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Related papers: Astroparticle Physics with AMS02

200 papers

In this work we perform a comprehensive statistical analysis of the AMS-02 electron, positron fluxes and the antiproton-to-proton ratio in the context of a simplified dark matter model. We include known, standard astrophysical sources and a…

High Energy Physics - Phenomenology · Physics 2016-05-25 Csaba Balázs , Tong Li

This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlier phase of the telescope, called AMANDA-B10, demonstrate…

Astrophysics · Physics 2015-06-24 Steven W. Barwick

Composition and spectra of Galactic cosmic rays (CRs) are vital for studies of high-energy processes in a variety of environments and on different scales, for interpretation of gamma-ray and microwave observations, disentangling possible…

The AMS-02 collaboration has just released its first result of the cosmic positron fraction $e^+/(e^-+e^+)$ with high precision up to $\sim 350$ GeV. The AMS-02 result shows the same trend with the previous PAMELA result, which requires…

High Energy Astrophysical Phenomena · Physics 2014-07-15 Qiang Yuan , Xiao-Jun Bi , Guo-Ming Chen , Yi-Qing Guo , Su-Jie Lin , Xinmin Zhang

The Altcriss project aims to perform a long term survey of the radiation environment on board the International Space Station. Measurements are being performed with active and passive devices in different locations and orientations of the…

GRAMS (Gamma-Ray and AntiMatter Survey) is a novel project that can simultaneously target both astrophysical observations with MeV gamma rays and an indirect dark matter search with antimatter. The GRAMS instrument is designed with a…

High Energy Astrophysical Phenomena · Physics 2019-12-06 Tsuguo Aramaki , Per Hansson Adrian , Georgia Karagiorgi , Hirokazu Odaka

We analyze the electron cosmic-ray spectrum from AMS-02, focusing on the spectral hardening around 42 GeV. Our findings confirm that this feature is intrinsic to the primary electron component rather than a byproduct of contamination from…

High Energy Astrophysical Phenomena · Physics 2025-03-04 Carmelo Evoli

The CALorimetric Electron Telescope (CALET) is a high-energy astroparticle physics space experiment installed on the International Space Station (ISS), developed and operated by Japan in collaboration with Italy and the United States. The…

The magnetised solar wind modulates the Galactic cosmic ray flux in the heliosphere up to rigidities as high as 40 GeV. In this work, we present a new and straightforward extension of the popular, but limited force-field model, thus…

High Energy Astrophysical Phenomena · Physics 2019-12-25 Marco Kuhlen , Philipp Mertsch

GLAST, a detector for cosmic gamma rays in the range from 20 MeV to 300 GeV, will be launched in space in 2005. Breakthroughs are expected in particular in the study of particle acceleration mechanisms in space and of gamma ray bursts, and…

Astrophysics · Physics 2016-11-03 Alessandro de Angelis

Cosmic-ray positrons have long been considered a powerful probe of dark matter annihilation. In particular, myriad studies of the unexpected rise in the positron fraction have debated its dark matter or pulsar origins. In this paper, we…

High Energy Astrophysical Phenomena · Physics 2022-01-07 Isabelle John , Tim Linden

Isochronous mass spectrometry (IMS) in storage rings is a powerful tool for mass measurements of exotic nuclei with very short half-lives down to several tens of microseconds, using a multicomponent secondary beam separated in-flight…

Our ability to identify the sources of cosmic rays and understand how these particles propagate through the interstellar medium is hindered by the combined effects of the solar wind and its embedded magnetic field, collectively known as…

High Energy Astrophysical Phenomena · Physics 2020-07-03 Ilias Cholis , Dan Hooper , Tim Linden

Measurements of redshifted 21-cm emission of neutral hydrogen at <30 MHz have the potential to probe the cosmic "dark ages," a period of the universe's history that remains unobserved to date. Observations at these frequencies are…

Instrumentation and Methods for Astrophysics · Physics 2020-11-24 H. C. Chiang , T. Dyson , E. Egan , S. Eyono , N. Ghazi , J. Hickish , J. M. Jauregui-Garcia , V. Manukha , T. Menard , T. Moso , J. Peterson , L. Philip , J. L. Sievers , S. Tartakovsky

The Any Light Particle Search II (ALPS II) is an experiment currently being built at DESY in Hamburg, Germany, that will use a light-shining-through-a-wall (LSW) approach to search for axion-like particles. ALPS II represents a significant…

We develop a high-precision model for relativistic observables of the Atomic Clock Ensemble in Space (ACES) experiment on the International Space Station (ISS). We develop all relativistic coordinate transformations that are needed to…

General Relativity and Quantum Cosmology · Physics 2016-02-25 Slava G. Turyshev , Nan Yu , Viktor T. Toth

The new Inner Tracking System (ITS2) of the ALICE experiment began operation in 2021 with the start of LHC Run 3. Compared to its predecessor, ITS2 offers substantial improvements in pointing resolution, tracking efficiency at low…

Instrumentation and Detectors · Physics 2026-04-15 D. Agguiaro , G. Aglieri Rinella , L. Aglietta , M. Agnello , F. Agnese , B. Alessandro , G. Alfarone , J. Alme , E. Anderssen , D. Andreou , M. Angeletti , N. Apadula , P. Atkinson , C. Azzan , R. Baccomi , A. Badalà , A. Balbino , P. Barberis , F. Barile , L. Barioglio , R. Barthel , F. Baruffaldi , N. K. Behera , I. Belikov , A. Benato , M. Benettoni , F. Benotto , S. Beole , N. Bez , A. Bhatti , M. Bhopal , A. P. Bigot , G. Boca , G. Bonomi , M. Bonora , F. Borotto Dalla Vecchia , M. Borri , V. Borshchov , E. Botta , L. Boynton , G. Brower , E. Bruna , O. Brunasso Cattarello , G. E. Bruno , M. D. Buckland , S. Bufalino , P. Camerini , P. Cariola , C. Ceballos Sanchez , J. Cho , S. Cho , K. Choi , Y. Choi , N. J. Clague , O. A. Clausse , F. Colamaria , D. Colella , S. Coli , A. Collu , M. Concas , G. Contin , Y. Corrales Morales , S. Costanza , J. B. Dainton , E. Danè , W. Degraw , C. De Martin , W. Deng , G. De Robertis , P. Dhankher , A. Di Mauro , F. Dumitrache , D. Elia , M. R. Ersdal , J. Eum , A. Fantoni , G. Feofilov , J. Ferencei , F. Fichera , G. Fiorenza , A. N. Flores , A. Franco , M. Franco , J. P. Fransen , D. Gajanana , A. Galdames Perez , C. Gao , C. Gargiulo , L. Garizzo , P. Giubilato , M. Goffe , A. Grant , E. Grecka , L. Greiner , A. Grelli , A. Grimaldi , O. S. Groettvik , F. Grosa , C. Guo Hu , R. P. Hannigan , H. Helstrup , A. Hill , H. Hillemanns , P. Hindley , G. Huang , M. Iannone , J. P. Iddon , P. Ijzermans , M. A. Imhoff , A. Isakov , J. Jeong , T. Johnson , A. Junique , J. Kaewjai , M. Keil , Z. Khabanova , H. Khan , H. Kim , J. Kim , J. Kim , J. Kim , M. Kim , T. Kim , J. Klein , C. Kobdaj , A. Kotliarov , M. J. Kraan , I. Králik , F. Krizek , T. Kugathasan , C. Kuhn , P. G. Kuijer , S. Kushpil , M. J. Kweon , M. Kwon , Y. Kwon , P. La Rocca , N. Lacalamita , P. Larionov , G. Ledey , S. Lee , T. Lee , R. C. Lemmon , Y. Lesenechal , E. D. Lesser , B. E. Liang-Gilman , F. Librizzi , B. Lim , S. Lim , S. Lindsay , J. Liu , J. Liu , F. Loddo , M. Lupi , M. Mager , A. Maire , G. Mandaglio , V. Manzari , C. Markert , G. Markey , D. Marras , P. Martinengo , S. Martiradonna , M. Masera , A. Mastroserio , G. Mazza , D. Mazzaro , F. Mazzaschi , M. Mazzilli , L. Mcalpine , M. Mongelli , J. Morant , F. Morel , P. Morrall , V. Muccifora , A. Mulliri , L. Musa , A. I. Nambrath , M. Obergger , A. Orlandi , A. Palasciano , R. Panero , E. Paoletti , G. S. Pappalardo , O. Parasole , J. Park , L. Passamonti , C. Pastore , R. N. Patra , F. Pellegrino , A. Pepato , C. Petta , S. Piano , D. Pierluigi , S. Pisano , M. Pĺoskoń , M. T. Poblocki , S. Politano , E. Prakasa , F. Prino , M. Protsenko , M. Puccio , C. Puggioni , A. Rachevski , L. Ramello , M. Rasa , I. Ravasenga , A. U. Rehman , F. Reidt , M. Richter , F. Riggi , M. Rizzi , K. Røed , D. Röhrich , F. Ronchetti , M. J. Rossewij , A. Rossi , A. Russo , B. Di Ruzza , G. Saccà , M. Sacchetti , R. Sadikin , A. Sanchez Gonzalez , U. Savino , J. Schambach , F. Schlepper , R. Schotter , P. J. Secouet , M. Selina , S. Senyukov , J. J. Seo , R. Shahoyan , S. Shaukat , F. Shirokopetlev , K. Sielewicz , G. Simantovic , M. Sitta , R. J. M. Snellings , W. Snoeys , J. Song , J. M. Sonneveld , R. Spijkers , A. Sturniolo , C. P. Stylianidis , M. Šuljić , D. Sun , X. Sun , R. A. Syed , A. Szczepankiewicz , C. Terrevoli , M. Toppi , A. Trifiró , A. S. Triolo , S. Trogolo , V. Trubnikov , M. Turcato , R. Turrisi , T. Tveter , I. Tymchuk , G. L. Usai , V. Valentino , N. Valle , J. B. Van Beelen , J. W. Van Hoorne , T. Vanat , M. Varga-Kofarago , A. Velure , G. Venier , F. Veronese , A. Villani , A. Viticchié , C. Wabnitz , Y. Wang , P. Yang , E. R. Yeats , I. -K. Yoo , J. H. Yoon , S. Yuan , V. Zaccolo , A. Zampieri , C. Zampolli , E. Zhang , L. Zhang , X. Zhang , Z. Zhang , V. Zherebchevskii , N. Zurlo

Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, $\bar{p}$, $e^{\pm}$, and nuclei (H--O, Ne, Mg, Si, Fe), which resulted in a number of…

The Isochronous Mass Spectrometry (IMS) is a powerful technique developed in heavy-ion storage rings for measuring masses of very short-lived exotic nuclei. The IMS is based on the isochronous setting of the ring. One of the main parameters…