The Large Hadron Collider (LHC)

Total Page:16

File Type:pdf, Size:1020Kb

The Large Hadron Collider (LHC) The Large Hadron Collider (LHC) Benjamin Radburn-Smith RAL Particle Physics • Aim to understand the laws of physics at a fundamental level • Use subatomic particles to probe this domain – Protons, antiprotons, lead ions, neutrinos, neutrons, muons • Use high energy machines for our experiments… Size! • Size matters – Higher energy Shorter wavelength probe smaller scales • Electron discovered – J.J. Thomson (Cambridge, 1897) Size! • Antiproton (1955 )and Antineutron (1956) discovered – Bevatron 6.5 GeV proton accelerator (Berkley, USA) Accelerator: Large Hadron Collider Accelerator: Large Hadron Collider • Accelerates bunches of proton to 99.9999991% the speed of light, so they circulate 11 245 times/s Accelerator: Large Hadron Collider • 700 million proton-proton collisions per second at CMS/ATLAS The SM • We have constructed a theory of how the Universe works on the smallest scales • This theory of particle physics is called the Standard Model (SM) • Explains particles and the forces that act between them – Has produced predictions which agrees with experimental data to unprecedented accuracy! – It has been correct for decades – … but ? The SM • There are a few problems with the SM: – It doesn’t explain Dark Matter or Dark Energy … i.e. 96% of the Universe – It doesn’t explain gravity (SM explains the world of the small scale where gravity is negligible) – Does it account for mass? – How does the Universe exist? Matter/Antimatter – There are inconsistencies at higher energies (we are still dealing with energies which are relatively low) – A number of free parameters – Different mass scales Designed and constructed the LHC to investigate these problems The BEH Mechanism • In the SM, forces are mediated by particles ( , , , ) – The mathematics only works if some of these are massless: ( , ) but they are heavy! • Brout, Englert and Higgs (and others) introduced a theory: The BEH mechanism – Massive particles appear massive due to some background interaction? – The force carrier is the Higgs particle ( ) "It's an energy field created by all living things. It surrounds us and penetrates us; it binds the galaxy together.” The BEH Mechanism • In the SM, forces are mediated by particles ( , , , ) – The mathematics only works if some of these are massless: ( , ) but they are heavy! • Brout, Englert and Higgs (and others) introduced a theory: The BEH mechanism – Massive particles appear massive due to some background interaction? – The force carrier is the Higgs particle ( ) "It's an energy field created by all living things. It surrounds us and penetrates us; it binds the galaxy together.” - Obi Wan-Kenobi The BEH Mechanism: Analogy • Cocktail Party: Room full of people represents Famous person is then surrounded space filled with the Higgs field by people creating a resistance, which represents a heavy particle interacting with the Higgs field • The Higgs Boson is a quantum of this field! Finding the Higgs • If the Higgs field exists, then we expect to find the Higgs Boson • The Higgs is predicted to decay into certain combination of particles, e.g. – Higgs to photons – Higgs to leptons Why the LHC? • Search for new things! • Find the Higgs Bosons? • New particles at higher energies? • Black holes? • Supersymmetry (SUSY: doubles the number of particles and solves many problems)? • Extra dimensions? Why the LHC? • Search for new things! • Find the Higgs Bosons? • New particles at higher energies? • Black holes? • Supersymmetry (SUSY: doubles the number of particles and solves many problems)? • Extra dimensions? • Something we didn’t think about? • How does the LHC work? • How do the experiments work? • How do we get data? • How do we turn the data into information? How does the LHC work? • Objective: Smash protons into each other with enormous energy and study the debris that results • LHC is part of the CERN accelerator complex Accelerator Complex • Use a bottle of hydrogen for the source of protons, by injecting them into a duoplasmatron and ripping off the the electrons – Need lots: 2 beams of around 3000 bunches each containing around 100 billion protons • These protons are then accelerated using a Linear accelerator to 50 MeV • Then accelerated by the Proton Synchrotron Booster to 1.4 GeV Accelerator Complex • The Proton Synchrotron accelerates the protons to 25 GeV • The Super Proton Synchrotron accelerates the protons to 450 GeV • This then feeds the LHC in both directions Movie: http://cds.cern.ch/record/1228924 What is the LHC? • Holds two beams of protons in a vacuum pipes – To stop them from interacting with any dust particles – LHC: 1/10 000 000 000 000th of atmospheric pressure! – (better vacuum than space around the ISS) • These protons are then accelerated using RF cavities – To kinetic energies of a proton beam equal to the Eurostar at around 100 mph! • Need get the beams to repeatedly pass through the accelerating cavities (taking ~20mins to get up to energy) • For this we need strong magnets! What is the LHC? • Contains a total of ~9300 magnets – With 1232 large 15m long cryodipole magnets to steer the beams Strong magnets require huge currents need superconducting magnets! LHC is the largest fridge on the planet! 6000 tons kept at -271°C Corresponds to ~150 000 household fridges at a temperature colder than the coldest regions of space What is the LHC? • The LHC takes protons from the SPS with 2808 bunches per beam and 1011 protons per bunch • Accelerates them up to (4) 7 TeV per beam • Collides the beams at 4 places around the ring • Then dumps the beams into large carbon/steel cylinders • ~30 collisions every 50 ns • Need huge numbers of collisions to analyse the rare ones Movie: https://cds.cern.ch/record/1406040 But what about the Moon?! • We need accurately control the position of the protons in the pipe – to collide the micrometer size beams head on inside a kilometer scaled machine – Extremely precise beam position monitoring and feedback system • LHC is sensitive to the location of the Moon! – Through ground (25 cm) and water tides – Varies the circumference by 1 mm • LEP used to be sensitive to the TGV! 4 Main Experiments • ATLAS (general purpose) – 7000 tons, 25 m diameter, 46 m length • CMS (general purpose) – 14500 tons, 15 m diameter, 22 m length 4 Main Experiments • LHCb (b physics) – 5600 tons, 13 m width, 21 m length • ALICE (heavy ion physics) – 10000 tons, 16 m diameter, 26 m length (No RAL involvement) Who runs it? • We are an international bunch! Officially (roughly) – ATLAS: 35 countries – CMS: 40 countries – LHCb: 15 countries – ALICE: 30 countires How do we run the machines? • With computers in control centres How do we run the machines? • With computers in control centres Angels and Demons How do we run the machines? • With computers in control centres CMS ATLAS FNAL LHC Role of the Experiments • The LHC smashes the protons (quarks & gluons) together • This produces interesting massive particles • These decay almost immediately • Decay products fly off in all directions • Intercept and analyse these with detectors • Attempt to reconstruct the interesting part of the event using computers and our brains! What we detect • Most interesting particles decay almost immediately What we detect • Most interesting particles decay almost immediately – Can’t see these What we detect • Most interesting particles decay almost immediately – Difficult to see these Never appear isolated: produce whole bundles of protons, neutrons, mesons etc (jet) What we detect • Most interesting particles decay almost immediately – Can’t see these Never appear isolated: produce whole bundles of protons, neutrons, mesons etc (jet) Undetectable here How to detect particles • Tracking • Charged particles ionise the material they pass through – Use a small amount of material to detect the ionisation charges left find the position • Then use many layers to follow the path of the charged particles • Typically we use silicon for this job – Similar to your camera sensors – However these are quite thin, high resolution and radiation hard How to detect particles • Tracking trick! • Remember that charged particles bend in a magnetic field – Immerse the silicon detectors in a magnetic field – Path of the particle is bent – We can then calculate the momentum of the particles • However: we are dealing with particles with high energies – Small curvature – Need large tracking detectors (approx meters) – High spatial resolution (to a few micrometers) How to detect particles • Tracking works for charged particles, but not for neutrals • Use calorimeters: – Large amounts of material which absorb the energies of the particles (as the particles interact with the material) – This creates showers of secondary particles • Absorbers: stop the particles (kinetic energy into showers) • Detectors: measure the shower energies • Derive the energy and position of the initial particle from the properties of the showers How to detect particles • 2 main classes of calorimeters: • Electromagnetic – Absorption via electromagnetic cascade of lightweight particles (electrons, photons) • Hadronic – Nuclear interaction with absorber material (for protons, neutrons, mesons etc) – As we are dealing with high energy: need lots of material e.g. few meters thick using dense material (lead, iron, uranium) How to detect particles • Muons – Are a special case: they are almost unstoppable – Need specific muon detectors to find them – E.g. CMS uses iron absorbers to stop any other particles from reaching the muon detectors, which work in a similar way to tracker
Recommended publications
  • Proton Driven Plasma Wakefield Acceleration in AWAKE
    Proton Driven Plasma Article submitted to journal Wakefield Acceleration in Subject Areas: AWAKE Plasma Wakefield Acceleration, 1 1 Proton Driven, Electron Acceleration E. Gschwendtner , M. Turner , **Author List Continues Next Page** Keywords: AWAKE, Plasma Wakefield Acceleration, Seeded Self Modulation In this article, we briefly summarize the experiments Author for correspondence: performed during the first Run of the Advanced Insert corresponding author name Wakefield Experiment, AWAKE, at CERN (European e-mail: [email protected] Organization for Nuclear Research). The final goal of AWAKE Run 1 (2013 - 2018) was to demonstrate that 10-20 MeV electrons can be accelerated to GeV- energies in a plasma wakefield driven by a highly- relativistic self-modulated proton bunch. We describe the experiment, outline the measurement concept and present first results. Last, we outline our plans for the future. 1 Continued Author List 2 E. Adli2,A. Ahuja1,O. Apsimon3;4,R. Apsimon3;4, A.-M. Bachmann1;5;6,F. Batsch1;5;6 C. Bracco1,F. Braunmüller5,S. Burger1,G. Burt7;4, B. Buttenschön8,A. Caldwell5,J. Chappell9, E. Chevallay1,M. Chung10,D. Cooke9,H. Damerau1, L.H. Deubner11,A. Dexter7;4,S. Doebert1, J. Farmer12, V.N. Fedosseev1,R. Fiorito13;4,R.A. Fonseca14,L. Garolfi1,S. Gessner1, B. Goddard1, I. Gorgisyan1,A.A. Gorn15;16,E. Granados1,O. Grulke8;17, A. Hartin9,A. Helm18, J.R. Henderson7;4,M. Hüther5, M. Ibison13;4,S. Jolly9,F. Keeble9,M.D. Kelisani1, S.-Y. Kim10, F. Kraus11,M. Krupa1, T. Lefevre1,Y. Li3;4,S. Liu19,N. Lopes18,K.V. Lotov15;16, M. Martyanov5, S.
    [Show full text]
  • The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland
    34th SLAC Summer Institute On Particle Physics (SSI 2006), July 17-28, 2006 The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland 1. INTRODUCTION The Large Hadron Collider (LHC) at CERN is now in its final installation and commissioning phase. It is a two-ring superconducting proton-proton collider housed in the 27 km tunnel previously constructed for the Large Electron Positron collider (LEP). It is designed to provide proton-proton collisions with unprecedented luminosity (1034cm-2.s-1) and a centre-of-mass energy of 14 TeV for the study of rare events such as the production of the Higgs particle if it exists. In order to reach the required energy in the existing tunnel, the dipoles must operate at 1.9 K in superfluid helium. In addition to p-p operation, the LHC will be able to collide heavy nuclei (Pb-Pb) with a centre-of-mass energy of 1150 TeV (2.76 TeV/u and 7 TeV per charge). By modifying the existing obsolete antiproton ring (LEAR) into an ion accumulator (LEIR) in which electron cooling is applied, the luminosity can reach 1027cm-2.s-1. The LHC presents many innovative features and a number of challenges which push the art of safely manipulating intense proton beams to extreme limits. The beams are injected into the LHC from the existing Super Proton Synchrotron (SPS) at an energy of 450 GeV. After the two rings are filled, the machine is ramped to its nominal energy of 7 TeV over about 28 minutes. In order to reach this energy, the dipole field must reach the unprecedented level for accelerator magnets of 8.3 T.
    [Show full text]
  • Remembering Alvin Tollestrup: 1924-2020 – CERN Courier
    3/26/2020 Remembering Alvin Tollestrup: 1924-2020 – CERN Courier PEOPLE | NEWS Remembering Alvin Tollestrup: 1924-2020 6 March 2020 Alvin Tollestrup, who passed away on 9 February at the age of 95, was a visionary. When I joined his group at Caltech in the summer of 1960, experiments in particle physics at universities were performed at accelerators located on campus. Alvin had helped build Caltech’s electron synchrotron, the highest energy photon-producing accelerator at the time. But he thought more exciting physics could be performed elsewhere, and managed to get approval to run an experiment at Berkeley Lab’s Bevatron to measure a rare decay mode of the K+ meson. This was the rst time an outsider was allowed to access Berkeley’s machine, much to the consternation of Luis Alvarez and other university faculty. When I joined Alvin’s group he asked a postdoc, Ricardo Gomez, and me to design, build and test https://cerncourier.com/a/remembering-alvin-tollestrup-1924-2020/ 1/5 3/26/2020 Remembering Alvin Tollestrup: 1924-2020 – CERN Courier Machine maestro – Alvin Tollestrup led the pioneering a new type of particle detector called a spark work of designing and testing the superconducting magnets for the Tevatron, the rst large-scale chamber. He gave us a paper by two Japanese application of superconductivity. Credit: Fermilab authors on “A new type of particle detector: the discharge chamber”, not what he wanted, but a place to start. In retrospect it was remarkable that Alvin was willing to risk the success of his experiment on the creation of new technology.
    [Show full text]
  • Il Nostro Mondo
    IL NOSTRO MONDO THE DESIGN, CONSTRUCTION AND PERFORMANCE OF THE CERN INTERSECTING STORAGE RINGS (ISR) A RECOLLECTION OF WORLD’S FIRST PROTON-PROTON COLLIDER KURT HÜBNER CERN, Geneva, Switzerland 1 Design which had a beam energy of 160 MeV. The interaction points to increase the collision rate The concept of colliding beams appeared design of these colliders started in 1957. but without special lattice insertions as one first in a German patent by Rolf Widerøe In 1961, the Accelerator Research Group would use these days. registered in 1943 and published in 1952. Division was expanded into the Accelerator Combined-function magnets were chosen However, at that time the intensity of beams Division as experienced manpower had as in the PS, i.e. the main magnets had a was too low for an exploitable collision rate as become available after the running-in of the magnetic dipole field to bend the beam and a beam accumulation had not yet been invented. PS in 1960. At the same time it was decided quadrupole field to focus the beam. This type The first ideas of a realistic design were to construct a small accelerator to test rf of magnet provided space for the elaborate published in 1956 by Gerard O’Neill and by the stacking, a technique to be experimentally pole-face windings foreseen to control the MURA Group lead by Donald Kerst in the USA. proven, as it was essential for the performance magnetic field to a very high precision. It also MURA had come up with beam accumulation and success of the ISR.
    [Show full text]
  • ANTIMATTER a Review of Its Role in the Universe and Its Applications
    A review of its role in the ANTIMATTER universe and its applications THE DISCOVERY OF NATURE’S SYMMETRIES ntimatter plays an intrinsic role in our Aunderstanding of the subatomic world THE UNIVERSE THROUGH THE LOOKING-GLASS C.D. Anderson, Anderson, Emilio VisualSegrè Archives C.D. The beginning of the 20th century or vice versa, it absorbed or emitted saw a cascade of brilliant insights into quanta of electromagnetic radiation the nature of matter and energy. The of definite energy, giving rise to a first was Max Planck’s realisation that characteristic spectrum of bright or energy (in the form of electromagnetic dark lines at specific wavelengths. radiation i.e. light) had discrete values The Austrian physicist, Erwin – it was quantised. The second was Schrödinger laid down a more precise that energy and mass were equivalent, mathematical formulation of this as described by Einstein’s special behaviour based on wave theory and theory of relativity and his iconic probability – quantum mechanics. The first image of a positron track found in cosmic rays equation, E = mc2, where c is the The Schrödinger wave equation could speed of light in a vacuum; the theory predict the spectrum of the simplest or positron; when an electron also predicted that objects behave atom, hydrogen, which consists of met a positron, they would annihilate somewhat differently when moving a single electron orbiting a positive according to Einstein’s equation, proton. However, the spectrum generating two gamma rays in the featured additional lines that were not process. The concept of antimatter explained. In 1928, the British physicist was born.
    [Show full text]
  • Anomalous Muon Magnetic Moment, Supersymmetry, Naturalness, LHC Search Limits and the Landscape
    OU-HEP-210415 Anomalous muon magnetic moment, supersymmetry, naturalness, LHC search limits and the landscape Howard Baer1∗, Vernon Barger2†, Hasan Serce1‡ 1Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA 2Department of Physics, University of Wisconsin, Madison, WI 53706 USA Abstract The recent measurement of the muon anomalous magnetic moment aµ ≡ (g − 2)µ=2 by the Fermilab Muon g − 2 experiment sharpens an earlier discrepancy between theory and the BNL E821 experiment. We examine the predicted ∆aµ ≡ aµ(exp) − aµ(th) in the context of supersymmetry with low electroweak naturalness (restricting to models which give a plausible explanation for the magnitude of the weak scale). A global analy- sis including LHC Higgs mass and sparticle search limits points to interpretation within the normal scalar mass hierarchy (NSMH) SUSY model wherein first/second generation matter scalars are much lighter than third generation scalars. We present a benchmark model for a viable NSMH point which is natural, obeys LHC Higgs and sparticle mass constraints and explains the muon magnetic anomaly. Aside from NSMH models, then we find the (g − 2)µ anomaly cannot be explained within the context of natural SUSY, where a variety of data point to decoupled first/second generation scalars. The situation is worse within the string landscape where first/second generation matter scalars are pulled arXiv:2104.07597v2 [hep-ph] 16 May 2021 to values in the 10 − 50 TeV range. An alternative interpretation for SUSY models with decoupled scalar masses is that perhaps the recent lattice evaluation of the hadronic vac- uum polarization could be confirmed which leads to a Standard Model theory-experiment agreement in which case there is no anomaly.
    [Show full text]
  • Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks
    Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks Joseph I. Kapusta∗ Abstract The possibility that experiments at high-energy accelerators could create new forms of matter that would ultimately destroy the Earth has been considered several times in the past quarter century. One consequence of the earliest of these disaster scenarios was that the authors of a 1993 article in Physics Today who reviewed the experi- ments that had been carried out at the Bevalac at Lawrence Berkeley Laboratory were placed on the FBI's Unabomber watch list. Later, concerns that experiments at the Relativistic Heavy Ion Collider at Brookhaven National Laboratory might create mini black holes or nuggets of stable strange quark matter resulted in a flurry of articles in the popular press. I discuss this history, as well as Richard A. Pos- ner's provocative analysis and recommendations on how to deal with such scientific risks. I conclude that better communication between scientists and nonscientists would serve to assuage unreasonable fears and focus attention on truly serious potential threats to humankind. Key words: Wladek Swiatecki; Subal Das Gupta; Gary D. Westfall; Theodore J. Kaczynski; Frank Wilczek; John Marburger III; Richard A. Posner; Be- valac; Relativistic Heavy Ion Collider (RHIC); Large Hadron Collider (LHC); Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; CERN; Unabomber; Federal Bureau of Investigation; nuclear physics; accel- erators; abnormal nuclear matter; density isomer; black hole; strange quark matter; scientific risks. arXiv:0804.4806v1 [physics.hist-ph] 30 Apr 2008 ∗Joseph I. Kapusta received his Ph.D. degree at the University of California at Berkeley in 1978 and has been on the faculty of the School of Physics and Astronomy at the University of Minnesota since 1982.
    [Show full text]
  • Top Quark Physics in the Large Hadron Collider Era
    Top Quark Physics in the Large Hadron Collider era Michael Russell Particle Physics Theory Group, School of Physics & Astronomy, University of Glasgow September 2017 arXiv:1709.10508v2 [hep-ph] 31 Jan 2018 A thesis submitted in fulfilment of the requirements for the degree of Doctor of Philosophy Abstract We explore various aspects of top quark phenomenology at the Large Hadron Collider and proposed future machines. After summarising the role of the top quark in the Standard Model (and some of its well-known extensions), we discuss the formulation of the Standard Model as a low energy effective theory. We isolate the sector of this effective theory that pertains to the top quark and that can be probed with top observables at hadron colliders, and present a global fit of this sector to currently available data from the LHC and Tevatron. Various directions for future improvement are sketched, including analysing the potential of boosted observables and future colliders, and we highlight the importance of using complementary information from different colliders. Interpretational issues related to the validity of the effective field theory formulation are elucidated throughout. Finally, we present an application of artificial neural network algorithms to identifying highly- boosted top quark events at the LHC, and comment on further refinements of our analysis that can be made. 2 Acknowledgements First and foremost I must thank my supervisors, Chris White and Christoph Englert, for their endless support, inspiration and encouragement throughout my PhD. They always gave me enough freedom to mature as a researcher, whilst providing the occasional neces- sary nudge to keep me on the right track.
    [Show full text]
  • MIT at the Large Hadron Collider—Illuminating the High-Energy Frontier
    Mit at the large hadron collider—Illuminating the high-energy frontier 40 ) roland | klute mit physics annual 2010 gunther roland and Markus Klute ver the last few decades, teams of physicists and engineers O all over the globe have worked on the components for one of the most complex machines ever built: the Large Hadron Collider (LHC) at the CERN laboratory in Geneva, Switzerland. Collaborations of thousands of scientists have assembled the giant particle detectors used to examine collisions of protons and nuclei at energies never before achieved in a labo- ratory. After initial tests proved successful in late 2009, the LHC physics program was launched in March 2010. Now the race is on to fulfill the LHC’s paradoxical mission: to complete the Stan- dard Model of particle physics by detecting its last missing piece, the Higgs boson, and to discover the building blocks of a more complete theory of nature to finally replace the Standard Model. The MIT team working on the Compact Muon Solenoid (CMS) experiment at the LHC stands at the forefront of this new era of particle and nuclear physics. The High Energy Frontier Our current understanding of the fundamental interactions of nature is encap- sulated in the Standard Model of particle physics. In this theory, the multitude of subatomic particles is explained in terms of just two kinds of basic building blocks: quarks, which form protons and neutrons, and leptons, including the electron and its heavier cousins. From the three basic interactions described by the Standard Model—the strong, electroweak and gravitational forces—arise much of our understanding of the world around us, from the formation of matter in the early universe, to the energy production in the Sun, and the stability of atoms and mit physics annual 2010 roland | klute ( 41 figure 1 A photograph of the interior, central molecules.
    [Show full text]
  • CERN Intersecting Storage Rings (ISR)
    Proc. Nat. Acad. Sci. USA Vol. 70, No. 2, pp. 619-626, February 1973 CERN Intersecting Storage Rings (ISR) K. JOHNSEN CERN It has been realized for many years that it would be possible to beams of protons collide with sufficiently high interaction obtain a glimpse into a much higher energy region for ele- rates for feasible experimentation in an energy range otherwise mentary-particle research if particle beams could be persuaded unattainable by known techniques except at enormous cost. to collide head-on. A group at CERN started investigating this possibility in To explain why this is so, let us consider what happens in a 1957, first studying a special two-way fixed-field alternating conventional accelerator experiment. When accelerated gradient (FFAG) accelerator and then, in 1960, turning to the particles have reached the required energy they are directed idea of two intersecting storage rings that could be fed by the onto a target and collide with the stationary particles of the CERN 28 GeV proton synchrotron (CERN-PS). This change target. Most of the energy given to the accelerated particles in concept for these initial studies was stimulated by the then goes into keeping the particles that result from the promising performance of the CERN-PS from the very start collision moving in the direction of the incident particles (to of its operation in 1959. conserve momentum). Only a quite modest fraction is "useful After an extensive study that included building an electron energy" for the real purpose of the experiment-the trans- storage ring (CESAR) to investigate many of the associated formation of particles, the creation of new particles.
    [Show full text]
  • Femtoscopy of Proton-Proton Collisions in the ALICE Experiment
    Femtoscopy of proton-proton collisions in the ALICE experiment DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Nicolas Bock, B.Sc. B.Eng., M.Sc. Graduate Program in Physics The Ohio State University 2011 Dissertation Committee: Professor Thomas J. Humanic, Advisor Professor Michael Lisa #1 Professor Klaus Honscheid #2 Professor Richard Furnstahl #3 c Copyright by Nicolas Bock 2011 Abstract The Large Ion Collider Experiment (ALICE) at CERN has been designed to study matter at extreme conditions of temperature and pressure, with the long term goal of observing deconfined matter (free quarks and gluons), study its properties and learn more details about the phase diagram of nuclear matter. The ALICE experiment provides excellent particle tracking capabilities in high multiplicity proton-proton and heavy ion collisions, allowing to carry out detailed research of nuclear matter. This dissertation presents the study of the space time structure of the particle emission region, also known as femtoscopy, in proton- proton collisions at 0.9, 2.76 and 7.0 TeV. The emission region can be characterized by taking advantage of the Bose-Einstein effect for identical particles, which causes an enhancement of produced identical pairs at low relative momentum. The geometry of the emission region is related to the relative momentum distribution of all pairs by the Fourier transform of the source function, therefore the measurement of the final relative momentum distribution allows to extract the initial space-time characteristics. Results show that there is a clear dependence of the femtoscopic radii on event multiplicity as well as transverse momentum, a signature of the transition of nuclear matter into its fundamental components and also of strong interaction among these.
    [Show full text]
  • Pos(ICRC2019)446
    New Results from the Cosmic-Ray Program of the NA61/SHINE facility at the CERN SPS PoS(ICRC2019)446 Michael Unger∗ for the NA61/SHINE Collaborationy Karlsruhe Institute of Technology (KIT), Postfach 3640, D-76021 Karlsruhe, Germany E-mail: [email protected] The NA61/SHINE experiment at the SPS accelerator at CERN is a unique facility for the study of hadronic interactions at fixed target energies. The data collected with NA61/SHINE is relevant for a broad range of topics in cosmic-ray physics including ultrahigh-energy air showers and the production of secondary nuclei and anti-particles in the Galaxy. Here we present an update of the measurement of the momentum spectra of anti-protons produced in p−+C interactions at 158 and 350 GeV=c and discuss their relevance for the understanding of muons in air showers initiated by ultrahigh-energy cosmic rays. Furthermore, we report the first results from a three-day pilot run aimed at investigating the ca- pability of our experiment to measure nuclear fragmentation cross sections for the understanding of the propagation of cosmic rays in the Galaxy. We present a preliminary measurement of the production cross section of Boron in C+p interactions at 13.5 AGeV=c and discuss prospects for future data taking to provide the comprehensive and accurate reaction database of nuclear frag- mentation needed in the era of high-precision measurements of Galactic cosmic rays. 36th International Cosmic Ray Conference -ICRC2019- July 24th - August 1st, 2019 Madison, WI, U.S.A. ∗Speaker. yhttp://shine.web.cern.ch/content/author-list c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
    [Show full text]