Transverse–Spin Quark Distributions from Asymmetry Data and Symmetry Arguments
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Followed by a Stretcher That Fits Into the Same
as the booster; the main synchro what cheaper because some ex tunnel (this would require comple tron taking the beam to the final penditure on buildings and general mentary funding beyond the normal energy; followed by a stretcher infrastructure would be saved. CERN budget); and at the Swiss that fits into the same tunnel as In his concluding remarks, SIN Laboratory. Finally he pointed the main ring of circumference 960 F. Scheck of Mainz, chairman of out that it was really one large m (any resemblance to existing the EHF Study Group, pointed out community of future users, not presently empty tunnels is not that the physics case for EHF was three, who were pushing for a unintentional). Bradamante pointed well demonstrated, that there was 'kaon factory'. Whoever would be out that earlier criticisms are no a strong and competent European first to obtain approval, the others longer valid. The price seems un physics community pushing for it, would beat a path to his door. der control, the total investment and that there were good reasons National decisions on the project for a 'green pasture' version for building it in Europe. He also will be taken this year. amounting to about 870 million described three site options: a Deutschmarks. A version using 'green pasture' version in Italy; at By Florian Scheck existing facilities would be some- CERN using the now defunct ISR A ZEUS group meeting, with spokesman Gunter Wolf one step in front of the pack. (Photo DESY) The HERA electron-proton collider now being built at the German DESY Laboratory in Hamburg will be a unique physics tool. -
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. -
Estimation of Baryon Asymmetry of the Universe from Neutrino Physics
ESTIMATION OF BARYON ASYMMETRY OF THE UNIVERSE FROM NEUTRINO PHYSICS Manorama Bora Department of Physics Gauhati University This thesis is submitted to Gauhati University as requirement for the degree of Doctor of Philosophy Faculty of Science March 2018 I would like to dedicate this thesis to my parents . Abstract The discovery of neutrino masses and mixing in neutrino oscillation experiments in 1998 has greatly increased the interest in a mechanism of baryogenesis through leptogenesis, a model of baryogenesis which is a cosmological consequence. The most popular way to explain why neutrinos are massive but at the same time much lighter than all other fermions, is the see-saw mechanism. Thus, leptogenesis realises a highly non-trivial link between two completely independent experimental observations: the absence of antimatter in the observable universe and the observation of neutrino mixings and masses. Therefore, leptogenesis has a built-in double sided nature.. The discovery of Higgs boson of mass 125GeV having properties consistent with the SM, further supports the leptogenesis mechanism. In this thesis we present a brief sketch on the phenomenological status of Standard Model (SM) and its extension to GUT with or without SUSY. Then we review on neutrino oscillation and its implication with latest experiments. We discuss baryogenesis via leptogenesis through the decay of heavy Majorana neutrinos. We also discuss formulation of thermal leptogenesis. At last we try to explore the possibilities for the discrimination of the six kinds of Quasi- degenerate neutrino(QDN)mass models in the light of baryogenesis via leptogenesis. We have seen that all the six QDN mass models are relevant in the context of flavoured leptogenesis. -
An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders
416 Brazilian Journal of Physics, vol. 38, no. 3B, September, 2008 An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders M. V. T. Machado Universidade Federal do Pampa, Centro de Cienciasˆ Exatas e Tecnologicas´ Campus de Bage,´ Rua Carlos Barbosa, CEP 96400-970, Bage,´ RS, Brazil (Received on 20 March, 2008) In this contribution results from a phenomenological analysis for the diffractive hadroproduction of heavy flavors at high energies are reported. Diffractive production of charm, bottom and top are calculated using the Regge factorization, taking into account recent experimental determination of the diffractive parton density functions in Pomeron by the H1 Collaboration at DESY-HERA. In addition, multiple-Pomeron corrections are considered through the rapidity gap survival probability factor. We give numerical predictions for single diffrac- tive as well as double Pomeron exchange (DPE) cross sections, which agree with the available data for diffractive production of charm and beauty. We make estimates which could be compared to future measurements at the LHC. Keywords: Heavy flavour production; Pomeron physics; Single diffraction; Quantum Chromodynamics 1. INTRODUCTION the diffractive quarkonium production, which is now sensitive to the gluon content of the Pomeron at small-x and may be For a long time, diffractive processes in hadron collisions particularly useful in studying the different mechanisms for have been described by Regge theory in terms of the exchange quarkonium production. of a Pomeron with vacuum quantum numbers [1]. However, the nature of the Pomeron and its reaction mechanisms are In order to do so, we will use the hard diffractive factoriza- not completely known. -
The Matter – Antimatter Asymmetry of the Universe and Baryogenesis
The matter – antimatter asymmetry of the universe and baryogenesis Andrew Long Lecture for KICP Cosmology Class Feb 16, 2017 Baryogenesis Reviews in General • Kolb & Wolfram’s Baryon Number Genera.on in the Early Universe (1979) • Rio5o's Theories of Baryogenesis [hep-ph/9807454]} (emphasis on GUT-BG and EW-BG) • Rio5o & Trodden's Recent Progress in Baryogenesis [hep-ph/9901362] (touches on EWBG, GUTBG, and ADBG) • Dine & Kusenko The Origin of the Ma?er-An.ma?er Asymmetry [hep-ph/ 0303065] (emphasis on Affleck-Dine BG) • Cline's Baryogenesis [hep-ph/0609145] (emphasis on EW-BG; cartoons!) Leptogenesis Reviews • Buchmuller, Di Bari, & Plumacher’s Leptogenesis for PeDestrians, [hep-ph/ 0401240] • Buchmulcer, Peccei, & Yanagida's Leptogenesis as the Origin of Ma?er, [hep-ph/ 0502169] Electroweak Baryogenesis Reviews • Cohen, Kaplan, & Nelson's Progress in Electroweak Baryogenesis, [hep-ph/ 9302210] • Trodden's Electroweak Baryogenesis, [hep-ph/9803479] • Petropoulos's Baryogenesis at the Electroweak Phase Transi.on, [hep-ph/ 0304275] • Morrissey & Ramsey-Musolf Electroweak Baryogenesis, [hep-ph/1206.2942] • Konstandin's Quantum Transport anD Electroweak Baryogenesis, [hep-ph/ 1302.6713] Constituents of the Universe formaon of large scale structure (galaxy clusters) stars, planets, dust, people late ame accelerated expansion Image stolen from the Planck website What does “ordinary matter” refer to? Let’s break it down to elementary particles & compare number densities … electron equal, universe is neutral proton x10 billion 3⇣(3) 3 3 n =3 T 168 cm− neutron x7 ⌫ ⇥ 4⇡2 ⌫ ' matter neutrinos photon positron =0 2⇣(3) 3 3 n = T 413 cm− γ ⇡2 CMB ' anti-proton =0 3⇣(3) 3 3 anti-neutron =0 n =3 T 168 cm− ⌫¯ ⇥ 4⇡2 ⌫ ' anti-neutrinos antimatter What is antimatter? First predicted by Dirac (1928). -
A New Avenue to Parton Distribution Functions Uncertainties: Self-Organizing Maps Abstract
A New Avenue to Parton Distribution Functions Uncertainties: Self-Organizing Maps Abstract Neural network algorithms have been recently applied to construct Parton Distribution Functions (PDFs) parametrizations as an alternative to standard global fitting procedures. We propose a different technique, namely an interactive neural network algorithm using Self-Organizing Maps (SOMs). SOMs enable the user to directly control the data selection procedure at various stages of the process. We use all available data on deep inelastic scattering experiments in the kinematical region of 0:001 ≤ x ≤ 0:75, and 1 ≤ Q2 ≤ 100 GeV2, with a cut on the final state invariant mass, W 2 ≥ 10 GeV2. Our main goal is to provide a fitting procedure that, at variance with standard neural network approaches, allows for an increased control of the systematic bias. Controlling the theoretical uncertainties is crucial for determining the outcome of a variety of high energy physics experiments using hadron beams. In particular, it is a prerequisite for unambigously extracting from experimental data the signal of the Higgs boson, that is considered to be, at present, the key for determining the theory of the masses of all known elementary particles, or the Holy Grail of particle physics. PACS numbers: 13.60.-r, 12.38.-t, 24.85.+p 1 I. DEFINITION OF THE PROBLEM AND GENERAL REMARKS In high energy physics experiments one detects the cross section, σX , for observing a particle X during a given collision process. σX is proportional to the number of counts in the detector. It is, therefore, directly \observable". Consider the collision between two hadrons (a hadron is a more general name to indicate a proton, neutron...or a more exotic particle made of quarks). -
Collider Physics at HERA
ANL-HEP-PR-08-23 Collider Physics at HERA M. Klein1, R. Yoshida2 1University of Liverpool, Physics Department, L69 7ZE, Liverpool, United Kingdom 2Argonne National Laboratory, HEP Division, 9700 South Cass Avenue, Argonne, Illinois, 60439, USA May 21, 2008 Abstract From 1992 to 2007, HERA, the first electron-proton collider, operated at cms energies of about 320 GeV and allowed the investigation of deep-inelastic and photoproduction processes at the highest energy scales accessed thus far. This review is an introduction to, and a summary of, the main results obtained at HERA during its operation. To be published in Progress in Particle and Nuclear Physics arXiv:0805.3334v1 [hep-ex] 21 May 2008 1 Contents 1 Introduction 4 2 Accelerator and Detectors 5 2.1 Introduction.................................... ...... 5 2.2 Accelerator ..................................... ..... 6 2.3 Deep Inelastic Scattering Kinematics . ............. 9 2.4 Detectors ....................................... .... 12 3 Proton Structure Functions 15 3.1 Introduction.................................... ...... 15 3.2 Structure Functions and Parton Distributions . ............... 16 3.3 Measurement Techniques . ........ 18 3.4 Low Q2 and x Results .................................... 19 2 3.4.1 The Discovery of the Rise of F2(x, Q )....................... 19 3.4.2 Remarks on Low x Physics.............................. 20 3.4.3 The Longitudinal Structure Function . .......... 22 3.5 High Q2 Results ....................................... 23 4 QCD Fits 25 4.1 Introduction.................................... ...... 25 4.2 Determinations ofParton Distributions . .............. 26 4.2.1 TheZEUSApproach ............................... .. 27 4.2.2 TheH1Approach................................. .. 28 4.3 Measurements of αs inInclusiveDIS ............................ 29 5 Jet Measurements 32 5.1 TheoreticalConsiderations . ........... 32 5.2 Jet Cross-Section Measurements . ........... 34 5.3 Tests of pQCD and Determination of αs ......................... -
Deep Inelastic Scattering
Particle Physics Michaelmas Term 2011 Prof Mark Thomson e– p Handout 6 : Deep Inelastic Scattering Prof. M.A. Thomson Michaelmas 2011 176 e– p Elastic Scattering at Very High q2 ,At high q2 the Rosenbluth expression for elastic scattering becomes •From e– p elastic scattering, the proton magnetic form factor is at high q2 Phys. Rev. Lett. 23 (1969) 935 •Due to the finite proton size, elastic scattering M.Breidenbach et al., at high q2 is unlikely and inelastic reactions where the proton breaks up dominate. e– e– q p X Prof. M.A. Thomson Michaelmas 2011 177 Kinematics of Inelastic Scattering e– •For inelastic scattering the mass of the final state hadronic system is no longer the proton mass, M e– •The final state hadronic system must q contain at least one baryon which implies the final state invariant mass MX > M p X For inelastic scattering introduce four new kinematic variables: ,Define: Bjorken x (Lorentz Invariant) where •Here Note: in many text books W is often used in place of MX Proton intact hence inelastic elastic Prof. M.A. Thomson Michaelmas 2011 178 ,Define: e– (Lorentz Invariant) e– •In the Lab. Frame: q p X So y is the fractional energy loss of the incoming particle •In the C.o.M. Frame (neglecting the electron and proton masses): for ,Finally Define: (Lorentz Invariant) •In the Lab. Frame: is the energy lost by the incoming particle Prof. M.A. Thomson Michaelmas 2011 179 Relationships between Kinematic Variables •Can rewrite the new kinematic variables in terms of the squared centre-of-mass energy, s, for the electron-proton collision e– p Neglect mass of electron •For a fixed centre-of-mass energy, it can then be shown that the four kinematic variables are not independent. -
Introduction to Flavour Physics
Introduction to flavour physics Y. Grossman Cornell University, Ithaca, NY 14853, USA Abstract In this set of lectures we cover the very basics of flavour physics. The lec- tures are aimed to be an entry point to the subject of flavour physics. A lot of problems are provided in the hope of making the manuscript a self-study guide. 1 Welcome statement My plan for these lectures is to introduce you to the very basics of flavour physics. After the lectures I hope you will have enough knowledge and, more importantly, enough curiosity, and you will go on and learn more about the subject. These are lecture notes and are not meant to be a review. In the lectures, I try to talk about the basic ideas, hoping to give a clear picture of the physics. Thus many details are omitted, implicit assumptions are made, and no references are given. Yet details are important: after you go over the current lecture notes once or twice, I hope you will feel the need for more. Then it will be the time to turn to the many reviews [1–10] and books [11, 12] on the subject. I try to include many homework problems for the reader to solve, much more than what I gave in the actual lectures. If you would like to learn the material, I think that the problems provided are the way to start. They force you to fully understand the issues and apply your knowledge to new situations. The problems are given at the end of each section. -
Outline of Lecture 2 Baryon Asymmetry of the Universe. What's
Outline of Lecture 2 Baryon asymmetry of the Universe. What’s the problem? Electroweak baryogenesis. Electroweak baryon number violation Electroweak transition What can make electroweak mechanism work? Dark energy Baryon asymmetry of the Universe There is matter and no antimatter in the present Universe. Baryon-to-photon ratio, almost constant in time: nB 10 ηB = 6 10− ≡ nγ · Baryon-to-entropy, constant in time: n /s = 0.9 10 10 B · − What’s the problem? Early Universe (T > 1012 K = 100 MeV): creation and annihilation of quark-antiquark pairs ⇒ n ,n n q q¯ ≈ γ Hence nq nq¯ 9 − 10− nq + nq¯ ∼ How was this excess generated in the course of the cosmological evolution? Sakharov conditions To generate baryon asymmetry, three necessary conditions should be met at the same cosmological epoch: B-violation C-andCP-violation Thermal inequilibrium NB. Reservation: L-violation with B-conservation at T 100 GeV would do as well = Leptogenesis. & ⇒ Can baryon asymmetry be due to electroweak physics? Baryon number is violated in electroweak interactions. Non-perturbative effect Hint: triangle anomaly in baryonic current Bµ : 2 µ 1 gW µνλρ a a ∂ B = 3colors 3generations ε F F µ 3 · · · 32π2 µν λρ ! "Bq a Fµν: SU(2)W field strength; gW : SU(2)W coupling Likewise, each leptonic current (n = e, µ,τ) g2 ∂ Lµ = W ε µνλρFa Fa µ n 32π2 · µν λρ a 1 Large field fluctuations, Fµν ∝ gW− may have g2 Q d3xdt W ε µνλρFa Fa = 0 ≡ 32 2 · µν λρ ' # π Then B B = d3xdt ∂ Bµ =3Q fin− in µ # Likewise L L =Q n, fin− n, in B is violated, B L is not. -
Redalyc.An Analysis on Single and Central Diffractive Heavy Flavour
Brazilian Journal of Physics ISSN: 0103-9733 [email protected] Sociedade Brasileira de Física Brasil Machado, M. V. T. An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders Brazilian Journal of Physics, vol. 38, núm. 3B, septiembre, 2008, pp. 416-420 Sociedade Brasileira de Física Sâo Paulo, Brasil Available in: http://www.redalyc.org/articulo.oa?id=46415795006 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative 416 Brazilian Journal of Physics, vol. 38, no. 3B, September, 2008 An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders M. V. T. Machado Universidade Federal do Pampa, Centro de Cienciasˆ Exatas e Tecnologicas´ Campus de Bage,´ Rua Carlos Barbosa, CEP 96400-970, Bage,´ RS, Brazil (Received on 20 March, 2008) In this contribution results from a phenomenological analysis for the diffractive hadroproduction of heavy flavors at high energies are reported. Diffractive production of charm, bottom and top are calculated using the Regge factorization, taking into account recent experimental determination of the diffractive parton density functions in Pomeron by the H1 Collaboration at DESY-HERA. In addition, multiple-Pomeron corrections are considered through the rapidity gap survival probability factor. We give numerical predictions for single diffrac- tive as well as double Pomeron exchange (DPE) cross sections, which agree with the available data for diffractive production of charm and beauty. We make estimates which could be compared to future measurements at the LHC. -
First Measurement of the Charge Asymmetry in Beauty-Quark Pair Production at a Hadron Collider
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN) CERN-PH-EP-2014-130 LHCb-PAPER-2014-023 September 10, 2014 First measurement of the charge asymmetry in beauty-quark pair production at a hadron collider The LHCb collaborationy Abstract The difference in the angular distributions between beauty quarks and antiquarks, referred to as the charge asymmetry, is measured for the first time in bb pair production at a hadron collider. The data used correspond to an integrated luminosity of 1.0 fb−1 collected at 7 TeV center-of-mass energy in proton-proton collisions with the LHCb detector. The measurement is performed in three regions of the invariant mass of the bb system. The results obtained are b¯b 2 AC (40 < Mb¯b < 75 GeV=c ) = 0:4 ± 0:4 (stat) ± 0:3 (syst)%; b¯b 2 AC (75 < Mb¯b < 105 GeV=c ) = 2:0 ± 0:9 (stat) ± 0:6 (syst)%; b¯b 2 AC (Mb¯b > 105 GeV=c ) = 1:6 ± 1:7 (stat) ± 0:6 (syst)%; b¯b where AC is defined as the asymmetry in the difference in rapidity between jets formed from the beauty quark and antiquark. The beauty jets are required to satisfy 2 < η < 4, ET > 20 GeV, and have an opening angle in the transverse plane ∆φ > 2:6 rad. These measurements are arXiv:1406.4789v2 [hep-ex] 13 Sep 2014 consistent with the predictions of the Standard Model. c CERN on behalf of the LHCb collaboration, license CC-BY-3.0. yAuthors are listed on the following pages. ii LHCb collaboration R.