Rare Components in Cosmic Rays with AMS-02
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1 Rare Components in Cosmic Rays with AMS-02 TAUP Sendai Sep.07 IEKP - Andreas Sabellek Universität (TH) for the AMS Collaboration
2 The AMS Project: History and Future again ready for launch AMS-01 Alpha Magnetic Spectrometer AMS days Precursor Flight on board the Space Shuttle Discovery Spectra of primary and secondary p,e and He M. Aguilar et al., Physics Reports, vol. 366/6 (Aug.2002), pp years on the International Space Station ISS with 1000-times higher statistics measurement Superconducting magnet and new subdetectors for better particle identification: Precise antimatter and heavy nuclei fluxes measurement 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.2
3 Outline AMS-02 Experiment on board the ISS Science with AMS-02 and Achievement Potential Standard Cosmology : Cosmic Ray Spectra and Composition Gamma ray astrophysics Indirect Dark Matter Search Direct Search for Antimatter (a heavy Anti-nuceus) Search or Exotic Matter: Strangelets, Flight Status and Summary AMS-02 will record about 2 * physics events from comic rays in 3 years and identify its rare components with excellent paticle identification 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.3
4 The AMS-02 Detector Dimensions: 7 tons and 3x3x3.5 m 3 Acceptance: 0.5m 2 sr Lifetime (cryomagnet): min 3 years Redundant measurement in different subdetectors to gain precision 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.4
5 Flight Subdetector Hardware Superconducting Magnet: Field 0.86 Tesla; 5.2 MJ stored NbTi/Copper conductor I~460A; Cooled to 1.8K by 2500l Superfluid Helium B From 120 GeV/c muon beam 8 Plane Silicon Tracker: 200,000 channels on 6.6m 2 strips Resolution σ=30µm and 10µm in bending direction Rigidity measurement up to few TeV Particle identification by de/dx ~Z 2 Measurement of gammes in conversion mode Anticoincidence counters: 16 cylindrical shell paddels of plastic scintillator for veto 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.5
6 Flight Subdetector Hardware 2 m Transition Radiation Detector: 20 layers, 5248 strawtubes with Xe/CO 2 1bar Fleece radiator for electron/proton separation e/h rejection > 100 de/dx measurement Time of Flight: 2x2 scintillator planes as primary trigger Resolution t<130ps Velocity measurement dβ/β~3% de/dx measurement 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.6
7 Flight Subdetector Hardware Ring Image Cherenkov Detector: NaF (n=1.336) and Aerogel (n=1.035) radiator PMT s array of spatial pixel size 8.5x8.5 mm β measurement up to 20GeV/n Charge measurement up to Z=26 (Nγ~Z 2 ) Radiator (NaF and Aerogel) Electromagnetic Calorimeter: 18 planes (640kg) of Pb with scintillator fiber Reflector inserts; thickness 16X 0 /.5λ h e/p separation ~1000 to 1Tev de/e= /se[gev] PMT array Space qualified electronics running with 650 micropocessors to read out channels, GPS, Startracker Camera and heat control systems. 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.7
8 Photon Detection with AMS-02 Single photon mode Energy resolution (100GeV) ~3% 3% γ EM Shower Conversion mode Angular resolution (100GeV) ~0.02 γ e + /e - -pair /09/2007 TAUP 07, Sendai Andreas Sabellek p.8
9 Chemical Composition Univ. of Measurement Test results from accelerator 158 GeV/n Abundance of cosmic nuclei de/dx~z 2 Nγ~Z 2 p B Ne P Ca MnCo Cosmic spectra with 1% accuracy from Helium to Cobalt 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.9
10 Precision Study of Cosmic Rays Univ. of Radioactive Isotopes AMS-02 will collect Be isotopes in 3 years Half-life of 10 Be in the order of confinement time Information about Confinement time Galactic halo size 0.4 AMS-02 (6 months) B / C Dwyer et al. HEAO ISEE-3 Spacelab Strong & Moskalenko Kinetic Energy (GeV/n) and collect 10 5 C and 10 4 B to measure the ratio of Carbon to its spallation secondary Boron up to 1TeV/n Information about Amount of matter traversed Diffusion (to understand propagation and to fix free parameters of models) 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.10
11 Isotope Identification AMS-02 can destinguish 4 He and 3 He There is room for discoveries in different channels Unexpected result from AMS-01: He Isotopes are completely separated AMS-02 is also a long duration cosmic radiation monitor (e.g. solar modulation) 3 He / 4 He AMS-02 (1 day) SMILI IMAX BESS Davis et al Kinetic Energy (GeV/n) from AMS-01 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.11
12 Diffuse Gamma Rays and Sky Univ. of Survey Two complementary modes for Gamma detection Main source: cosmic ray interaction with gas (Pion decay, Bremsstrahlung, Inverse Compton) Information about Interstellar matter Accelerating processes and origin of cosmic rays in standard astrophysics 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.12
13 Probe the Unknown Dark Energy ~73% Matter ~27% ~4.4% Barions (~0.5% Stars) 23% Cold Dark Matter From CMB + SN1a + structure formation Leading idea is some kind of not-yet-seen stable particle (WIMP candidate: Neutralino as lightest SUSY-particle in R-conserving model) Direct search on Earth ongoing (if the Earth not in a void, results expected) Indirect searches are based on χ + χ bb quark pair production in annihilation, its decay then is well known from accelerator experiments 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.13
14 Search for Cold Dark Matter Univ. of Annihilation Antiprotons Antielectrons J.J Beatty et al., PRL 93 (2004) (Projected spectrum from cosmic ray collisions) AMS-02 will at the same time measure p - and e + spectra, which may contain an antimatter excess from annihilating dark matter particles 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.14
15 Dark Matter Fit in different Sky Univ. of EGRET Data Directions W. de Boer et al. Univ. of inner Galaxy outer disc outer Galaxy low latitude intermediate lat. galactic poles 3 components gamma spectrum: galactic background + extragalactic bg + DM annihilation fitted simultaneously with same WIMP mass in all directions. 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.15
16 Dark Matter Ring Interpretation Univ. of Fit in 180 directions implies substructure in the galactic distribution. Observed rotation curve of our galaxy then can be very well explained with obtained dark matter profile. Inner ring (coincidences with H 2 ring) Outer ring (coincidences with orbit of dwarf galaxy, which looses mass by tidal forces) W. de Boer, C. Sander, V. Zhukov, A. Gladyshev, D. Kazakov, EGRET excess of diffuse Galactic Gamma Rays as Tracer of DM, astro-ph/ , A&A, 444 (2005) 51 Promising hint for annihilation of 60 GeV WIMP from Gamma rays: Verification of EGRET data necessary! Theory could allow to predict mass spectrum of SUSY from annihilation, which could be checked with accelerators. 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.16
17 Combined Analysis Charged Particles Univ. of Positrons Antiprotons Signal Background Signal Background Fluxes of Positrons and Antiprotons dependent on propagation models, but Dark Matter Annihilation with same Halo and WIMP parameters from Gamma Rays could (as input) be used to tune cosmic models, e.g. introduce unisotropic diffusion. 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.17
18 Search for Neutralino DM with Univ. of Anti-Deuterons Antideuterons in standard astrophysics are produced with high energies, whereas antideuterons from Neutralino annihilation can be found below 1 GeV. This is more promising than antiprotons since easier extraction of SUSY signal (orders of magn.!!). Antideuterons from F, Giovacchini (2007) years Φ SUSY / Φ sec 1 A large acceptance spectrometer like AMS-02 is required to measure the extremely low fluxes. 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.18
19 Kaluza-Klein Klein Bosons as Dark Univ. of Matter Candidates Low Scale Quantum Gravity (extra-dimensional) predicts Bosons with mass, allowing direct annihilation into e +/ e - pairs (dominant channel ~20%). steep spectra from BB collisions are different from neutralino annihilation Excess from possible Boson mass of 300 GeV can be seen by AMS-02 H.C.Cheng, J.L.Feng and K.T.Matchev, Phys.Rev.Lett V89, N21 (2002) ; J.Feng,Nucl.Phys.Proc.Suppl.134 (2004) 95 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.19
20 Search for the existence of Univ. of Antimatter in the Universe The primordial antimatter content of the Universe is unknown. Up to today existance of antimatter domains in the universe is not excluded (predicted by Big Bang) No antimatter annihilation signal from within our cluster No antimatter particle found by AMS-02 means there is no Antimatter in the Universe He/He (CL 95%) A single anti-c: there are antimatter stars! 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.20
21 Example for Exotic Matter in the Univ. of Universe: Strangelets Signature of a Strangelet event simply is anomalous Z/A STRANGELET Nucleus s d u s u s d d s d u s Z~0.3A 2/3 Z/A < 0.12 d u s d u u One anomalous event was reported by AMS-01 (background probability <10-3 ), compatible with a Strangelet. Stable strange quark matter was first proposed by E. Witten, Phys. Rev. D, (1984) Could there be another new type of matter? 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.21
22 AMS-02 Flight Status Final Detector Intergation at CERN,Geneva cleanroom in progress CERN Cleanroom and completed for detector test at ESTEC,NL space simulating chamber in Summer 2008 Jul.07 AMS-02 is strongly supported by NASA and on schedule for delivery to KSC, Florida in December 2008 ISS constuction continued 06 Kennedy-Space-Center today 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.22
23 Summary AMS-02 perfectly complements current big experiments in exploring new physics and is a general purpose instrument It will take high statistics and long duration cosmic ray data on board ISS and is ready for launch early 2009 It will provide simultaneous measurements to tune parameters of current cosmic models allow combined dark matter search on matter/antimatter ratios and Gamma ray spectra AMS-02 will strongly extend limits on direct searches for heavy Antimatter as well as exotics in the Universe Thank you! 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.23
24 Backups 11/09/2007 TAUP 07, Sendai Andreas Sabellek p.24
25 Current Experiments R. Battiston, Direct Measurements and Origin of CR, ICRC, /09/2007 TAUP 07, Sendai Andreas Sabellek p.25
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