Risultati recenti di produzione

Size: px
Start display at page:

Download "Risultati recenti di produzione"

Transcription

1 Risultati recenti di produzione dell anti-idrogeno Luca Venturelli Università di Brescia (Dipartimento di Ingegneria dell Informazione) Istituto Nazionale di Fisica Nucleare Physics Department/INFN joint seminar DIPARTIMENTO DI FISICA, VIA CELORIA 16, MILANO 9 maggio 2014

2 2

3 Antihydrogen Matter Anti-matter particles antiparticles elements anti-elements H Antihydrogenis the simplest atom consisting entirely of antimatter 3

4 Antihydrogen: whatisitknown? Hydrogen Antihydrogen H 4

5 Antihydrogen: whatisitknown? Hydrogen Antihydrogen H one of the best understood and most precisely measuredsystem quantity exp. value[hz] ν -15 δ ν δ th exp ν 1s -2s ( ) ν ( ) 3 2s -2p ν HFS ( 9) ± ( ) 5

6 Antihydrogen: whatisitknown? Hydrogen Antihydrogen expected H one of the best understood and most precisely measuredsystem quantity 1s -2s exp. value[hz] δ ν δ th exp ν -15 ν ( ) 3 2s -2p ( ) ν HFS ( 9) ν ± ( ) No precise measurement Why? - Annihilations - Antihydrogen study is young 6

7 Antihydrogenhistoryisyoung H ( c) v H ( K) 7

8 Annihilation Matter-antimatter encounter annihilation Ex.1 Ex.2 electron-positron collision e + γ e Mass converted into energy γ 2 proton-antiproton collision π E = mc p p N.B. Pair production (inverse process of annihilation) permits antimatter production 8

9 Whystudyantihydrogen 1) Precise matter/antimatter comparison test of CPT symmetry 2) Measurement of the gravitational behaviour of antimatter test of WEP? Impossible with charged antiparticle onlywithneutralsystem H 9

10 Whystudyantihydrogen 1) Precise matter/antimatter comparison test of CPT symmetry 2) Measurement of the gravitational behaviour of antimatter test of WEP? Impossible with charged antiparticle onlywithneutralsystem H 10

11 Matter/antimatterasymmetryin the Universe Earth, Moon and planets made of matter Positrons and antiprotons in the cosmics rays are compatible with secondary production (made in the matter collision with the interstellar medium) No primordial antimatter detected 11

12 t 0 t < s equalquantityofmatterand antimatterexpectedfromsymmetry!? All antimatter disappeared and only(part of) matter(and we) survive Possible explanations rely on the fundamental symmetries violations 12

13 Discrete symmetries: C, P, T Parity transformation P: Inversion of the spatial coordinates ( x, y, z ) ( x, y, z ) Mirror reflection Charge coniugation transformation C: Change of each additive quantum numbers (for example the electrical charge) in its opposite q q Time reversal transformation T: Change the time arrow t t 13

14 Violationsofthe discrete symmetries In the pastc, P and T transformationswerebelievedtobeexactsymmetries But for Weak interaction: Parity violation SuggestedbyLee & Yang (1956) β-decay experiment by Wu et al (1957) CP violation(1964) K 0 decaysbycronin& Fitch(1964) 14

15 The CPT theorem 50 s Pauli, Schwinger, Lüders, Jost The CPTtheorem (1954): Any Lorentz-invariant local quantum field theory is invariant under the successive application of C, P and T Assumptions: - flat space-time, Lorentz-invariance, local interactions, unitarity, point-like particles Consequences: - particles/antiparticles: equal mass, lifetime; equal and opposite charge and magnetic moment - atoms/antiatoms: identical energy levels CPT invariance is inside the Standard Model In string theory(and quantum gravity): assumptions non valid CPT violations as a signature of string theory? No measurement of CPT violation exists Luca Venturelli-Risultati recenti di 15

16 CPT tests: relative & absoluteprecisions absolute precision(left edge) measuredquantity(right edge) = relative precision(length) planned Where CPT violation might appear is unknown 0 0 Considered best CPT test : K K Δm/m ~ Hz but absolute precision could be relevant H H highly competitive Luca Venturelli-Risultati recenti di 16

17 Test ofcpt symmetry 17

18 CPT violationin Standard ModelExtension Indiana group, Kostelecky et al. (since 1997) Standard Model can be extended with CPT violation Standard Model Extension (SME) is an effective field theory which contains: - General Relativity - Standard Model -Possibility of Lorentz Invariance Violation -CPT violation comes with Lorentz violation Modified Dirac equation CPT Violating terms Lorentz Invariance Violating terms R.Bluhm, A.Kostelecky, N.Russell, Phys. Rev. Lett. 82, 2254 (1999) - a & b have energy dimensions( absolute comparisons are important) - No quantitative prediction 18

19 Antihydrogenformation 19

20 CERN Accelerators LHC: 27 km Antihydrogenexperimentsat AD(Antiproton Decelerator) AD: 188 m Protons: Linac2 (50 MeV) ->ProtonSyncrotonBooster(1.4 GeV) ->ProtonSyncroton(25GeV) ->AD(:antiprotons) 20

21 Antihydrogenfactory LHC AD PS 21

22 AntiprotonDecelerator-AD AD is the only source of low-energy antiprotons All-in-one machine: antiproton capture, deceleration& cooling 2 E = mc + E K p + p p + p + p + p p + n p + n + p + p Efficiency: acceleration 10-3 production 10-4 collection(ad) 10-2 total 10-9 AD delivers to the experiments: antiprotonsper bunch( nslength) - 1 bunch/ 100 s - Energy = 5.3 MeV(100 MeV/c) 22

23 The experimentsat AD Experiments: -(2014) ALPHA, ATRAP, ASACUSA, ACE, AEgIS, BASE - ATHENA (terminated), GBAR(future) 23

24 Howtoformantihydrogen Recombinationprocesses Radiative recombination + p + e H + hν p Three-body recombination e + e H + e Two-stage charge exchange -9/2 24

25 ATHENA, ALPHA, ATRAP, ASACUSA Superposition of e+plasma and pbar cloud Howtoformantihydrogen Recombinationprocesses Radiative recombination + p + e H + hν p Three-body recombination e + e H + e Two-stage charge exchange ATRAP, AEGIS -9/2 25

26 Two-stagechargeexchange -Cold antihydrogen( antiproton at rest) - antihydrogen n-state can be controlled by laser (n-antihydrogen=n- Cs*) 26

27 Radiative and 3-body recombinationrates ATHENA 27

28 Typicalantihydrogenexperiment: ATHENA Three-body recombination letter to Nature Nature 419, (2002) 2.5 cm 10 4 pbars 10 8 e + 3T Radiative recombination antiprotons positrons First cold antihydrogens fromad fromthe experimentwithradioactivesources( 22 Na: 400 M e+/s) Procedure: 1) Trapping and cooling of antiprotons 2) Trapping and cooling of positrons 3) antiprotons& positrons mixing to form antihydrogens 10 7 (AD) (trapped) 1.5 GBq 22 Na10 8 (trapped) Hz 28

29 (charged) antimattertrap Charged particles are confined by: radially by B and longitudinally by E Penning trap ATHENA trap(2002): 29

30 Trappingand coolingofantiprotons T=15 K p<10-12 mb Technique developed by TRAP Collaboration 30

31 Trappingand coolingofpositrons 31

32 Antiprotonsand positronsmixing 32

33 Antihydrogenformation When antiprotons and positrons have similar velocities p e + e H + e + p + e H + hν Antihydrogen escapes from the trap centre and annihilates on the trap wall 33

34 ATHENA Antihydrogendetection M.Doser-CERN 34

35 ATHENA Antihydrogendetection M.Doser-CERN 35

36 ATHENA Antihydrogendetection M.Doser-CERN First antihydrogen detection (2002) Millions of antihydrogens produced 36

37 2.5 cm Si strips π 10 4 pbars Antihydrogendetection γ 10 8 e + H 10 4 p & 10 8 e + are mixed in Penning trap H form and fly away π H annihilate on trap wall Offline selection of H annihilation: CsI crystals γ π 3T Coincidence in space & time (<5µs) of: p annihilation(charged pion vertex) e + annihilation(2 back-to-back511 kev γ) Antihydrogen detection: field ionization technique ATRAP Coll. 37

38 AntihydrogenforCPT test matter-antimatter precise comparison by means of spectroscopy directexperimentaltest (no model is required) Plans for antihydrogen: - measurements: - Hyperfine splitting - methods: of ground state - 1S-2S transition - Antihydrogen trapping - Antihydrogen beam 38

39 AntihydrogenforCPT test matter-antimatter precise comparison by means of spectroscopy directexperimentaltest (no model is required) ALPHA ATRAP Plans for antihydrogen: - measurements: - Hyperfine splitting of ground state - 1S-2S transition -methods: - Antihydrogen trapping - Antihydrogen beam 39

40 AntihydrogenforCPT test matter-antimatter precise comparison by means of spectroscopy directexperimentaltest (no model is required) ASACUSA AEGIS Plans for antihydrogen: - measurements: - Hyperfine splitting of ground state - 1S-2S transition -methods: - Antihydrogen trapping - Antihydrogen beam 40

41 Trappedantihydrogenfor1S-2S spectroscopy 41

42 Antihydrogentrap Broken rotational symmetry: can a Penning trap be superposed? large B-fields needed for pbars trapping, cooling, etc. but large B needed for Hbartrapping 42

43 ALPHA: first trapofantihydrogen Nature 468, 673 (2010) Fast shutdown of trap magnets (9 ms) Trap depth=0.5k Hbar simulation pbar simulation 38 annihilations in 335 attempts Final number: 1 trapped Hbar per trial Trapped antihydrogen for at least 172 ms 43

44 ALPHA: trapofantihydrogenfor1000 s ALPHA Coll. Nature Physics 2011 Detection throughquenching Trapping rate Hbarsat 1S state 44

45 ATRAP: trapofantihydrogen Gabrielse et al. PRL 2012 Confinement for s High trapping rate: 5+-1 annihilations per trial 45

46 Ground-statehyperfinesplittingof antihydrogen 46

47 (Anti)hydrogen ground-state hyperfine splitting Interaction between (anti)proton and (anti)electron spin magnetic moments Between the triplet (F= 1) and singlet (F= 0) sublevels : νhfis proportional to the (anti)proton magnetic moment μp δ: higher-order QED & strong interaction corrections: ~10-3 (5 ppm2012 Gabrielse, previously 0.3%) Theoretical uncertainty on δ: ~

48 AntihydrogenGS-HFS in magneticfield Hyperfine levels depend on magnetic field: Energyincreases for (F, M) = (1, 1) and (1, 0): low-field seekers(μ< 0 ) Energy decreasesfor (F, M) = (1, 1) and (0, 0): high-field seekers(μ> 0 ) B=0 48

49 AntihydrogenGS-HFS measurement For hydrogen: precision (hydrogen maser) But maser not possible for antihydrogen Spectroscopy of trapped antihydrogen low precision due to strong confining field Spectroscopy of H_ beam far from largeb atomic beam method can work up to K (for trapped H_: << 1 K) H_ can be guided with inhomogeneous magnetic field 49

50 ALPHA: AntihydrogenGS-HFS in a trap C Amole et al., Nature 483, 439 (2012) High magnetic field Onlyproofofprinciple ( f/f=100 MHz/29 GHz= ) Start of Hbar spectroscopy 50

51 GS-HFS withantihydrogenbeam 51

52 ASACUSA Spokesperson: R. Hayano Not only antihydrogen 52

53 Schemeofthe measurement flip Hbar spin confine pbarsand e + ; select Hbar spin state select spin state HFS-states: de-focused LFS-states: focused B and E axially symmetric 53

54 Schemeofthe measurement off resonance on resonance Disappearance Mode 54

55 Schemeofthe experimentalset-up ASACUSA p e ev e + accumulator AD RFQD MUSASHI p trap cusp trap H_ beamline 5.3 MeV 115 kev 150 ev ε=25% 3D tracking detector p : accumulation(3 5 AD shots), compression in MUSASHI pulse extraction from MUSASHI transfer of tothe cusptrap guided by magnetic fields(non adiabatic transport?) e + : 22 Na source (0.6 GBq), Ne moderator, N 2 gas moderator, MRE accumulation( stacks) transfer of every 10 min to the cusp 55

56 RadiofrequencyQuadrupoleDecelerator RFQD inverse linac RFQD 56

57 Antiprotonaccumulator(MUSASHI) RFQDfoilcapturecoolwithe-compresstransport tocusp RFQD+MUSASHI 5-50 more pbars than other experiments 57

58 experimentalset-up 58

59 experimentalset-up MUSASHI MUSASHI 59

60 experimentalset-up 60

61 Antihydrogenformation 61

62 Antihydrogenformation Hbar formation p Field Ionization of Hbar ( pbar capture) 62

63 Antihydrogenformation p annihilation signal First antihydrogen production in a cusp trap 63

64 64

65 Trackingdetector 65

66 Annihilationsvertices 66

67 Annihilationsvertices 67

68 Increaseantihydrogenproduction 68

69 Fieldionizationmeasurement 69

70 Antihydrogenbeam expected polarization of antihydrogen beam 70

71 Antihydrogenbeam Not yet used Hbar detector Field Ionization before the detector OnlyHbarswithn<43 (or n<29) reachthe detector BGO measures energy deposition by Hbar annih. coincidence: BGO AND (>1 S) 71

72 Energy depositionin the BGO mostly Hbars Background = pbars e - mixing 72

73 Antihydrogensreachingthe BGO a-c (see previous slide) IntegrationfromE th to200 MeV After detection efficiency correction(from GEANT) 25 Hbars/hour(n<43) 16 Hbars/hour(n<29) 73

74 Nextsteps Study and improve the beam features(hbar numbers, temperature, n-states, ) Introduce MW cavity 74

75 Expectations D D=10 cm, v=1 km/s 1/T=10 khz f/f=7x10 6 σ=7x10 7 Achievableresolution: -betterthan10-6 fort < 100 K -100 Hbar/s in 1S state needed (in 4 π)eventrate=1/min. 1 improvement(ramsey): Linewidth reduced by D/L Antihydrogenfountain: -trapping and laser cooling - Ramsey method with L=1m Δf ~3 Hz, Δf/f~ 2x10 9 <-- AEGIS 75

76 Future ELENA decelerator: 5.3 MeV100 kev x 100 pbars trapping efficiencies 4 experiments can run in parallel 76

77 Summary Antihydrogen research: -covers many fields of physics (particle, atomic, plasma, accelerators, ) - requires modest resources (but needs time) - promises high sensitive tests of CPT symmetry - several improvements performed - recent results on production, trapping and beam formation spectroscopy era 77

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 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

More information

Antimatter. Jan Meier. Seminar: Experimental Methods in Atomic Physics May, 8th 2007

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

More information

Prospects of in-flight hyperfine spectroscopy of (anti)hydrogen for tests of CPT symmetry E. Widmann Stefan Meyer Institute for Subatomic Physics,

Prospects of in-flight hyperfine spectroscopy of (anti)hydrogen for tests of CPT symmetry E. Widmann Stefan Meyer Institute for Subatomic Physics, Prospects of in-flight hyperfine spectroscopy of (anti)hydrogen for tests of CPT symmetry Stefan Meyer Institute for Subatomic Physics, Vienna Austrian Academy of Sciences HISEBSM Rencontres de Vietnam

More information

Progress of antihydrogen beam production with the double cusp trap

Progress of antihydrogen beam production with the double cusp trap 1 / 34 Progress of antihydrogen beam production with the double cusp trap Yugo Nagata Department of applied physics, Tokyo University of Agriculture and Technology Atomic Physics Research Unit, RIKEN March

More information

Fundamental physics with antihydrogen and antiprotons at the AD. Michael Doser CERN

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

More information

Sub-Doppler two-photon laser spectroscopy of antiprotonic helium and the antiproton-toelectron

Sub-Doppler two-photon laser spectroscopy of antiprotonic helium and the antiproton-toelectron Sub-Doppler two-photon laser spectroscopy of antiprotonic helium and the antiproton-toelectron mass ratio Fukuoka, August 2012 Masaki Hori Max Planck Institute of Quantum Optics A. Sótér, D. Barna, A.

More information

In-beam measurement of the hydrogen hyperfine splitting: towards antihydrogen spectroscopy. Martin Diermaier LEAP 2016 Kanazawa Japan

In-beam measurement of the hydrogen hyperfine splitting: towards antihydrogen spectroscopy. Martin Diermaier LEAP 2016 Kanazawa Japan In-beam measurement of the hydrogen hyperfine splitting: towards antihydrogen spectroscopy Martin Diermaier LEAP 2016 Kanazawa Japan Martin Diermaier Stefan-Meyer-Institute March th 2016 MOTIVATION Charge

More information

Experiments with low energy antimatter

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

More information

Towards the production of an anti-hydrogen beam

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

More information

Observation of the 1S-2S Transition in Antihydrogen

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

More information

CPT ALPHA CPT 2.1 CPT , CERN. TRIUMF Canada s National Laboratory for Particle and Nuclear Physics

CPT ALPHA CPT 2.1 CPT , CERN. TRIUMF Canada s National Laboratory for Particle and Nuclear Physics 258 501 ALPHA (CERN) CPT, CERN ishida@icepp.s.u-tokyo.ac.jp TRIUMF Canada s National Laboratory for Particle and Nuclear Physics Makoto.Fujiwara@triumf.ca 2015 2 26 ( H ) (p ) ( e + ) CPT ( ) CERN (AD;

More information

Antiprotonic Helium: Measuring the Antiproton Mass and Magnetic Moment

Antiprotonic Helium: Measuring the Antiproton Mass and Magnetic Moment Dezső Horváth Antiprotonic Helium 10-14 September 2012, Stara Lesna, Slovakia p. 1/37 Antiprotonic Helium: Measuring the Antiproton Mass and Magnetic Moment Dezső Horváth on behalf of the ASACUSA Collaboration

More information

The CERN Antiproton Physics Programme The Antiproton Decelerator (AD) & ELENA

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

More information

Testing CPT Invariance with Antiprotonic Atoms

Testing CPT Invariance with Antiprotonic Atoms Testing CPT Invariance with Antiprotonic Atoms Dezső Horváth horvath@rmki.kfki.hu. KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary & ATOMKI, Debrecen, Hungary Outline CPT Invariance

More information

CPT symmetry test Gravity between matter and antimatter Listen to the whisper of nature (Planck mass vs our limitedness )

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

More information

ASACUSA: Measuring the Antiproton Mass and Magnetic Moment

ASACUSA: Measuring the Antiproton Mass and Magnetic Moment Dezső Horváth ASACUSA 9 October 2013, St. Petersburg, Russia p. 1/41 ASACUSA: Measuring the Antiproton Mass and Magnetic Moment Dezső Horváth on behalf of the ASACUSA Collaboration horvath.dezso@wigner.mta.hu

More information

Recent results from ATHENA

Recent results from ATHENA Recent results from ATHENA G. Bonomi a, M. Amoretti b,p.d.bowe c,c.canali bd, C. Carraro bd,c.l.cesar e,m. Charlton f,m.doser a, A. Fontana gh,m.c.fujiwara il, R. Funakoshi l, P. Genova gh,j.s.hangst c,r.s.hayano

More information

Testing CPT Invariance with Antiprotonic Atoms 1

Testing CPT Invariance with Antiprotonic Atoms 1 Testing CPT Invariance with Antiprotonic Atoms 1 Dezső Horváth KFKI Research Institute for Particle and Nuclear Physics, H 1525 Budapest, Hungary and Institute of Nuclear Research (ATOMKI), Debrecen, Hungary

More information

Proceedings of the 12th International Conference on Low Energy Antiproton Physics (LEAP216) Downloaded from journals.jps.jp by on 3/23/

Proceedings of the 12th International Conference on Low Energy Antiproton Physics (LEAP216) Downloaded from journals.jps.jp by on 3/23/ Proceedings of the 12th International Conference on Low Energy Antiproton Physics (LEAP216) Downloaded from journals.jps.jp by 128.141.46.242 on 3/23/18 Proc. 12th Int. Conf. Low Energy Antiproton Physics

More information

Experimental Tests of CPT Invariance at CERN

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

More information

The Magnetic Moment of the Proton. A. Mooser for the BASE collaboration

The Magnetic Moment of the Proton. A. Mooser for the BASE collaboration The Magnetic Moment of the Proton A. Mooser for the BASE collaboration Motivation CPT-Symmetry fundamental cornerstone of Standard Model Strategy: Compare properties of matter and antimatter conjugates

More information

Antimatter research at F(L)AIR

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

More information

High-precision measurements of the fundamental properties of the antiproton

High-precision measurements of the fundamental properties of the antiproton High-precision measurements of the fundamental properties of the antiproton Hiroki Nagahama on behalf of the BASE collaboration PSAS 2016, Jerusalem 26/May Goal of BASE Table of contents Principle of CPT

More information

arxiv: v1 [physics.ins-det] 6 Jun 2016

arxiv: v1 [physics.ins-det] 6 Jun 2016 Hyperfine Interactions manuscript No. (will be inserted by the editor) Towards Measuring the Ground State Hyperfine Splitting of Antihydrogen A Progress Report arxiv:1606.01791v1 [physics.ins-det] 6 Jun

More information

Precision tests of the Standard Model with trapped atoms 1 st lecture. Luis A. Orozco SUNYSB

Precision tests of the Standard Model with trapped atoms 1 st lecture. Luis A. Orozco SUNYSB Precision tests of the Standard Model with trapped atoms 1 st lecture Luis A. Orozco SUNYSB The Standard Model (brief review) Symmetries Conserved quantities Gauge Symmetries (local and continuous) Particles

More information

POSITRON ACCUMULATOR SCHEME for AEGIS

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-

More information

The ATHENA experiment

The ATHENA experiment The ATHENA experiment Antihydrogen at Rest for precision Tests of CPT and WEP M. H. Holzscheiter Los Alamos National Laboratory (for the ATHENA Collaboration) 1. Physics Goals 2. Antiproton Decelerator

More information

Dynamics of antiproton cooling in a positron plasma during antihydrogen formation

Dynamics of antiproton cooling in a positron plasma during antihydrogen formation Physics Letters B 590 (2004) 133 142 www.elsevier.com/locate/physletb Dynamics of antiproton cooling in a positron plasma during antihydrogen formation ATHENA Collaboration M. Amoretti a,c.amsler b, G.

More information

Ion traps. Trapping of charged particles in electromagnetic. Laser cooling, sympathetic cooling, optical clocks

Ion traps. Trapping of charged particles in electromagnetic. Laser cooling, sympathetic cooling, optical clocks Ion traps Trapping of charged particles in electromagnetic fields Dynamics of trapped ions Applications to nuclear physics and QED The Paul trap Laser cooling, sympathetic cooling, optical clocks Coulomb

More information

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 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,

More information

Finally. Thanks to the organizers for organizing this nice school. Thanks to the participants for stimulating discussions.

Finally. Thanks to the organizers for organizing this nice school. Thanks to the participants for stimulating discussions. Finally Thanks to the organizers for organizing this nice school Thanks to the participants for stimulating discussions. Unusual year for me -- no antiprotons are available at CERN -- I am on sabbatical

More information

A 680-fold improved comparison of the antiproton and proton magnetic moments

A 680-fold improved comparison of the antiproton and proton magnetic moments A 680-fold improved comparison of the antiproton and proton magnetic moments Eric Tardiff Gerald Gabrielse, Jack DiSciacca, Kathryn Marable, Mason Marshall Harvard University July 21, 2014 Testing CPT

More information

Matter, Antimatter and the Strangeness of CP violation

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

More information

Exam Results. Force between charges. Electric field lines. Other particles and fields

Exam Results. Force between charges. Electric field lines. Other particles and fields Exam: Exam scores posted on Learn@UW No homework due next week Exam Results F D C BC B AB A Phy107 Fall 2006 1 Particles and fields We have talked about several particles Electron,, proton, neutron, quark

More information

THE ELENA PROJECT AT CERN

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

More information

A Next-generation Low-energy Antiproton Facility

A Next-generation Low-energy Antiproton Facility A Next-generation Low-energy Antiproton Facility E. Widmann, University of Tokyo Chairman, FLAIR steering committee Nuclear Physics @ J-PARC Workshop NP04, Tokai, August 2 4, 2004 University of Tokyo Antiproton

More information

THE ALPHA COLLABORATION

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

More information

GBAR Project Gravitational Behavior of Antihydrogen at Rest

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

More information

The First Cold Antihydrogen *

The First Cold Antihydrogen * The First Cold Antihydrogen * M.C. Fujiwara ab, M. Amoretti c, C. Amsler d, G. Bonomi e, A.Bouchta e, P.D. Bowe f, C. Carraro cg C.L. Cesar h, M. Charlton i, M. Doser e, V. Filippini j, A. Fontana jk,

More information

Laser driven Positronium excitation in the AEGIS antimatter

Laser driven Positronium excitation in the AEGIS antimatter Laser driven Positronium excitation in the AEGIS antimatter experiment at CERN F. Castelli Dipartimento di Fisica, Università degli Studi di Milano, and INFN Sezione di Milano, Italy M.G. Giammarchi Istituto

More information

Units and dimensions

Units and dimensions Particles and Fields Particles and Antiparticles Bosons and Fermions Interactions and cross sections The Standard Model Beyond the Standard Model Neutrinos and their oscillations Particle Hierarchy Everyday

More information

Temporally Controlled Modulation of Antihydrogen Production and the Temperature Scaling of Antiproton-Positron Recombination

Temporally Controlled Modulation of Antihydrogen Production and the Temperature Scaling of Antiproton-Positron Recombination Temporally Controlled Modulation of Antihydrogen Production and the Temperature Scaling of Antiproton-Positron Recombination M. C. Fujiwara, 1,2, * M. Amoretti, 3 C. Amsler, 4 G. Bonomi, 5,6 A. Bouchta,

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

The GBAR experiment. Dirk van der Werf

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

More information

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e +

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e + β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Last Lecture: Radioactivity, Nuclear decay Radiation damage This lecture: nuclear physics in medicine and fusion and fission Final

More information

This content has been downloaded from IOPscience. Please scroll down to see the full text.

This content has been downloaded from IOPscience. Please scroll down to see the full text. This content has been downloaded from IOPscience. Please scroll down to see the full text. Download details: IP Address: 148.251.232.83 This content was downloaded on 06/04/2018 at 00:28 Please note that

More information

Antihydrogen production temperature dependence

Antihydrogen production temperature dependence Physics Letters B 583 (2004) 59 67 www.elsevier.com/locate/physletb Antihydrogen production temperature dependence ATHENA Collaboration M. Amoretti a,c.amsler b, G. Bazzano c, G. Bonomi d,, A. Bouchta

More information

Recent results on the antiproton-nucleus annihilation cross section at low energy

Recent results on the antiproton-nucleus annihilation cross section at low energy Recent results on the antiroton-nucleus annihilation cross section at low energy Luca Venturelli for H. Aghai-Khozani 1, M. Corradini 2, R. Hayano 3, M. Hori 1, M.Leali 2, E. Lodi-Rizzini 2, V. Mascagna

More information

On the Possibility of Non-Neutral Antiproton Plasmas and Antiproton-Positron Plasmas

On the Possibility of Non-Neutral Antiproton Plasmas and Antiproton-Positron Plasmas On the Possibility of Non-Neutral Antiproton Plasmas and Antiproton-Positron Plasmas H. Higaki Plasma Research Center, University of Tsukuba 1-1-1, Tennoudai, Tsukuba, Ibaraki, Japan 305-8577 Abstract.

More information

First Attempts at Antihydrogen Trapping in ALPHA

First Attempts at Antihydrogen Trapping in ALPHA First Attempts at Antihydrogen Trapping in ALPHA G.B. Andresen,W.Bertsche,P.D.Bowe,C.C.Bray, E. Butler,C.L. Cesar,S.Chapman,M.Charlton, J. Fajans, M.C. Fujiwara,R. Funakoshi,D.R.Gill,J.S.Hangst,W.N.Hardy,

More information

Lecture 11. Weak interactions

Lecture 11. Weak interactions Lecture 11 Weak interactions 1962-66: Formula/on of a Unified Electroweak Theory (Glashow, Salam, Weinberg) 4 intermediate spin 1 interaction carriers ( bosons ): the photon (γ) responsible for all electromagnetic

More information

ANTIMATTER MATTER. does the difference between matter and antimatter arise?

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.

More information

Atomic Physics in Traps

Atomic Physics in Traps Atomic Physics in Traps QED Fundamental Constants CPT Invariance Wolfgang Quint GSI Darmstadt and Univ. Heidelberg Quantum mechanics, Relativity, and P.A.M. Dirac Quantum mechanics Special Relativity Dirac

More information

Gravitational Repulsion of Matter and Antimatter

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

More information

Precision Penning Trap Experiments with Exotic Ions

Precision Penning Trap Experiments with Exotic Ions Klaus.blaum@mpi-hd.mpg.de EMMI Physics Days 2011, GSI Darmstadt Precision Penning Trap Experiments with Exotic Ions Klaus Blaum November 08, 2011 Outline Introduction and motivation Principle of Penning

More information

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 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

More information

TAMU-TRAP facility for Weak Interaction Physics. P.D. Shidling Cyclotron Institute, Texas A&M University

TAMU-TRAP facility for Weak Interaction Physics. P.D. Shidling Cyclotron Institute, Texas A&M University TAMU-TRAP facility for Weak Interaction Physics P.D. Shidling Cyclotron Institute, Texas A&M University Outline of the talk Low energy test of Standard Model T =2 Superallowed transition Facility T-REX

More information

The ATHENA experiment for the study of antihydrogen

The ATHENA experiment for the study of antihydrogen International Journal of Modern Physics A Vol. 29, No. 20 (2014) 1430035 (75 pages) c World Scientific Publishing Company DOI: 10.1142/S0217751X1430035X C. Amsler, G. Bonomi,, A. Fontana, A. Kellerbauer,,

More information

Emerging science and technology of antimatter plasmas and trap-based beams a

Emerging science and technology of antimatter plasmas and trap-based beams a PHYSICS OF PLASMAS VOLUME 11, NUMBER 5 MAY 2004 Emerging science and technology of antimatter plasmas and trap-based beams a C. M. Surko b) Department of Physics, University of California, San Diego, 9500

More information

New and accelerator research facility, using MW-class high power proton beams at both 3 GeV and 30 GeV. J-PARC Tokai KEK Tsukuba LINAC 400 MeV Rapid Cycle Synchrotron Energy : 3 GeV Repetition : 25 Hz

More information

Møller Polarimetry on Atomic Hydrogen

Møller Polarimetry on Atomic Hydrogen E.Chudakov June 21, 2011 Møller Polarimetry on Atomic Hydrogen 1 Møller Polarimetry on Atomic Hydrogen E.Chudakov 1 1 JLab Meeting at UVA Outline E.Chudakov June 21, 2011 Møller Polarimetry on Atomic Hydrogen

More information

Essentials of Particle Physics

Essentials of Particle Physics Essentials of Particle Physics Kajari Mazumdar Department of High Energy Physics Tata Institute of Fundamental Research Mumbai http://www.tifr.res.in/~mazumdar Kajari.Mazumdar@gmail.com KSTA Lecture Series

More information

Precision Penning Trap Experiments with Exotic Ions

Precision Penning Trap Experiments with Exotic Ions Klaus.blaum@mpi-hd.mpg.de Hirschegg 2012 Precision Penning Trap Experiments with Exotic Ions Klaus Blaum January 16, 2012 Outline Introduction and motivation Principle of Penning traps Setup and measurement

More information

ALICE, ATLAS, CMS, LHCb, TOTEM, LHCf

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

More information

Possibilities for a Bose-Einstein Condensed Positronium Annihilation Gamma Ray Laser

Possibilities for a Bose-Einstein Condensed Positronium Annihilation Gamma Ray Laser Possibilities for a Bose-Einstein Condensed Positronium Annihilation Gamma Ray Laser Allen Mills, Jr., University of California Riverside in collaboration with David Cassidy and Harry Tom (UCR) Rod Greaves

More information

Clock based on nuclear spin precession spin-clock

Clock based on nuclear spin precession spin-clock Clock based on nuclear spin precession spin-clock signal (a.u.) detector t exp - T (G. D. Cates, et al., Phys. Rev. A 37, 877) T T T, field T, field 4 4R 75D B, z B, y B, x R 4 p B (ms ) T 00h Long T :

More information

Antihydrogen for precision tests in physics

Antihydrogen for precision tests in physics Contemporary Physics Vol. 49, No. 1, January February 2008, 29 41 Antihydrogen for precision tests in physics M. Charlton*, S. Jonsell, L.V. Jørgensen, N. Madsen and D.P. van der Werf Department of Physics,

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

Continuous Stern-Gerlach effect and the Magnetic Moment of the Antiproton

Continuous Stern-Gerlach effect and the Magnetic Moment of the Antiproton Continuous Stern-Gerlach effect and the Magnetic Moment of the Antiproton W. Quint a, J. Alonso b, S. Djekić b, H.-J. Kluge a, S. Stahl b, T. Valenzuela b, J. Verdú b, M. Vogel b, and G. Werth b a Gesellschaft

More information

Equivalence principle for free and bound antiparticles

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

More information

Study on positronium Bose-Einstein condensation

Study on positronium Bose-Einstein condensation Study on positronium Bose-Einstein condensation Akira Ishida a,*, K. Shu a, T. Murayoshi a, X. Fan a, T. Namba a,s. Asai a, K. Yoshioka b, M. Kuwata-Gonokami a, N. Oshima c, B. E. O Rourke c, R. Suzuki

More information

Evidence For The Production Of Slow Antiprotonic Hydrogen In Vacuum

Evidence For The Production Of Slow Antiprotonic Hydrogen In Vacuum PRL 97, 534 (6) 3 OCTOBER 6 Evidence For The Production Of Slow Antiprotonic Hydrogen In Vacuum N. Zurlo,, M. Amoretti, 3 C. Amsler, 4 G. Bonomi, 5,6 C. Carraro, 3,7 C. L. Cesar, 8 M. Charlton, 9 M. Doser,

More information

\ \ \/ \\// (o) (o) U. February 11, UT Saturday Morning Physics. Yuri Kamyshkov University of Tennessee

\ \ \/ \\// (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,

More information

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG

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

More information

Two-stage Rydberg charge exchange in a strong magnetic field

Two-stage Rydberg charge exchange in a strong magnetic field Two-stage Rydberg charge exchange in a strong magnetic field M. L. Wall, C. S. Norton, and F. Robicheaux Department of Physics, Auburn University, Auburn, Alabama 36849-5311, USA Received 21 June 2005;

More information

ASACUSA STATUS REPORT

ASACUSA STATUS REPORT January, 29 ASACUSA STATUS REPORT ASACUSA progress during 28 and plans for 29 CERN-SPSC-29-5 / SPSC-SR-4 27/1/29 ASACUSA collaboration D. Barna 1,6, M. Charlton 2, M. Corradini 3, A. Dax 1, H. Dølrath

More information

Spectra of Cosmic Rays

Spectra of Cosmic Rays Spectra of Cosmic Rays Flux of relativistic charged particles [nearly exactly isotropic] Particle density Power-Law Energy spectra Exponent (p, Nuclei) : Why power laws? (constraint on the dynamics of

More information

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

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..............................

More information

Detection of trapped antihydrogen in ALPHA

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

More information

Frontier Science: The mystery of Antimatter

Frontier Science: The mystery of Antimatter Frontier Science: The mystery of Antimatter Cristina Lazzeroni Professor in Particle Physics STFC Public Engagement Fellow ASE Frontier Science Lecture University of Birmingham Poynting Physics S02 7th

More information

Space-Time Symmetries

Space-Time Symmetries Space-Time Symmetries Outline Translation and rotation Parity Charge Conjugation Positronium T violation J. Brau Physics 661, Space-Time Symmetries 1 Conservation Rules Interaction Conserved quantity strong

More information

Neutrino Helicity Measurement

Neutrino Helicity Measurement PHYS 851 Introductory Nuclear Physics Instructor: Chary Rangacharyulu University of Saskatchewan Neutrino Helicity Measurement Stefan A. Gärtner stefan.gaertner@gmx.de December 9 th, 2005 2 1 Introduction

More information

High rate production of antihydrogen

High rate production of antihydrogen Physics Letters B 578 (2004) 23 32 www.elsevier.com/locate/physletb High rate production of antihydrogen ATHENA Collaboration M. Amoretti a,c.amsler b, G. Bazzano c,d, G. Bonomi e, A. Bouchta e,p.bowe

More information

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst Electroweak Physics Krishna S. Kumar University of Massachusetts, Amherst Acknowledgements: M. Grunewald, C. Horowitz, W. Marciano, C. Quigg, M. Ramsey-Musolf, www.particleadventure.org Electroweak Physics

More information

The achievements of the CERN proton antiproton collider

The achievements of the CERN proton antiproton collider The achievements of the CERN proton antiproton collider Luigi DiLella Scuola Normale Superiore, Pisa, Italy Motivation of the project The proton antiproton collider UA1 and UA2 detectors Discovery of the

More information

Polarised Gas Targets and Polarised Ion Sources for Accelerators

Polarised Gas Targets and Polarised Ion Sources for Accelerators Polarised Gas Targets and Polarised Ion Sources for Accelerators Geoff Court Physics Dept., Liverpool University Mainly principles time limitation Protons only ideas apply for other nuclei (D, 3 He..)

More information

Search for a Permanent Electric Dipole Moment in Ra EDM Spin EDM Spin EDM. Spin. Pseudo-scalar. s d

Search for a Permanent Electric Dipole Moment in Ra EDM Spin EDM Spin EDM. Spin. Pseudo-scalar. s d Search for a Permanent Electric Dipole Moment in Ra-225 + T + P - - - + EDM Spin EDM Spin EDM Spin Pseudo-scalar s d C. S. Wu 1912-1997 Parity (space reversal) x, y, z -x, -y, -z z y Parity z x x y Pseudo-scalar

More information

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 14: CP and CP Violation

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 14: CP and CP Violation Particle Physics Dr Victoria Martin, Spring Semester 01 Lecture 14: CP and CP Violation!Parity Violation in Weak Decay!CP and CPT!Neutral meson mixing!mixing and decays of kaons!cp violation in K 0 and

More information

Quadrupole Induced Resonant Particle Transport in a Pure Electron Plasma

Quadrupole Induced Resonant Particle Transport in a Pure Electron Plasma Quadrupole Induced Resonant Particle Transport in a Pure Electron Plasma E. Gilson 1 and J. Fajans 2 Department of Physics University of California, Berkeley Berkeley, California, 94720-7300 Abstract.

More information

AEGIS. Antihydrogen Experiment: Gravity, Interferometry, Spectroscopy University of Oslo - H. Sandaker

AEGIS. Antihydrogen Experiment: Gravity, Interferometry, Spectroscopy University of Oslo - H. Sandaker AEGIS Antihydrogen Experiment: Gravity, Interferometry, Spectroscopy AEGIS experiment - Importance of anti-matter research We observe a matter-antimatter asymmetry in the Universe We expect there to be

More information

Study on Bose-Einstein Condensation of Positronium

Study on Bose-Einstein Condensation of Positronium Study on Bose-Einstein Condensation of Positronium K. Shu 1, T. Murayoshi 1, X. Fan 1, A. Ishida 1, T. Yamazaki 1,T. Namba 1,S. Asai 1, K. Yoshioka 2, M. Kuwata-Gonokami 1, N. Oshima 3, B. E. O Rourke

More information

Fundamentals in Nuclear Physics

Fundamentals in Nuclear Physics Fundamentals in Nuclear Physics Kenichi Ishikawa () http://ishiken.free.fr/english/lecture.html ishiken@n.t.u-tokyo.ac.jp 1 Nuclear decays and fundamental interactions (II) Weak interaction and beta decay

More information

Physics 2D Lecture Slides Jan 22. Vivek Sharma UCSD Physics

Physics 2D Lecture Slides Jan 22. Vivek Sharma UCSD Physics Physics 2D Lecture Slides Jan 22 Vivek Sharma UCSD Physics Nuclear Fusion : What Powers the Sun Opposite of Fission Mass of a Nucleus < mass of its component protons+neutrons Nuclei are stable, bound

More information

novel DIagnostic Techniques for future particle Accelerators: A Marie Curie Initial Training NETwork

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

More information

Study of the hyperfine structure of antiprotonic helium

Study of the hyperfine structure of antiprotonic helium Nuclear Instruments and Methods in Physics Research B 214 (2004) 89 93 www.elsevier.com/locate/nimb Study of the hyperfine structure of antiprotonic helium J. Sakaguchi a, J. Eades a, R.S. Hayano a, M.

More information

Propagation in the Galaxy 2: electrons, positrons, antiprotons

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

More information

Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places

Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places The 64 th Compton Lecture Series Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places http://kicp.uchicago.edu/~odom/compton.htm Lecture 5: Using the Fine Structure Constant to Push

More information

Dark Energy or Repulsive Gravity

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

More information

Cavity Control in a Single-Electron Quantum Cyclotron

Cavity Control in a Single-Electron Quantum Cyclotron Cavity Control in a Single-Electron Quantum Cyclotron An Improved Measurement of the Electron Magnetic Moment David Hanneke Michelson Postdoctoral Prize Lectures 13 May 2010 The Quantum Cyclotron Single

More information

EDM. Spin. ν e. β - Li + Supported by DOE, Office of Nuclear Physics

EDM. Spin. ν e. β - Li + Supported by DOE, Office of Nuclear Physics T + - + - He Ra EDM Spin EDM Spin β - θ ν e He Kr 6 He 6 Li + Supported by DOE, Office of Nuclear Physics Search for a Permanent Electric Dipole Moment in Ra-225 + T + P - - - + EDM Spin EDM Spin EDM Spin

More information