Constituent Quark Model and New Particles

Total Page:16

File Type:pdf, Size:1020Kb

Constituent Quark Model and New Particles Constituent-Quark Model and New Particles David Akers* Lockheed Martin Corporation, Dept. 6F2P, Bldg. 660, Mail Zone 6620, 1011 Lockheed Way, Palmdale, CA 93599 *Email address: [email protected] An elementary constituent-quark (CQ) model by Mac Gregor is reviewed with currently published data from light meson spectroscopy. It was previously shown in the CQ model that there existed several mass quanta m = 70 MeV, B = 140 MeV and X = 420 MeV, which were responsible for the quantization of meson yrast levels. The existence of a 70-MeV quantum was postulated by Mac Gregor and was shown to fit the Nambu empirical mass formula mn = (n/2)137me , n a positive integer. The 70-MeV quantum can be derived in three different ways: 1) pure electric coupling, 2) pure magnetic coupling, and 3) mixed electric and magnetic charges (dyons). Schwinger first introduced dyons in a magnetic model of matter. It is shown in this paper that recent data of new light mesons fit into the CQ model (a pure electric model) without the introduction of magnetic charges. However, by introducing electric and magnetic quarks (dyons) into the CQ model, new dynamical forces can be generated by the presence of magnetic fields internal to the quarks (dyons). The laws of angular momentum and of energy conservation are valid in the presence of magnetic charge. With the introduction of the Russell-Saunders coupling scheme into the CQ model, several new meson particles are predicted to exist. The existence of the f0(560) meson is predicted and is shown to fit current experimental data from the Particle Data Group listing. The existence of meson partners or groupings is shown. PACS. 12.39.-x Phenomenological quark models - 12.40.Yx Hadron mass models and calculations - 14.80.Hv Magnetic monopoles 1 Introduction In the course of researching particle physics over several decades, Mac Gregor [1] developed a comprehensive constituent-quark (CQ) model of elementary particles. It was shown that the CQ masses were directly related to the masses of the electron, muon, and pion. A connection was later discovered between the CQ masses of Mac Gregor’s model and Nambu’s empirical mass formula mn = (n/2)137me, n a positive integer and me the mass of the electron [2]. Mac Gregor’s esoteric notation included a 70 MeV quantum, a boson excitation B with the mass of the pion at 140 MeV, a fermion excitation F with a mass of 210 MeV or twice the muon mass, and a 420 MeV excitation quantum X. The 70 MeV quantum and the 420 MeV quantum X do not correspond to any observed particles but serve as the building blocks of mesons and baryons in the CQ model. These building blocks were not introduced in an ad hoc manner but were derived from experimental systematics and angular momentum systematics of hadron spectroscopy [3- 4]. The mass regularities in meson and baryon spectra were identified independently of any theoretical viewpoint [5]. The mechanism for generating the CQ masses is discussed in Mac Gregor [1] and will be discussed further in Section 3. It is sufficient to say that we shall accept the evidence of Mac Gregor’s CQ model from its previous agreement with earlier experimental data and that we shall present further evidence from the Particle Data Group listing [6]. The experimental evidence to be presented is limited to the meson spectrum only for the purpose of our study. The common mass-band structures of the baryons were also studied and can be found in Mac Gregor’s work [1]. A sequel to the present paper on the subject of baryons can be found in Ref. [7]. In the CQ model, the mass of the resonance is determined mainly from the masses of the constituent quarks. Spin and orbital excitations can also contribute to the mass of the resonance with higher mass-states appearing at higher total angular momentum values. However, mesons with different J values appear in the same mass band in Fig. 2 of Mac 2 Gregor’s work [1]. These meson resonances appear with accurate J ~ M2 Regge trajectories for JP = 1-, 2+, and 3-. Likewise, the meson spectrum also exhibits non-Regge spacing with J ~ M for the 2+, 3-, 4+, 5- and 1+, 2-, 3+ yrast levels in Fig. 2 of Mac Gregor’s paper. The spacing of the Regge-like and non-Regge levels is in accurate 420 MeV intervals, for which Mac Gregor assigned an excitation quantum X1 = 420 MeV. The quantum X can appear with zero or non-zero units of angular momentum. Additional sets of resonances are found to depend upon their quark content. For the CQ model, the constituent-quark basis states are calculated to be u(315), d(320), s(525), c(1575), and b(4725). The CQ model was postulated long before the advent of the top quark and has not been extended to the energy range for resonances involving the top quark. For purposes of our study, we limit our discussion to mesons below 2600 MeV. In addition to the excitation quantum X, there are mesons which exhibit equal spacing in the excitation quantum B = 140 MeV or the mass of the pion, as shown in Fig. 3 of Mac Gregor’s work [1]. From the analysis in Ref. [1] and from previous work [3-5], Mac Gregor concluded that the excitation quantum B served as a fundamental mass unit. In this paper, it is shown that there is exists a fine structure in one-half units of B or m = 70 MeV, separating meson band states. The mechanisms for generating this quantum m = 70 MeV will be discussed in Section 3. The evidence for this quantum is presented in Refs. [1, 3-5] and is shown in Table 1, which has the usual CQ model notation and which has the primary mesons π0(134), K±(494), and η(547) in the ground states. These mesons are listed with shell numbers (on the 70 MeV scale) in isospin space. Evidence of shell structure can be found in meson and baryon spectroscopy [8]. Earlier ideas of shell structure can be found in Ref. [9]. In Table 1, we list all the well-established 3 mesons, underlining them. The not-so-well-established resonances are also included in the CQ model. This table is an update to Table VII in Mac Gregor’s work [1] and has additional fine structure representing new states at the 1400 to 2450 MeV energy levels. These new states have m = 70 MeV regular spacings between them. This is a feature not explained in the Standard Model of elementary particle physics. It is noted that many if not all the known mesons below 2600 MeV fit into the CQ model. Moreover, in Table 2 we show a regrouping of the mesons from Table 1. On the 70-MeV scale, shell numbers are now identified in ordinary space in Table 2. In the paper by Mac Gregor [3], the 70- MeV excitation spacing can also be found for both mesons and baryons in his Fig. 8. Additional 70-MeV spacing is shown in Fig. 21 of Ref. [4]. The CQ notations for Tables 1 and 2 do not follow the rotational band rules established by Mac Gregor in Ref. [3], because we are only interested in the total CQ excitation masses for the energy levels shown in parentheses. Additional rules for hadronic binding energies and properties can be found in Ref. [4]. As shown in Tables 1 and 2, these mesons are grouped into excitation bands with different spins and isospins. For the sake of readers who may not be familiar with the notation of the CQ model, the energy bands are calculated from the total mass values as indicated by the symbols of the m, B, F and X quanta. For a notation such as X3, this represents a molecular type writing by Mac Gregor and thus has value XXX = 420 + 420 + 420 = 1260 MeV, as shown in Table 1. The superscripts to these quanta represent spin J and parity P. In studying Tables 1 and 2, we note that these mesons fit within the band structure of the CQ model, and yet there are spreads of particles within each band due to the estimates 4 for peak masses and particle widths. A comparison of the CQ model and the particles in Table 1 could be made with the Standard Model. Comparisons to meson nonet membership and to meson fits to Regge theory are possible. However, these comparisons are not in the present scope of this paper and will be presented in a later paper. In this paper, we are concerned with the groupings of the particles in Table 1 and their spreads in energy. In the next section, we introduce quarks (dyons) with electric and magnetic charges into the CQ model, which allows for new dynamical forces in the meson spectrum. These mesons are studied in the CQ model, identifying their groupings or associated states. 2 CQ Model and Russell-Saunders Coupling Mesons are composites of two quarks or quark-antiquark pairs and have been extensively studied as quarkonium and compared to nonrelativistic positronium-like bound states, which are observable as narrow resonances in electron-positron annihilation. If these quark-antiquark states are indeed comparable to atomic-like systems, then it would seem logical that the physics of the atomic scale would be applicable to the particle scale. However, the nature of the quarks would have dramatic effects as well on the physics. In the original CQ model, the quarks were of the Fermi- Yang type not the nucleon quarks of Gell-Mann and Zweig [3].
Recommended publications
  • Magnetic Monopole Searches See the Related Review(S): Magnetic Monopoles
    Citation: P.A. Zyla et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2020, 083C01 (2020) Magnetic Monopole Searches See the related review(s): Magnetic Monopoles Monopole Production Cross Section — Accelerator Searches X-SECT MASS CHG ENERGY (cm2) (GeV) (g) (GeV) BEAM DOCUMENT ID TECN <2.5E−37 200–6000 1 13000 pp 1 ACHARYA 17 INDU <2E−37 200–6000 2 13000 pp 1 ACHARYA 17 INDU <4E−37 200–5000 3 13000 pp 1 ACHARYA 17 INDU <1.5E−36 400–4000 4 13000 pp 1 ACHARYA 17 INDU <7E−36 1000–3000 5 13000 pp 1 ACHARYA 17 INDU <5E−40 200–2500 0.5–2.0 8000 pp 2 AAD 16AB ATLS <2E−37 100–3500 1 8000 pp 3 ACHARYA 16 INDU <2E−37 100–3500 2 8000 pp 3 ACHARYA 16 INDU <6E−37 500–3000 3 8000 pp 3 ACHARYA 16 INDU <7E−36 1000–2000 4 8000 pp 3 ACHARYA 16 INDU <1.6E−38 200–1200 1 7000 pp 4 AAD 12CS ATLS <5E−38 45–102 1 206 e+ e− 5 ABBIENDI 08 OPAL <0.2E−36 200–700 1 1960 p p 6 ABULENCIA 06K CNTR < 2.E−36 1 300 e+ p 7,8 AKTAS 05A INDU < 0.2 E−36 2 300 e+ p 7,8 AKTAS 05A INDU < 0.09E−36 3 300 e+ p 7,8 AKTAS 05A INDU < 0.05E−36 ≥ 6 300 e+ p 7,8 AKTAS 05A INDU < 2.E−36 1 300 e+ p 7,9 AKTAS 05A INDU < 0.2E−36 2 300 e+ p 7,9 AKTAS 05A INDU < 0.07E−36 3 300 e+ p 7,9 AKTAS 05A INDU < 0.06E−36 ≥ 6 300 e+ p 7,9 AKTAS 05A INDU < 0.6E−36 >265 1 1800 p p 10 KALBFLEISCH 04 INDU < 0.2E−36 >355 2 1800 p p 10 KALBFLEISCH 04 INDU < 0.07E−36 >410 3 1800 p p 10 KALBFLEISCH 04 INDU < 0.2E−36 >375 6 1800 p p 10 KALBFLEISCH 04 INDU < 0.7E−36 >295 1 1800 p p 11,12 KALBFLEISCH 00 INDU < 7.8E−36 >260 2 1800 p p 11,12 KALBFLEISCH 00 INDU < 2.3E−36 >325 3 1800 p p 11,13 KALBFLEISCH 00 INDU < 0.11E−36 >420 6 1800 p p 11,13 KALBFLEISCH 00 INDU <0.65E−33 <3.3 ≥ 2 11A 197Au 14,15 HE 97 <1.90E−33 <8.1 ≥ 2 160A 208Pb 14,15 HE 97 <3.E−37 <45.0 1.0 88–94 e+ e− PINFOLD 93 PLAS <3.E−37 <41.6 2.0 88–94 e+ e− PINFOLD 93 PLAS <7.E−35 <44.9 0.2–1.0 89–93 e+ e− KINOSHITA 92 PLAS <2.E−34 <850 ≥ 0.5 1800 p p BERTANI 90 PLAS <1.2E−33 <800 ≥ 1 1800 p p PRICE 90 PLAS <1.E−37 <29 1 50–61 e+ e− KINOSHITA 89 PLAS <1.E−37 <18 2 50–61 e+ e− KINOSHITA 89 PLAS <1.E−38 <17 <1 35 e+ e− BRAUNSCH..
    [Show full text]
  • The Moedal Experiment at the LHC. Searching Beyond the Standard
    126 EPJ Web of Conferences , 02024 (2016) DOI: 10.1051/epjconf/201612602024 ICNFP 2015 The MoEDAL experiment at the LHC Searching beyond the standard model James L. Pinfold (for the MoEDAL Collaboration)1,a 1 University of Alberta, Physics Department, Edmonton, Alberta T6G 0V1, Canada Abstract. MoEDAL is a pioneering experiment designed to search for highly ionizing avatars of new physics such as magnetic monopoles or massive (pseudo-)stable charged particles. Its groundbreaking physics program defines a number of scenarios that yield potentially revolutionary insights into such foundational questions as: are there extra dimensions or new symmetries; what is the mechanism for the generation of mass; does magnetic charge exist; what is the nature of dark matter; and, how did the big-bang develop. MoEDAL’s purpose is to meet such far-reaching challenges at the frontier of the field. The innovative MoEDAL detector employs unconventional methodologies tuned to the prospect of discovery physics. The largely passive MoEDAL detector, deployed at Point 8 on the LHC ring, has a dual nature. First, it acts like a giant camera, comprised of nuclear track detectors - analyzed offline by ultra fast scanning microscopes - sensitive only to new physics. Second, it is uniquely able to trap the particle messengers of physics beyond the Standard Model for further study. MoEDAL’s radiation environment is monitored by a state-of-the-art real-time TimePix pixel detector array. A new MoEDAL sub-detector to extend MoEDAL’s reach to millicharged, minimally ionizing, particles (MMIPs) is under study Finally we shall describe the next step for MoEDAL called Cosmic MoEDAL, where we define a very large high altitude array to take the search for highly ionizing avatars of new physics to higher masses that are available from the cosmos.
    [Show full text]
  • Accelerator Search of the Magnetic Monopo
    Accelerator Based Magnetic Monopole Search Experiments (Overview) Vasily Dzhordzhadze, Praveen Chaudhari∗, Peter Cameron, Nicholas D’Imperio, Veljko Radeka, Pavel Rehak, Margareta Rehak, Sergio Rescia, Yannis Semertzidis, John Sondericker, and Peter Thieberger. Brookhaven National Laboratory ABSTRACT We present an overview of accelerator-based searches for magnetic monopoles and we show why such searches are important for modern particle physics. Possible properties of monopoles are reviewed as well as experimental methods used in the search for them at accelerators. Two types of experimental methods, direct and indirect are discussed. Finally, we describe proposed magnetic monopole search experiments at RHIC and LHC. Content 1. Magnetic Monopole characteristics 2. Experimental techniques 3. Monopole Search experiments 4. Magnetic Monopoles in virtual processes 5. Future experiments 6. Summary 1. Magnetic Monopole characteristics The magnetic monopole puzzle remains one of the fundamental and unsolved problems in physics. This problem has a along history. The military engineer Pierre de Maricourt [1] in1269 was breaking magnets, trying to separate their poles. P. Curie assumed the existence of single magnetic poles [2]. A real breakthrough happened after P. Dirac’s approach to the solution of the electron charge quantization problem [3]. Before Dirac, J. Maxwell postulated his fundamental laws of electrodynamics [4], which represent a complete description of all known classical electromagnetic phenomena. Together with the Lorenz force law and the Newton equations of motion, they describe all the classical dynamics of interacting charged particles and electromagnetic fields. In analogy to electrostatics one can add a magnetic charge, by introducing a magnetic charge density, thus magnetic fields are no longer due solely to the motion of an electric charge and in Maxwell equation a magnetic current will appear in analogy to the electric current.
    [Show full text]
  • Magnetic Monopoles
    Magnetic Monopoles Since Maxwell discovered the unified theory, Maxwell equations, of electric and magnetic forces, people have studied its implications. Maxwell conjectured the electromagnetic wave in his equations to be the light, based on the speed of electromagnetic wave being close to the speed of light. Since Herz and Heaviside, independently, have written the current form of Maxwell’s equations, 1905 Poincare and Einstein independently found the Lorentz transformation which is the property of Maxwell equation. The study of cathode ray has led to the discovery of electrons. The electron orbits are bending around when a magnet was brought near it. By imagining the motion of electron near a tip of a very long solenoid, Poincare introduced a magnetic monopole around which the magnetic field comes out radially. B = gr/r3 1. Consider the motion of a charged particle with equation of motion, m d2r/dt2 = e v x B Find the conserved energy E and the explicit form of the conserved angular momentum J=mr x dr/dt+.… 2. Find the orbit of the charged particle. 3. Consider the motion of two magnetic monopoles appearing in the 4-dim field theory. Magnetic monopoles are characterized by their positions and internal phase angle. The Lagrangian for the relative position r and phase ψ is given as below. where ψ ~ ψ+2π and ∇xw(r)= -r/r3 , and r0 and a are constant positive parameters.. µ r r 1 1 a2 L = 1+ 0 r˙ 2 + r2 1+ 0 − (ψ˙ + w(r) r˙)2 + 0 2 r0 2 r r · 2µr0 1+ r Calling the conserved charge q under the shift symmetry of ψ and the conjugate momentum π of the coordinate r, find the expression for the conserved energy and angular momentum J.
    [Show full text]
  • An Introduction to the Quark Model
    An Introduction to the Quark Model Garth Huber Prairie Universities Physics Seminar Series, November, 2009. Particles in Atomic Physics • View of the particle world as of early 20th Century. • Particles found in atoms: –Electron – Nucleons: •Proton(nucleus of hydrogen) •Neutron(e.g. nucleus of helium – α-particle - has two protons and two neutrons) • Related particle mediating electromagnetic interactions between electrons and protons: Particle Electric charge Mass – Photon (light!) (x 1.6 10-19 C) (GeV=x 1.86 10-27 kg) e −1 0.0005 p +1 0.938 n 0 0.940 γ 0 0 Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 2 Early Evidence for Nucleon Internal Structure • Apply the Correspondence Principle to the Classical relation for q magnetic moment: µ = L 2m • Obtain for a point-like spin-½ particle of mass mp: qqeq⎛⎞⎛⎞ µ == =µ ⎜⎟ ⎜⎟ N 2222memepp⎝⎠ ⎝⎠ 2 Experimental values: µp=2.79 µN (p) µn= -1.91 µN (n) • Experimental values inconsistent with point-like assumption. • In particular, the neutron’s magnetic moment does not vanish, as expected for a point-like electrically neutral particle. This is unequivocal evidence that the neutron (and proton) has an internal structure involving a distribution of charges. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 3 The Particle Zoo • Circa 1950, the first particle accelerators began to uncover many new particles. • Most of these particles are unstable and decay very quickly, and hence had not been seen in cosmic ray experiments. • Could all these particles be fundamental? Dr. Garth Huber, Dept.
    [Show full text]
  • 1 Quark Model of Hadrons
    1 QUARK MODEL OF HADRONS 1 Quark model of hadrons 1.1 Symmetries and evidence for quarks 1 Hadrons as bound states of quarks – point-like spin- 2 objects, charged (‘coloured’) under the strong force. Baryons as qqq combinations. Mesons as qq¯ combinations. 1 Baryon number = 3 (N(q) − N(¯q)) and its conservation. You are not expected to know all of the names of the particles in the baryon and meson multiplets, but you are expected to know that such multiplets exist, and to be able to interpret them if presented with them. You should also know the quark contents of the simple light baryons and mesons (and their anti-particles): p = (uud) n = (udd) π0 = (mixture of uu¯ and dd¯) π+ = (ud¯) K0 = (ds¯) K+ = (us¯). and be able to work out others with some hints. P 1 + Lowest-lying baryons as L = 0 and J = 2 states of qqq. P 3 + Excited versions have L = 0 and J = 2 . Pauli exclusion and non existence of uuu, ddd, sss states in lowest lying multiplet. Lowest-lying mesons as qq¯0 states with L = 0 and J P = 0−. First excited levels (particles) with same quark content have L = 0 and J P = 1−. Ability to explain contents of these multiplets in terms of quarks. J/Ψ as a bound state of cc¯ Υ (upsilon) as a bound state of b¯b. Realization that these are hydrogenic-like states with suitable reduced mass (c.f. positronium), and subject to the strong force, so with energy levels paramaterized by αs rather than αEM Top is very heavy and decays before it can form hadrons, so no top hadrons exist.
    [Show full text]
  • The Structure of Quarks and Leptons
    The Structure of Quarks and Leptons They have been , considered the elementary particles ofmatter, but instead they may consist of still smaller entities confjned within a volume less than a thousandth the size of a proton by Haim Harari n the past 100 years the search for the the quark model that brought relief. In imagination: they suggest a way of I ultimate constituents of matter has the initial formulation of the model all building a complex world out of a few penetrated four layers of structure. hadrons could be explained as combina­ simple parts. All matter has been shown to consist of tions of just three kinds of quarks. atoms. The atom itself has been found Now it is the quarks and leptons Any theory of the elementary particles to have a dense nucleus surrounded by a themselves whose proliferation is begin­ fl. of matter must also take into ac­ cloud of electrons. The nucleus in turn ning to stir interest in the possibility of a count the forces that act between them has been broken down into its compo­ simpler-scheme. Whereas the original and the laws of nature that govern the nent protons and neutrons. More recent­ model had three quarks, there are now forces. Little would be gained in simpli­ ly it has become apparent that the pro­ thought to be at least 18, as well as six fying the spectrum of particles if the ton and the neutron are also composite leptons and a dozen other particles that number of forces and laws were thereby particles; they are made up of the small­ act as carriers of forces.
    [Show full text]
  • 117. Magnetic Monopoles
    1 117. Magnetic Monopoles 117. Magnetic Monopoles Revised August 2019 by D. Milstead (Stockholm U.) and E.J. Weinberg (Columbia U.). 117.1 Theory of magnetic monopoles The symmetry between electric and magnetic fields in the source-free Maxwell’s equations naturally suggests that electric charges might have magnetic counterparts, known as magnetic monopoles. Although the greatest interest has been in the supermassive monopoles that are a firm prediction of all grand unified theories, one cannot exclude the possibility of lighter monopoles. In either case, the magnetic charge is constrained by a quantization condition first found by Dirac [1]. Consider a monopole with magnetic charge QM and a Coulomb magnetic field Q ˆr B = M . (117.1) 4π r2 Any vector potential A whose curl is equal to B must be singular along some line running from the origin to spatial infinity. This Dirac string singularity could potentially be detected through the extra phase that the wavefunction of a particle with electric charge QE would acquire if it moved along a loop encircling the string. For the string to be unobservable, this phase must be a multiple of 2π. Requiring that this be the case for any pair of electric and magnetic charges gives min min the condition that all charges be integer multiples of minimum charges QE and QM obeying min min QE QM = 2π . (117.2) (For monopoles which also carry an electric charge, called dyons [2], the quantization conditions on their electric charges can be modified. However, the constraints on magnetic charges, as well as those on all purely electric particles, will be unchanged.) Another way to understand this result is to note that the conserved orbital angular momentum of a point electric charge moving in the field of a magnetic monopole has an additional component, with L = mr × v − 4πQEQM ˆr (117.3) Requiring the radial component of L to be quantized in half-integer units yields Eq.
    [Show full text]
  • Full-Heavy Tetraquarks in Constituent Quark Models
    Eur. Phys. J. C (2020) 80:1083 https://doi.org/10.1140/epjc/s10052-020-08650-z Regular Article - Theoretical Physics Full-heavy tetraquarks in constituent quark models Xin Jina, Yaoyao Xueb, Hongxia Huangc, Jialun Pingd Department of Physics and Jiangsu Key Laboratory for Numerical Simulation of Large Scale Complex Systems, Nanjing Normal University, Nanjing 210023, People’s Republic of China Received: 4 July 2020 / Accepted: 10 November 2020 / Published online: 23 November 2020 © The Author(s) 2020 Abstract The full-heavy tetraquarks bbb¯b¯ and ccc¯c¯ are [5]. Since then, more and more exotic states were observed systematically investigated within the chiral quark model and proposed, such as Y (4260), Zc(3900), X(5568), and so and the quark delocalization color screening model. Two on. The study of exotic states can help us to understand the structures, meson–meson and diquark–antidiquark, are con- hadron structures and the hadron–hadron interactions better. sidered. For the full-beauty bbb¯b¯ systems, there is no any The full-heavy tetraquark states (QQQ¯ Q¯ , Q = c, b) bound state or resonance state in two structures in the chiral attracted extensive attention for the last few years, since such quark model, while the wide resonances with masses around states with very large energy can be accessed experimentally 19.1 − 19.4 GeV and the quantum numbers J P = 0+,1+, and easily distinguished from other states. In the experiments, and 2+ are possible in the quark delocalization color screen- the CMS collaboration measured pair production of ϒ(1S) ing model. For the full-charm ccc¯c¯ systems, the results are [6].
    [Show full text]
  • Properties of Baryons in the Chiral Quark Model
    Properties of Baryons in the Chiral Quark Model Tommy Ohlsson Teknologie licentiatavhandling Kungliga Tekniska Hogskolan¨ Stockholm 1997 Properties of Baryons in the Chiral Quark Model Tommy Ohlsson Licentiate Dissertation Theoretical Physics Department of Physics Royal Institute of Technology Stockholm, Sweden 1997 Typeset in LATEX Akademisk avhandling f¨or teknologie licentiatexamen (TeknL) inom ¨amnesomr˚adet teoretisk fysik. Scientific thesis for the degree of Licentiate of Engineering (Lic Eng) in the subject area of Theoretical Physics. TRITA-FYS-8026 ISSN 0280-316X ISRN KTH/FYS/TEO/R--97/9--SE ISBN 91-7170-211-3 c Tommy Ohlsson 1997 Printed in Sweden by KTH H¨ogskoletryckeriet, Stockholm 1997 Properties of Baryons in the Chiral Quark Model Tommy Ohlsson Teoretisk fysik, Institutionen f¨or fysik, Kungliga Tekniska H¨ogskolan SE-100 44 Stockholm SWEDEN E-mail: [email protected] Abstract In this thesis, several properties of baryons are studied using the chiral quark model. The chiral quark model is a theory which can be used to describe low energy phenomena of baryons. In Paper 1, the chiral quark model is studied using wave functions with configuration mixing. This study is motivated by the fact that the chiral quark model cannot otherwise break the Coleman–Glashow sum-rule for the magnetic moments of the octet baryons, which is experimentally broken by about ten standard deviations. Configuration mixing with quark-diquark components is also able to reproduce the octet baryon magnetic moments very accurately. In Paper 2, the chiral quark model is used to calculate the decuplet baryon ++ magnetic moments. The values for the magnetic moments of the ∆ and Ω− are in good agreement with the experimental results.
    [Show full text]
  • 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]