AEGIS. Antihydrogen Experiment: Gravity, Interferometry, Spectroscopy University of Oslo - H. Sandaker
|
|
|
- Amberly Murphy
- 5 years ago
- Views:
Transcription
1 AEGIS Antihydrogen Experiment: Gravity, Interferometry, Spectroscopy
2 AEGIS experiment - Importance of anti-matter research We observe a matter-antimatter asymmetry in the Universe We expect there to be produced equal amounts of matter and antimatter in the big bang but today we only observe matter We search for the origin of this asymmetry Quantum theory (CPT) violations? Gravitation asymmetries? Other possibilities? Anti-matter experiments probing gravitation AEGIS GBAR ALPHA Main goal of AEGIS is to test the Weak Equivalence Principle stating that all bodies fall with the same acceleration independent of mass and composition and to perform spectroscopy measurements with anti-hydrogen
3 AEGIS experiment - Principle Pulsed! Positronium excitation Ps(n = 1) + Laser fields Ps(n 30) Charge exchange at low energies: Ps(n 30) + H H (n) + e Manipulation and acceleration of excited anti-hydrogen Rydberg atoms in time depend. fields Deecitation H (n) H (n = 1) Annihilation of ground state anti hydrogen in the detector
4 AEGIS experiment - at AD at CERN
5 AEGIS experiment - apparatus The AEGIS Experiment proposal (Antimatter Experiment, Gravity, Interferometry, Spectroscopy) Very first production of a pulsed cold beam of anti-hydrogen (T~ 100 mk) Measurement of the beam deflection with a Moire reflectometer (grating pitch ~ 40 um) g measurement with 1% accuracy on anti-hydrogen
6 AEGIS experiment - AD hall
7 AEGIS collaboration - about 80 authors
8 Norwegian Contributions to AEGIS - Research Overview 1. Antiproton annihilation studies 2. Development of annihilation detectors 3. Software and simulations 4. Novel beamline GRACE 5. Positronium research 6. Common tasks (e.g. testbeam) 7. Local infrastructure in Norway
9 Norwegian contribution - Example results 1. Antiproton annihilation studies MIMOTERA: First (successful) measurement of antiproton annihilation directly on a segmented silicon sensor. Silicon strip: Observation of effects due to space plasma ( volcano effect) at lower bias voltage, sensitivity to different annihilation products can be tuned through the thickness ATLAS 3D: Thicker sensor allows observation of secondary prongs, pions distringuisable from heavier fragments, - production saturation Thanks to MIMOTERA and ATLAS and others N. Pacifico et al. NIM A - DOI: /j.nima etc. 9
10 Norwegian contribution - Example results Antiproton tagging and vertex fitting in a Timepix3 detector S. Aghion et al 2018 JINST 13 P Software and Simulations - Studies of annihilation in a Timepix3 detector Thanks to TIMEPIX et al.
11 Norwegian contribution - Example results 2. Development of annihilation detector - Novel strip detector Building a position sensitive strip detector to measure the annihilation of anti-hydrogen Initial requirements : - ~ 10 µm precision (25 µm pitch) - < 77 K operation - 1ms time resolution - 20 x 20 cm 2 area Additional new requirements : max 50 um thickness to avoid scattering vacuum separation window (UHV - UV) 10 x 8 cm 2 area Thanks to Chloe and Tim
12 AEGIS experiment - Example result 4. Novel beamline GRACE Energy [kev] One electrode bends the low energy antiprotons and the high energy particles, heavy fragments (background) goes straight Two Einzel lenses for focussing 300 um Timepix3 detector First measurements with this new setup last week, test-beam ongoing Result: single anti-protons at kev energies
13 AEGIS experiment - Example result 5. Positronium Research
14 Norwegian Contributions to AEGIS - Collaboration PhDs: Helga Holmestad (UiO), (Stapnes/Sandaker/Røhne) Angela Gligorova (UiB), (Sandaker/Pacifico/Doser) Postdoctor: Lillian Smestad (CERN), Researchers: Torkjell Huuse (UiO), Nicola Pacifico (UiB), University staff: UiO: Ole Dorholt, David Bang (ELAB), UiO: Ole Røhne, Heidi Sandaker (High Energy Physics) UiB: Jan Petter Hansen (Atomic physics) UiB: Heidi Sandaker (Subatomic Physics), end 2018 Industrial partners: SINTEF: Ozhan Koybasi et al. IDEAS: Gunnar Mæhlum et al.
15 Norwegian Contributions to AEGIS - Funding RCN: CERN related research project: ~2 MNOK RCN: Personal postdoctor grant (Smestad): ~2.4 MNOK RCN/UiB: FRINATEK Research project ~10.2 MNOK BRF/UiB: Bergen Research Foundation grant UiB: PhD Quota Scholarship PhD student finished
16 AEGIS experiment - Future plans Previous project Physics Run April 2018 Refurbishing of lab Project period Contributions to Testbeam Building 2nd generation detectors Test of 2nd generation detectors (sources) Future of AEGIS Norway meeting Final results for current project
17 Education and Outreach Slide from L. Smestad
18 Backup
19 AEGIS experiment - Current plans 3. Improved infrastructure in Oslo New clean room, thanks to the UiO MN faculty and the FI Currently refurbishing the new laboratory for better detector development Novel bonding machine arrived, the first in a series of new equipment, which is important for the current work on AEGIS Next step: We have material to build more silicon strip sensors, 2nd generation UiO FI Cleanroom - will be used for ATLAS upgrade as well as AEGIS etc.
OVERVIEW OF RECENT WORK ON LASER EXCITATION OF POSITRONIUM FOR THE FORMATION OF ANTIHYDROGEN
OVERVIEW OF RECENT WORK ON LASER EXCITATION OF POSITRONIUM FOR THE FORMATION OF ANTIHYDROGEN Anti-Apple g? g? Pauline Yzombard (1), on behalf of the AEgIS (2) collaboration (1) Laboratoire Aimé Cotton,
Fundamental physics with antihydrogen and antiprotons at the AD. Michael Doser CERN
Fundamental physics with antihydrogen and antiprotons at the AD Michael Doser CERN What measurements are we talking about? 1) Precise spectroscopic comparison between H and H tests of fundamental symmetry
Experiments with low energy antimatter
Experiments with low energy antimatter Giovanni Consolati, on behalf of the AEGIS collaboration Politecnico di Milano and Istituto Nazionale Fisica Nucleare - Milano Introduction to cold antimatter Experiments
Development and data analysis of a position detector for AEḡIS (Antimatter Experiment: Gravity, Interferometry, Spectroscopy)
Development and data analysis of a position detector for AEḡIS (Antimatter Experiment: Gravity, Interferometry, Spectroscopy) Angela Gligorova Dissertation for the degree of Philosophiae Doctor (PhD) Department
Antimatter. Jan Meier. Seminar: Experimental Methods in Atomic Physics May, 8th 2007
Antimatter Jan Meier Seminar: Experimental Methods in Atomic Physics May, 8th 27 Overview Antimatter and CPT theorie what is antimatter? what physics does it follow to? First observations of antimatter
ATHENA / AD-1. First production and detection of cold antihydrogen atoms. ATHENA Collaboration. Rolf Landua CERN
ATHENA / AD-1 First production and detection of cold antihydrogen atoms ATHENA Collaboration Rolf Landua CERN 1 LONG TERM PHYSICS GOALS Antihydrogen = Hydrogen? CPT Gravity But... 2 FIRST GOAL PRODUCTION
CDF. Antimatter Gravity Experiment. An Opportunity for Fermilab to (potentially) Answer Three of the Big Questions of Particle Physics
Antimatter Gravity Experiment An Opportunity for Fermilab to (potentially) Answer Three of the Big Questions of Particle Physics Physics Motivation g has never been measured! CPT: g g earth antiearth earth
The GBAR experiment. Dirk van der Werf
The GBAR experiment Dirk van der Werf principle detector Laser (t 0 ) gravity J.Walz & T. Hänsch" General Relativity and Gravitation, 36 (2004) 561 detector (t 1 ) 2 principle detector Laser (t 0 ) gravity
AEgIS Experiment Commissioning at CERN
AEgIS Experiment Commissioning at CERN D. Krasnický a,b,s.aghion c,d,c.amsler e,a.ariga e,t.ariga e, A. S. Belov f,g.bonomi g,h,p.bräunig i,r.s.brusa j,j.bremer k, G. Burghart k,l.cabaret l,m.caccia d,c.canali
IAP NAN of Ukraine activity in. Possible areas of cooperation in. Roman Kholodov, PICS Meeting, Basivka, Ukraine,
1 IAP NAN of Ukraine activity in field of High Energy Physics. Possible areas of cooperation in frame of PICS and beyond. Institute of Applied Physics National Academy of Sciences of Ukraine 2 The Institute
Study of Edgeless TimePix Pixel Devices. Dylan Hsu Syracuse University 4/30/2014
Study of Edgeless TimePix Pixel Devices Dylan Syracuse University 2 3 Million-Dollar Question Universe is made of matter Particle decays putatively produce equal amounts of matter and antimatter Where
Gravitational Repulsion of Matter and Antimatter
Gravitational Repulsion of Matter and Antimatter The changing acceleration of the electrons explains the created negative electric field of the magnetic induction, the electromagnetic inertia, the changing
The CERN Antiproton Physics Programme The Antiproton Decelerator (AD) & ELENA
The CERN Antiproton Physics Programme The Antiproton Decelerator (AD) & ELENA Dániel Barna Wigner Research Centre for Physics, Budapest, Hungary The CERN antiproton facilities Experiments, their programmes
The Start of the LHC Era. Peter Wittich Laboratory of Elementary Particle Physics Cornell University
The Start of the LHC Era Peter Wittich Laboratory of Elementary Particle Physics Cornell University Big Bang - where it all began 3 4 13 billion years ago 4 13 billion years ago hot, highly energetic
POSITRON ACCUMULATOR SCHEME for AEGIS
POSITRON ACCUMULATOR SCHEME for AEGIS A. S. Belov, S. N. Gninenko INR RAS, Moscow 1 What positron beam is requiered for AEGIS? Number of antihydrogen atoms produced with AEGIS scheme: N Hbar ~ ce n H-
ANTIMATTER MATTER. does the difference between matter and antimatter arise?
WHY ANTIMATTER MATTERS! One of the most striking facts about the Universe is that it is composed almost entirely of matter. At the Big Bang equal amounts of matter and antimatter would have been created.
Testing the Weak Equivalence Principle with an antimatter beam at CERN
Home Search Collections Journals About Contact us My IOPscience Testing the Weak Equivalence Principle with an antimatter beam at CERN This content has been downloaded from IOPscience. Please scroll down
IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick April
IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick th April 14 2010 The Standard Model 2 Some Questions What is antimatter? Why are there three colours
GBAR Project Gravitational Behavior of Antihydrogen at Rest
GBAR Project Gravitational Behavior of Antihydrogen at Rest Pierre Dupré CEA Saclay, FRANCE 1 Contents Motivation Scheme Schedule 2 Motivation A direct test of the Equivalence Principle with antimatter
Particle + Physics at ATLAS and the Large Hadron Coillder
Particle + Physics at ATLAS and the Large Hadron Coillder Discovering the elementary particles of the Universe Kate Shaw The International Centre for Theoretical Physics + Overview Introduction to Particle
LHCb. Zooming in on the matter antimatter puzzle. researching fundamental physics since Nikhef Annual Report
20 LHCb Zooming in on the matter antimatter puzzle Elena Dall Occo working with the read-out electronics of the VeloPix detector. researching fundamental physics since 1947 2016 Figure 1. Display of a
\ \ \/ \\// (o) (o) U. February 11, UT Saturday Morning Physics. Yuri Kamyshkov University of Tennessee
\ \ \/ \\// (o) (o) U February 11, 2017 @ UT Saturday Morning Physics Yuri Kamyshkov University of Tennessee kamyshkov@utk.edu 1 2 Large Hadron Collider CERN European Centre for Particle Physics Geneva,
Observation of the 1S-2S Transition in Antihydrogen
Observation of the 1S-2S Transition in Antihydrogen Dirk van der Werf Swansea University CEA-Saclay ALPHA What do we want to do Check CPT conservation Baryon asymmetry Standard model extension (SME): Assume
IIT Bombay joins India-CMS proposal
IIT Bombay joins India-CMS proposal Pradeep Sarin, Assistant Professor, Department of Physics, IIT Bombay Page 1 of 13 Overlap of research interests: IIT-B & BARC Physics: Studies of jet fragmentation
Equivalence principle for free and bound antiparticles
Equivalence principle for free and bound antiparticles Savely G Karshenboim D.I. Mendeleev Institute for Metrology (St. Petersburg) and Max-Planck-Institut für Quantenoptik (Garching) How accurate are
Finish up our overview of small and large
Finish up our overview of small and large Lecture 5 Limits of our knowledge Clicker practice quiz Some terminology... "Elementary particles" = objects that make up atoms (n,p,e) or are produced when atoms
Examples for experiments that can be done at the T9 beam line
Examples for experiments that can be done at the T9 beam line Example 1: Use muon tomography to look for hidden chambers in pyramids (2016 winning proposal, Pyramid hunters) You may know computer tomography
Analyzing CMS events
Quarknet University of Rochester, March 23, 2012 Analyzing CMS events Questions in Particle Physics Introducing the Standard Model The Large Hadron Collider The CMS detector W and Z bosons: decays ispy
Yiming Li (LAL, Orsay) On behalf of the LHCb and MoEDAL collaborations
Yiming Li (LAL, Orsay) On behalf of the LHCb and MoEDAL collaborations LHCb 2016 operation Physics highlights Upgrade MoEDAL 16/12/2016 2 Why heavy flavour? A precision experiment for heavy flavour physics
THE ELENA PROJECT AT CERN
Vol. 46 (2015) ACTA PHYSICA POLONICA B No 1 THE ELENA PROJECT AT CERN W. Oelert representing the ELENA Collaboration Johannes Gutenberg-Universität Institut für Physik Staudingerweg 7, 55128 Mainz, Germany
IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick March 30th 2011
IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick March 30th 2011 The Standard Model 2 Some Questions What is antimatter? Why are there three colours
Light ion recoil detector
Light ion recoil detector Overall design The detector for light (target-like) particles is a substantial part of the R3B setup. It allows registration of recoils in coincidence with the heavy fragments,
Option 212: UNIT 2 Elementary Particles
Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.pm LRB Intro lecture 28-Jan-15 12.pm LRB Problem solving (2-Feb-15 1.am E Problem Workshop) 4-Feb-15 12.pm
Matter, Antimatter and the Strangeness of CP violation
Matter, Antimatter and the Strangeness of CP violation Angela Romano Angela Romano Masterclass 21/04/10 1 Cambridge, 1928 : Dirac predicted the existence of the positron e+, same mass but opposite charge
The Physics of Particles and Forces David Wilson
The Physics of Particles and Forces David Wilson Particle Physics Masterclass 21st March 2018 Overview David Wilson (TCD) Particles & Forces 2/30 Overview of Hadron Spectrum Collaboration (HadSpec) scattering
Status on cold muonium production and testbeam request
Status on cold muonium production and testbeam request A. Antognini 1,2, P. Crivelli 1, K. Kirch 1,2, D. Taqqu 1 M. Bartkowiak 2, A. Knecht 2, A. Papa 2, N. Ritjoho 2, D. Rousso 2, R. Scheuermann 2, A.
Building a Tracking Detector for the P2 Experiment
Building a Tracking Detector for the P Experiment DPG Frühjahrstagung, Hamburg 016 Marco Zimmermann Institute for Nuclear Physics March 3, 016 The P Experiment: Overview The Idea Precision measurement
Dark Energy or Repulsive Gravity
Dark Energy or Repulsive Gravity The leading theory to explain the accelerating expansion is the existence of a hypothetical repulsive force called dark energy. But in the new study, Massimo Villata, an
Last Friday: pp(bar) Physics Intro, the TeVatron
Last Friday: pp(bar) Physics Intro, the TeVatron Today: The Large Hadron Collider (LHC) The Large Hadron Collider (LHC) 7 TeV + 7 TeV Protons Protons 10 11 Protons per bunch Bunch Crossings 4x10 7 Hz Proton
Information about the T9 beam line and experimental facilities
Information about the T9 beam line and experimental facilities The incoming proton beam from the PS accelerator impinges on the North target and thus produces the particles for the T9 beam line. The collisions
LASER MICRO-MACHINING FOR 3D DIAMOND DETECTORS APPLICATIONS
LASER MICRO-MACHINING FOR 3D DIAMOND DETECTORS APPLICATIONS B.Caylar 1, M.Pomorski 1, D.Tromson 1, P.Bergonzo 1, J.Alvarez 2, A.Oh 3,C. Da Via 3, I.Haughton 3, V.Tyzhnevy 3, T.Wengler 4 1 CEA-LIST, French
LHCb Overview. Barbara Storaci on behalf of the LHCb Collaboration
LHCb Overview Barbara Storaci on behalf of the LHCb Collaboration CERN Council, December 14 th, 2012 Overview Introduction Collaboration Type of physics considered Detector Detector performances Selection
COMPASS Drell-Yan. Michela Chiosso, University of Torino and INFN. TMD ECT* Workshop April 2016
COMPASS Drell-Yan Michela Chiosso, University of Torino and INFN TMD ECT* Workshop 11-15 April 2016 Outline Single polarized Drell-Yan at COMPASS DY vs SIDIS at COMPASS Experimental setup Spin-dependent
Research Publications at Politecnico di Milano
RE.PUBLIC@POLIMI Research Publications at Politecnico di Milano This is the published version of: R.S. Brusa, C. Amsler, T. Ariga, G. Bonomi, P. Braunig, L. Cabaret, M. Caccia, R. Caravita, F. Castelli,
Propagation in the Galaxy 2: electrons, positrons, antiprotons
Propagation in the Galaxy 2: electrons, positrons, antiprotons As we mentioned in the previous lecture the results of the propagation in the Galaxy depend on the particle interaction cross section. If
Tau-neutrino production study at CERN SPS: Novel approach by the DsTau experiment
Tau-neutrino production study at CERN SPS: Novel approach by the DsTau experiment O. Sato (Nagoya University) for the DsTau collaboration 26/Aug/2016 NuFact2016, ICISE, Quy Nhon Current status on neutrino
Laboratory for Nuclear Science
The Laboratory for Nuclear Science (LNS) provides support for research by faculty and research staff members in the fields of particle, nuclear, and theoretical plasma physics. This includes activities
arxiv:physics/ v2 [physics.ins-det] 18 Jul 2000
![arxiv:physics/ v2 [physics.ins-det] 18 Jul 2000](/thumbs/86/94459867.jpg "arxiv:physics/ v2 [physics.ins-det] 18 Jul 2000")
Lorentz angle measurements in irradiated silicon detectors between 77 K and 3 K arxiv:physics/759v2 [physics.ins-det] 18 Jul 2 W. de Boer a, V. Bartsch a, J. Bol a, A. Dierlamm a, E. Grigoriev a, F. Hauler
Neutron Source Capabilities at Ohio University
Neutron Source Capabilities at Ohio University Carl R. Brune, Steven M. Grimes, David. C. Ingram, and Thomas N. Massey Department of Physics and Astronomy, Ohio University, Athens OH 45701, USA (Dated:
What detectors measure
What detectors measure As a particle goes through matter, it releases energy Detectors collect the released energy and convert it to electric signals recorded by DAQ Raw event record is a collection of
PoS(DIS 2010)058. ATLAS Forward Detectors. Andrew Brandt University of Texas, Arlington
University of Texas, Arlington E-mail: brandta@uta.edu A brief description of the ATLAS forward detectors is given. XVIII International Workshop on Deep-Inelastic Scattering and Related Subjects April
Welcome to DESY. What is DESY and what kind of research is done here?
Welcome to DESY. What is DESY and what kind of research is done here? Michael Grefe DESY Press and Public Relations (PR) What is DESY? > Deutsches Elektronen-Synchrotron (German electron synchrotron) DESY
Control of the fabrication process for the sensors of the CMS Silicon Strip Tracker. Anna Macchiolo. CMS Collaboration
Control of the fabrication process for the sensors of the CMS Silicon Strip Tracker Anna Macchiolo Universita di Firenze- INFN Firenze on behalf of the CMS Collaboration 6 th International Conference on
Q U P L A S QUantum Interferometry, decoherence and gravitational studies with Positrons and LASers
Quantum Interferometry and Gravity with Positronium Marco G. Giammarchi Istituto Nazionale Fisica Nucleare Milano AEC and LHEP of the University of Bern Q U P L A S QUantum Interferometry, decoherence
Experimental High-Energy Subatomic Particle Physics
Experimental High-Energy Subatomic Particle Physics Andreas Warburton Department of Physics McGill University McGill Explorations 2008 Montréal, 2008.07.14 Andreas Warburton (McGill) 1 Outline Why did
Introduction to the Standard Model
Introduction to the Standard Model Bill Murray, RAL, Quarks and leptons Bosons and forces The Higgs March 2002 1 Outline: An introduction to particle physics What is the Higgs Boson? Some unanswered questions
THE ALPHA COLLABORATION
THE ALPHA COLLABORATION Aarhus University, Denmark Auburn University, USA University of British Columbia, Canada University of California Berkeley, USA University of Calgary, Canada CERN University of
arxiv: v2 [nucl-ex] 6 Oct 2008
![arxiv: v2 [nucl-ex] 6 Oct 2008](/thumbs/88/114593371.jpg "arxiv: v2 [nucl-ex] 6 Oct 2008")
he ime Projection Chamber for the ALICE Experiment C. Lippmann and the ALICE PC Collaboration CERN, 1211 Geneva 23, Switzerland he ime Projection Chamber of the ALICE Experiment has been installed in the
Tau-neutrino production study in 400 GeV proton interactions
Tau-neutrino production study in 400 GeV proton interactions Tomoko Ariga AEC/LHEP, University of Bern On behalf of the DsTau Collaboration Physics motivation Tau-neutrino: less studied particle in the
The Muonium Antimatter Gravity Experiment Testing to see if something is the Matter with Gravity. Thomas Phillips IIT
The Muonium Antimatter Gravity Experiment Testing to see if something is the Matter with Gravity Thomas Phillips IIT 1 Outline 1. Motivation: What if we are wrong about antimatter gravity? 2. Why Muonium
Accelerator facilities - Ruđer Bošković Institute, Zagreb, Croatia
Accelerator facilities - Ruđer Bošković Institute, Zagreb, Croatia Milko Jaksic, Neven Soic Our capabilities (accelerator, sources, beamlines,...) Research activities (projects, users, int. collaborations,...)
CPT symmetry test Gravity between matter and antimatter Listen to the whisper of nature (Planck mass vs our limitedness )
Trapped charged particles and Fundamental physics April 12-16, 2010, Saariselkae, Finland Advances in Antihydrogen y g Experiments p Yasunori Yamazaki RIKEN & Univ. Tokyo Trapped charged particles and
The Gamma Factory proposal for CERN
The Gamma Factory proposal for CERN Photon-2017 Conference, May 2017 Mieczyslaw Witold Krasny LPNHE, CNRS and University Paris Sorbonne 1 The Gamma Factory in a nutshell Accelerate and store high energy
A beam line for schools
A beam line for schools Great things can happen when high schools get involved with cutting edge science, and that s exactly what CERN is proposing with its new beam line for schools competition, which
novel DIagnostic Techniques for future particle Accelerators: A Marie Curie Initial Training NETwork
novel Iagnostic Techniques for future particle Accelerators: A Marie Curie Initial Training NETwork Carsten P. Welsch - On behalf of the ITANET Consortium - c.welsch@gsi.de Outline What is ITANET? Network
Electron Beam Polarimetry at JLab Hall C Dave Gaskell PST 2009 September 7, 2009
Electron Beam Polarimetry at JLab Hall C Dave Gaskell PST 2009 September 7, 2009 1. Møller Polarimeter 2. Compton Polarimeter 3. Summary JLab Polarimetry Techniques Three different processes used to measure
Long Range Plan Perspectives of Nuclear Physics in Europe. Günther Rosner IUPAP WG.9, Cambridge MA USA, 24/7/11 1
Long Range Plan 2010 Perspectives of Nuclear Physics in Europe Günther Rosner IUPAP WG.9, Cambridge MA USA, 24/7/11 1 Objectives Review status of the field Issue recommendations to advance The science
Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG
Weak Interactions The Theory of GLASHOW, SALAM and WEINBERG ~ 1959-1968 (Nobel 1979) Theory of the unified weak and electromagnetic interaction, transmitted by exchange of intermediate vector bosons mass
New subatomic particle and the Electro-Strong and -Weak Interaction
New subatomic particle and the Electro-Strong and -Weak Interaction Named Ds3*(2860), the particle, a new type of meson, was discovered by analyzing data collected with the LHCb detector at CERN's Large
The GBAR experiment. by on 04/05/19. Re-use and distribution is strictly not permitted, except for Open Access articles.
Antimatter and Gravity (WAG 2013) International Journal of Modern Physics: Conference Series Vol. 30 (2014) 1460263 (8 pages) c The Author DOI: 10.1142/S2010194514602634 The GBAR experiment (for the GBAR
ATLAS ITK Pixel 2018 CERN Plans (plus some telescope infrastructure)
ATLAS ITK Pixel 2018 CERN Plans (plus some telescope infrastructure) H6 USER MEETING 14th March 2018 A. Rummler1, M. Bomben2, J. Weingarten3 1 CERN; 2UPD&LPNHE, Paris; 3Göttingen University On behalf of
The Hermes Recoil Silicon Detector
The Hermes Recoil Silicon Detector Introduction Detector design considerations Silicon detector overview TIGRE microstrip sensors Readout electronics Test beam results Vertex 2002 J. Stewart DESY Zeuthen
J-PARC E07 Ξ - Junya Yoshida (Advanced Science Research Center, JAEA) On behalf of J-PARC E07 Collaboration K + K - X -
J-PARC E07 Systematic study of double strangeness nuclei with Hybrid emulsion method LL hypernucleus K - 1.8GeV/c Target SSD X - K + nλ p p Λ n X hypernucleus n p p Ξ - n Ge detector X-ray X-ray from X
AEGIS: Apparatus to Explore the Gravitational Interaction of antiatoms: the R& D programme
AEGIS: Apparatus to Explore the Gravitational Interaction of antiatoms: the R& D programme M. Amoretti 1, C. Amsler 2, G. Bonomi 3, C. Carraro 1,6, M. Doser 4, S. Farinon 1,G. Ferrari 5, A. Kellerbauer
The ATLAS Experiment and the CERN Large Hadron Collider
The ATLAS Experiment and the CERN Large Hadron Collider HEP101-2 January 28, 2013 Al Goshaw 1 HEP 101-2 plan Jan. 14: Introduction to CERN and ATLAS DONE Today: 1. Comments on grant opportunities 2. Overview
Introduction to Cosmology
Introduction to Cosmology Subir Sarkar CERN Summer training Programme, 22-28 July 2008 Seeing the edge of the Universe: From speculation to science Constructing the Universe: The history of the Universe:
Experimental Tests of CPT Invariance at CERN
Dezső Horváth: CPT Tests at CERN Szegedi Egyetem, 2018.10.15. p. 1 Experimental Tests of CPT Invariance at CERN Szegedi Egyetem, Elm-Fiz. Tanszék, 2018.10.15. Horváth Dezső horvath.dezso@wigner.mta.hu
Particle Production Measurements at Fermilab
Particle Production Measurements at Fermilab Dr. Nickolas Solomey, IIT and Fermilab co Spokesman of E907 TEV II Astroparticle Physics Conference Univ. of Wisconsin, Madison 28 31 Aug., 2006 Particle Production
Update on Timepix3 Telescope & Grazing Angles Results
Update on Timepix Telescope & Grazing Angles Results on behalf of the VELO Testbeam Group th Beam Telescopes and Test Beams workshop Barcelona -7//7 Timepix Telescope th BTTB - //7 Timepix Telescope Device
Non-collision Background Monitoring Using the Semi-Conductor Tracker of ATLAS at LHC
WDS'12 Proceedings of Contributed Papers, Part III, 142 146, 212. ISBN 978-8-7378-226-9 MATFYZPRESS Non-collision Background Monitoring Using the Semi-Conductor Tracker of ATLAS at LHC I. Chalupková, Z.
Measurement of the Proton Beam Polarization with Ultra Thin Carbon Targets at RHIC
1of23 Measurement of the Proton Beam Polarization with Ultra Thin Carbon Targets at RHIC Brookhaven National Laboratory for the RHIC Polarimetry Group Sep 12, 2013 Relativistic Heavy Ion Collider world
Report on Visit to Ruhr University Bochum by International Training Program From October 1st to November 29th 2010
Report on Visit to Ruhr University Bochum by International Training Program From October 1st to November 29th 2010 Graduate school of Engineering, Hori-Sekine Lab. Doctor course student Yusuke Abe Ruhr
AEGIS. Antimatter Experiment: Gravity, Interferometry, Spectroscopy. C. Canali INFN sez. Genova (AEgIS COLLABORATION)
AEGIS Antimatter Experiment: Gravity, Interferometry, Spectroscopy C. Canali INFN sez. Genova (AEgIS COLLABORATION) 46 Rencontres de Moriond 26 March 2011 LAPP, Annecy, France D. Sillou Queen s U Belfast,
Detection of trapped antihydrogen in ALPHA
Detection of trapped antihydrogen in ALPHA Richard Hydomako Department of Physics and Astronomy University of Calgary WNPPC, Feb 26 2012 Image credit: Maximilien Brice, CERN Physics motivation for antihydrogen
Possible sources of very energetic neutrinos. Active Galactic Nuclei
Possible sources of very energetic neutrinos Active Galactic Nuclei 1 What might we learn from astrophysical neutrinos? Neutrinos not attenuated/absorbed Information about central engines of astrophysical
Understanding the balance of matter and antimatter in the Universe
Understanding the balance of matter and antimatter in the Universe Physicists in the College of Arts and Sciences have made important discoveries regarding Bs meson particles -- something that may explain
HIGH INTENSITY ION BEAMS AT GANIL F. Chautard, September 6th, Cyclotron 2010 Lanzhou, China, september F. Chautard
HIGH INTENSITY ION BEAMS AT GANIL F. Chautard, September 6th, 2010 OUTLINE Operation modes at GANIL Statistics Stable beams Exotic beams ISOL In Flight Beam developments Stable beams Exotic beams Machine
The low Q 2 chicane and Compton polarimeter at the JLab EIC
EPJ Web of Conferences 112, 01007 (2016) DOI: 10.1051/ epjconf/ 201611201007 C Owned by the authors, published by EDP Sciences, 2016 The low Q 2 chicane and Compton polarimeter at the JLab EIC, Alexandre
ALICE, ATLAS, CMS, LHCb, TOTEM, LHCf
LHC EXPERIMENTS LHC EXPERIMENTS ALICE, ATLAS, CMS, LHCb, TOTEM, LHCf ACE Antiproton Cell Experiment Antiprotons versus cancer cells Non LHC Experiments ASACUSA Atomic Spectroscopy And Collisions Using
PMT Signal Attenuation and Baryon Number Violation Background Studies. By: Nadine Ayoub Nevis Laboratories, Columbia University August 5, 2011
PMT Signal Attenuation and Baryon Number Violation Background Studies By: Nadine Ayoub Nevis Laboratories, Columbia University August 5, 2011 1 The Standard Model The Standard Model is comprised of Fermions
The Large Hadron Collider, a marvel of technology Lyn Evans. Royal Institution of South Wales St David s day lecture, 16 th March 2017
The Large Hadron Collider, a marvel of technology Lyn Evans Royal Institution of South Wales St David s day lecture, 16 th March 2017 CERN was founded 1954: 12 European States Science for Peace Today:
Richard Hall-Wilton University College London. July 2002
PPRP, Richard Hall-Wilton University College London July 2002 July 2002, RAL Overview Introduction to HERA and ZEUS Detector Status Central Tracking Detector Microvertex Detector Global Tracking Trigger
Antimatter research at F(L)AIR
Antimatter research at F(L)AIR University of Wales Swansea Overview of the Flair facility Physics at FLAIR Antihydrogen spectroscopy Gravitational acceleration of amtihydrogen G-factor of the antiproton
A Brief History of Modern Physics
A Brief History of Modern Physics Modern Physics rests on two pillars: 1. Theory of Relativity (Einstein) Special Relativity 1905 General Relativity 1915 nature of space and time (phenomena at high speed)
E166: Polarized Positrons & Polarimetry
(DESY) - on behalf of the E166 Collaboration ILC: - why polarized positrons - e+ source options - undulator source scheme E166 - proof-of-principle demonstration of the undulator method - undulator basics
Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016
Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................
Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?
Origin of the Universe - 2 ASTR 2120 Sarazin What does it all mean? Fundamental Questions in Cosmology 1. Why did the Big Bang occur? 2. Why is the Universe old? 3. Why is the Universe made of matter?
SSA Measurements with Primary Beam at J-PARC
SSA Measurements with Primary Beam at J-PARC Joint UNM/RBRC Workshop on Orbital Angular Momentum in Albuquerque February 25 th, 2006 Yuji Goto (RIKEN/RBRC) February 25, 2006 Yuji Goto (RIKEN/RBRC) 2 Introduction
Towards the production of an anti-hydrogen beam
Towards the production of an anti-hydrogen beam S. Van Gorp 1, N. Kuroda 2, S. Ulmer 1, D.J. Murtagh 1, M. Corradini 4, M. Diermaier 6, M. Leali 4, C. Malbrunot 6, V. Mascagna 4, O. Massiczek 6, K. Michishio
Energy loss of alpha particles - Prelab questions
Energy loss of alpha particles - Prelab questions 1. Write down the decay path from 226 Ra to 206 Pb. Show the intermediate nuclides and the nuclear reactions which cause each transformation (α/β ± decay).