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First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV / AMS Collaboration
A precision measurement by the Alpha Magnetic Spectrometer on the International Space Station of the positron fraction in primary cosmic rays in the energy range from 0.5 to 350 GeV based on 6.8×106 positron and electron events is presented. The very accurate data show that the positron fraction is steadily increasing from 10 to ∼250 GeV, but, from 20 to 250 GeV, the slope decreases by an order of magnitude. [...]
2013 - 10 p. - Published in : Phys. Rev. Lett. 110 (2013) 141102 External links: Interactions.org article; Symmetry Magazine article; Press Release

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The Alpha Magnetic Spectrometer (AMS) on the International Space Station. I: Results from the test flight on the space shuttle / AMS Collaboration
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km . A search for antihelium nuclei in the rigidity range 1– 140 GV was performed. [...]
2002 - 75 p. - Published in : Phys. Rep. 366 (2002) 331-405
- Published in : Phys. Rep. 380 (2003) 97-98

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Isotopic Composition of Light Nuclei in Cosmic Rays: Results from AMS-01 / AMS-01 Collaboration
The variety of isotopes in cosmic rays allows us to study different aspects of the processes that cosmic rays undergo between the time they are produced and the time of their arrival in the heliosphere. In this paper, we present measurements of the isotopic ratios $^2$H/$^4$He, $^3$He/$^4$He, $^6$Li/$7$Li, $7$Be/($^9$Be+$^{10}$Be), and $^{10}$B/$^{11}$B in the range 0.2-1.4 GeV of kinetic energy per nucleon. [...]
arXiv:1106.2269.- 2011 - 12 p. - Published in : Astrophys. J. 736 (2011) 105 Fulltext: PDF; External link: Preprint

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Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01 / AMS-01 Collaboration
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. [...]
arXiv:1008.5051.- 2010 - 13 p. - Published in : Astrophys. J. 724 (2010) 329-340 Fulltext: PDF; External link: Preprint

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Observation of a resonance in the K$_s$p decay channel at a mass of 1765 MeV/c$^2$ / WA89 Collaboration
We report on the observation of a K$_s$p resonance signal at a mass of 1765$\pm$5 MeV/c$^2$, with intrinsic width $\Gamma = 108\pm 22$ MeV/c$^2$, produced inclusively in $\Sigma^-$-nucleus interactions at 340 GeV/c in the hyperon beam experiment WA89 at CERN. The signal was observed in the kinematic region $x_F>0.7$, in this region its production cross section rises approximately linearly with $(1-x_F)$, reaching $BR(X\to K_S p)\cdot d\sigma /dx_F = (5.2\pm 2.3) \mu b $ per nucleon at $x_F=0.8$. [...]
hep-ex/0702044.- 2007 - 5 p. - Published in : Eur. Phys. J. C 50 (2007) 535-538 Access to fulltext document: PDF; Fulltext: PDF; External link: hep-ex/0702044 PDF

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Spectra and correlations of Λ and Λ̅ produced in 340-GeV/c Σ-+C and 260-GeV/c n+C interactions / Adamovich, M I (Moscow Lebedev Physics Institute) ; Walcher, C (Univ. Mainz) ; Wälder,G (Univ. Heidelberg) ; Werding, R (Max-Planck-Institut für Kernphysik, Heidelberg) ; Wittmann, E (Max-Planck-Institut für Kernphysik, Heidelberg) ; Zavertyaev, M V (Moscow Lebedev Physics Institute) ; Pochodzalla, J (Max-Planck-Institut für Kernphysik, Heidelberg) ; Potashnikova, I K (Max-Planck-Institut für Kernphysik, Heidelberg) ; Povh, B (Max-Planck-Institut für Kernphysik, Heidelberg) ; Ransome, R (Rutgers, Univ. New Jersey) et al.
2002 - Published in : Phys. Rev. C 65 (2002) 42202-42206 APS Published version, local copy: PDF;

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Observation of rainbow scattering in the 12C+12C system at Ec.m.=508 MeV / Buenerd,M (Centre d'Etudes Nucléaires, Grenoble) ; Schröder, B (Univ. of Lund, Sweden) ; Tibell, G (Univ. of Uppsala, Sweden) ; Ryde, H (Univ. of Lund, Sweden) ; Otterlund, I (Univ. of Lund, Sweden) ; Oskarsson, A (Univ. of Lund, Sweden) ; Nielsen, O B (Niels Bohr Institute, Danemark) ; Kristiannson, P (Univ. of Lund, Sweden) ; Gustaffson, H A (CERN) ; Jakobsson, B (Univ. of Lund, Swden) et al.
1982 - Published in : Phys. Rev. C 26 (1982) 1299-1301 APS Published version, local copy: PDF;

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The AMS02 Cherenkov imager prototype : In-beam tests with high-energy ions / Buénerd, Michel /AMS-RICH Collaboration
A prototype of the AMS Cherenkov imager has been tested at CERN with 20 and per nucleon ion obtained by fragmentation of a primary beam of Pb and In ions, respectively. Data have been collected with single low-intensity beam settings, over the range of nuclear charges 2<Z45 in various beam conditions and using different radiators. [...]
2005 - Published in : Nucl. Instrum. Methods Phys. Res., A 553 (2005) 264-267

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A measurement of $\Xi^{-}$ polarization in inclusive production by $\Sigma^{-}$ of 340 GeV/c in C and Cu targets / WA89 Collaboration
We have measured the polarization of Xi /sup -/ hyperons produced inclusively by a Sigma /sup -/ beam of 340 GeV/c momentum in nuclear targets. From a sample of 880000 identified Xi /sup -/ decays, polarizations were determined in the range 0<x/sub F/<0.9 and p/sub t /<or=1.6 GeV/c. [...]
2004 - Published in : Eur. Phys. J. C 36 (2004) 315-321

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10.

The TOTEM experiment / Avati, V ; Bergholm, V ; Boccone, V ; Bozzo, M ; Buénerd, M ; Buzzo, A ; Cereseto, R ; Cuneo, S ; Da Vià, C ; Deile, M et al.
2004 - Published in : Eur. Phys. J. C 34 (2004) s255-s268
In : 4th International Symposium on LHC : Physics and Detectors, Batavia, IL, USA, 1 - 3 May 2003, pp.s225-s268

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Sehen Sie auch: ähnliche Autornamen
85	Buenerd, M
1	Buenerd, M J
85	Buénerd, M
17	Buénerd, M.
3	Buénerd, Michel

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