N(s)̅ −N(s) C=N(c)−N(c)̅ B=N(b)̅ −N(b) T=N( t )−N( t )̅ • Isospin: I, IZ - describe up and down quarks B conserved in all Quark I I S C B T Q(e) • Z interactions down d 1/2 1/2 0 0 0 0 1/3 up u 1/2 −1/2 0 0 0 0 +2− /3 • S, C, B, T conserved in strange s 0 0 1 0 0 0 1/3 strong and charm c 0 0 −0 +1 0 0 +2− /3 electromagnetic bottom b 0 0 0 0 1 0 1/3 • I, IZ conserved in strong top t 0 0 0 0 −0 +1 +2− /3 interactions only 3 Much Ado about Isospin • Isospin was introduced as a quantum number before it was known that hadrons are composed of quarks.
    [Show full text]
  • Quarks and Their Discovery
    Quarks and Their Discovery Parashu Ram Poudel Department of Physics, PN Campus, Pokhara Email: [email protected] Introduction charge (e) of one proton. The different fl avors of Quarks are the smallest building blocks of matter. quarks have different charges. The up (u), charm They are the fundamental constituents of all the (c) and top (t) quarks have electric charge +2e/3 hadrons. They have fractional electronic charge. and the down (d), strange (s) and bottom (b) quarks Quarks never exist alone in nature. They are always have charge -e/3; -e is the charge of an electron. The found in combination with other quarks or antiquark masses of these quarks vary greatly, and of the six, in larger particle of matter. By studying these larger only the up and down quarks, which are by far the particles, scientists have determined the properties lightest, appear to play a direct role in normal matter. of quarks. Protons and neutrons, the particles that make up the nuclei of the atoms consist of quarks. There are four forces that act between the quarks. Without quarks there would be no atoms, and without They are strong force, electromagnetic force, atoms, matter would not exist as we know it. Quarks weak force and gravitational force. The quantum only form triplets called baryons such as proton and of strong force is gluon. Gluons bind quarks or neutron or doublets called mesons such as Kaons and quark and antiquark together to form hadrons. The pi mesons. Quarks exist in six varieties: up (u), down electromagnetic force has photon as quantum that (d), charm (c), strange (s), bottom (b), and top (t) couples the quarks charge.
    [Show full text]
  • The Quantum Chromodynamics Theory of Tetraquarks and Mesomesonic Particles Unfinished Draft Version
    The Quantum Chromodynamics Theory Of Tetraquarks And Mesomesonic Particles Unfinished draft version Based on a generalized particle diagram of baryons and anti-baryons which, in turn, is based on symmetry principles, this theory predicts the existence of all the tetraquarks and dimeson molecules (mesomesonic particles) there exist in nature. by R. A. Frino Electronics Engineer - Degree from the University of Mar del Plata. March 4th, 2016 (v1) Keywords: mirror symmetry, parity, P symmetry, charge conjugation, C symmetry, time reversal, T symmetry, CP symmetry, CPT symmetry, PC+ symmetry, Q symmetry, quantum electrodynamics, quantum chromodynamics, quark, antiquark, up quark, down quark, strange quark, charm quark, bottom quark, top quark, anti-up quark, anti-down quark, anti-strange quark, anti-charm quark, anti-bottom quark, anti-top quark, tetraquark, pentaquark, antitetraquark, non-strange tetraquark, colour charge, anticolour, anticolour charge, strangeness, charmness, bottomness, topness, fermion, hadron, baryon, meson, boson, photon, gluon, mesobaryonic particle, meso-baryonic particle, mesobaryonic molecule, meso-mesonic molecule, meso-mesonic particle, dimeson particle, dimeson molecule, Pauli exclusion principle, force carrier, omega- minus particle, matter-antimatter way, quadruply flavoured tetraquark, MAW, MMP, MMM, LHC. (see next page) The Quantum Chromodynamics Theory Of Tetraquarks And Mesomesonic Particles - v1. Copyright © 2016 Rodolfo A. Frino. All rights reserved. 1 1. Introduction Quantum Chromodynamics (QCD) [1, 2, 3, 4] is a quantum mechanical description of the strong nuclear force. The strong force is mediated by gluons [4, 5] which are spin 1ℏ bosons (spin is quoted in units of reduced Plank's constant: ℏ =h/2π ). Gluons act on quarks only (only quarks feel the strong force).
    [Show full text]
  • Isospin and Isospin/Strangeness Correlations in Relativistic Heavy Ion Collisions
    Isospin and Isospin/Strangeness Correlations in Relativistic Heavy Ion Collisions Aram Mekjian Rutgers University, Department of Physics and Astronomy, Piscataway, NJ. 08854 & California Institute of Technology, Kellogg Radiation Lab 106-38, Pasadena, Ca 91125 Abstract A fundamental symmetry of nuclear and particle physics is isospin whose third component is the Gell-Mann/Nishijima expression I Z =Q − (B + S) / 2 . The role of isospin symmetry in relativistic heavy ion collisions is studied. An isospin I Z , strangeness S correlation is shown to be a direct and simple measure of flavor correlations, vanishing in a Qg phase of uncorrelated flavors in both symmetric N = Z and asymmetric N ≠ Z systems. By contrast, in a hadron phase, a I Z / S correlation exists as long as the electrostatic charge chemical potential µQ ≠ 0 as in N ≠ Z asymmetric systems. A parallel is drawn with a Zeeman effect which breaks a spin degeneracy PACS numbers: 25.75.-q, 25.75.Gz, 25.75.Nq Introduction A goal of relativistic high energy collisions such as those done at CERN or BNL RHIC is the creation of a new state of matter known as the quark gluon plasma. This phase is produced in the initial stages of a collision where a high density ρ and temperatureT are produced. A heavy ion collision then proceeds through a subsequent expansion to lower ρ andT where the colored quarks and anti-quarks form isolated colorless objects which are the well known particles whose properties are tabulated in ref[1]. Isospin plays an important role in the classification of these particles [1,2].
    [Show full text]
  • Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Lecture 13: Hadron Decays
    Particle Physics Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Lecture 13: Hadron Decays ★Decays and Quantum numbers ★CKM matrix 1 Decays of Hadrons Force Typical τ (s) QCD 10−20 - 10−23 • The proton is the only completely stable hadron QED 10−20 - 10−16 • The free neutron has a weak decay (~15 mins) Weak 10−13 - 103 • Decay length of a particle is distance it travels before decaying L=βγcτ ± ± 0 • π , K , KL mesons are long-lived (~10 ns) and have weak decays ➡ These particles live long enough to travel outside radii of collider detectors (~10 m) 0 0 • KS mesons and Λ hyperons are long-lived (~100 ps) and have weak decays with decay lengths of ~ cm. • π0→γγ, η→γγ are electromagnetic decays, reconstructed from pairs of photons. 2 2 mπ =(p(γ1)+p(γ2)) • ρ, ω, φ, Κ∗, Δ, Σ∗, Ξ∗ are resonances with strong decays. ➡Reconstructed as broad structures with widths ~100 MeV. 2 Decay Conservation Laws • Relevant quantum numbers are: • strong isospin (I, I3) • parity (P) • quark flavour: described using strangeness (S=N(s)−N(s)̅ ), charm (C=N(c)−N(c)̅ ), bottomness (B=N(b)−N(b)̅ ) • Baryon number and lepton numbers are always conserved! Strong Strong baryon Flavour, Isospin, Isospin, Parity, P number S, C, B I I3 Strong Y Y Y Y Y EM Y N Y Y Y Weak Y N N N N 3 Decays of Charmonium • The J/ψ meson is a2007/08 c c —̅ state. Physics 3: Particle It Physics must decay to particles4 without charm quarks as M(J/ψ) < 2 M(D).
    [Show full text]
  • Arxiv:1609.04034V1 [Physics.Gen-Ph] 8 Sep 2016 Asnme() 26.C 53.Q 98.80.Bp 95.30.Cq, 12.60.Rc, Number(S): PACS Atom
    The generation model of particle physics and the cosmological matter-antimatter asymmetry problem B.A. Robson∗ Department of Theoretical Physics, Research School of Physics and Engineering, The Australian National University, Acton ACT 2601, Australia ∗[email protected] The matter-antimatter asymmetry problem, corresponding to the virtual nonexis- tence of antimatter in the universe, is one of the greatest mysteries of cosmology. Within the framework of the Generation Model (GM) of particle physics, it is demon- strated that the matter-antimatter asymmetry problem may be understood in terms of the composite leptons and quarks of the GM. It is concluded that there is essen- tially no matter-antimatter asymmetry in the present universe and that the observed hydrogen-antihydrogen asymmetry may be understood in terms of statistical fluctu- ations associated with the complex many-body processes involved in the formation of either a hydrogen atom or an antihydrogen atom. Keywords: Generation model; antimatter; big bang. PACS Number(s): 12.60.Rc, 95.30.Cq, 98.80.Bp arXiv:1609.04034v1 [physics.gen-ph] 8 Sep 2016 1. Introduction The matter-antimatter asymmetry problem, corresponding to the virtual nonexis- tence of antimatter in the universe, is one of the greatest mysteries of cosmology, along with dark matter and dark energy.1 Recently, an understanding of both dark matter and dark energy has been provided by the development of a new quan- tum theory of gravity,2,3 which is based on the Generation Model (GM) of particle physics.4 In this paper it is demonstrated that the matter-antimatter asymmetry problem may also be understood in terms of the composite leptons and quarks of the GM, contrary to the elementary leptons and quarks of the Standard Model (SM) of particle physics.5 According to the SM of particle physics, the universe is made essentially of mat- ter comprising three kinds of elementary particles: electrons, up quarks and down quarks.
    [Show full text]
  • Introduction to Elementary Particle Physics
    Introduction to Elementary Particle Physics Néda Sadooghi Department of Physics Sharif University of Technology Tehran - Iran Elementary Particle Physics Lecture 9 and 10: Esfand 18 and 20, 1397 1397-98-II Leptons and quarks Lectrue 9 Leptons Lectrue 9 Remarks: I Lepton flavor number conservation: - Lepton flavor number of leptons Le; Lµ; Lτ = +1 - Lepton flavor number of antileptons Le; Lµ; Lτ = −1 Assumption: No neutrino mixing + + − + + Ex.: π ! µ + νµ; n ! p + e +ν ¯e; µ ! e + νe +ν ¯µ But, µ+ ! e+ + γ is forbidden I Two other quantum numbers for leptons - Weak hypercharge YW : It is 1 for all left-handed leptons - Weak isospin T3: ( ) ( ) e− − 1 ! 2 For each lepton generation, for example T3 = 1 νe + 2 I Type of interaction: - Charged leptons undergo both EM and weak interactions - Neutrinos interact only weakly Lectrue 9 Quarks Lectrue 9 Remarks I Hadrons are bound states of constituent (valence) quarks I Bare (current) quarks are not dressed. We denote the current quark mass by m0 I Dressed quarks are surrounded by a cloud of virtual quarks and gluons (Sea quarks) I This cloud explains the large constituent-quark mass M I For hadrons the constituent quark mass M = the binding energy required to make the hadrons spontaneously emit a meson containing the valence quark For light quarks (u,d,s): m0 ≪ M For heavy quarks (c,b,t): m0 ' M Lectrue 9 Remarks: I Type of interaction: - All quarks undergo EM and strong interactions I Mean lifetime (typical time of interaction): In general, - Particles which mainly decay through strong interactions have a mean lifetime of about 10−23 sec - Particles which mainly decay through electromagnetic interactions, signaled by the production of photons, have a mean lifetime in the range of 10−20 − 10−16 sec - Particles that decay through weak forces have a mean lifetime in the range of 10−10 − 10−8 sec Lectrue 9 Other quantum numbers (see Perkins Chapter 4) Flavor Baryon Spin Isospin Charm Strangeness Topness Bottomness El.
    [Show full text]
  • Particle Properties
    Particle Properties You don’t have to remember this information! In an exam the masses of the particles are given on the constant sheet. Any other required information will be given to you. What you should know, or be able to work out, is: • the quantum numbers, and if they are conserved are or not • the force responsible for a decay, from the lifetime • the main decay modes, using a Feynman diagram • that the +, − and 0 superscripts correspond to the electric charge of the particles • the relationship between a particle and its antiparticle. Anti-particles are not named in the tables. Anti-particles have the same mass, same lifetime, opposite quantum numbers from the particle. Anti-particles decay into the anti-particles of the shown modes. For example, an anti-muon, µ+, has a mass of 2 −6 105.7 MeV/c and a lifetime of 2.197 × 10 s. Its quantum numbers are Le = 0,Lµ = + + −1,Lτ = 0 and Q = +1. Its main decay mode is µ → e νeν¯µ. Quantum Numbers The following quantum numbers are conserved in all reactions: • Total quark number, Nq = N(q) − N(¯q). – Nq = +1 for all quarks – Nq = −1 for all anti-quarks – Nq = 0 for all leptons and anti-leptons – Nq = 3 for baryons and Nq = 0 for mesons. • The three lepton flavour quantum numbers: − + – Electron Number: Le = N(e ) − N(e ) + N(νe) − N(¯νe) − + – Muon Number: Lµ = N(µ ) − N(µ ) + N(νµ) − N(¯νµ) − + – Tau Number: Lτ = N(τ ) − N(τ ) + N(ντ ) − N(¯ντ ) • Electric charge, Q.
    [Show full text]
  • Quantum Mechanics Electric Charge
    Quantum Mechanics_Electric charge Electric field of a positive and a negative point charge. Electric charge is the physical property of matterthat causes it to experience a force when placed in an electromagnetic field. There are two types of electric charges – positive and negative. Positively charged substances are repelled from other positively charged substances, but attracted to negatively charged substances; negatively charged substances are repelled from negative and attracted to positive. An object will be negatively charged if it has an excess of electrons, and will otherwise be positively charged or uncharged. The SI derived unit of electric charge is the coulomb (C), although in electrical engineering it is also common to use theampere-hour (Ah), and in chemistry it is common to use the elementary charge (e) as a unit. The symbol Qis often used to denote a charge. The study of how charged substances interact is classical electrodynamics, which is accurate insofar asquantum effects can be ignored. The electric charge is a fundamental conserved property of some subatomic particles, which determines their electromagnetic interaction. Electrically charged matter is influenced by, and produces, electromagnetic fields. The interaction between a moving charge and an electromagnetic field is the source of the electromagnetic force, which is one of the four fundamental forces (See also: Magnetic field). Twentieth-century experiments demonstrated that electric charge is quantized; that is, it comes in integer multiples of individual small units called theelementary charge, e, approximately equal to1.602×10−19 coulombs (except for particles calledquarks, which have charges that are integer multiples of e/3). The proton has a charge of e, and the electron has a charge of −e.
    [Show full text]