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We perform kinetic simulations of diffusive shock acceleration (DSA) in Type Ia supernova remnants (SNRs) expanding into a uniform interstellar medium (ISM). Bohm-like diffusion assumed, and simple models for Alfvenic drift and dissipation…

High Energy Astrophysical Phenomena · Physics 2017-01-18 Hyesung Kang

We describe a Phased Array Feed (PAF) system, called Apertif, which will be installed in the Westerbork Synthesis Radio Telescope (WSRT). The aim of Apertif is, at frequencies from 1.0 to 1.7 GHz, to increase the instantaneous field of view…

Instrumentation and Methods for Astrophysics · Physics 2019-08-12 Tom Oosterloo , Marc Verheijen , Wim van Cappellen

The existing models of the interstellar radiation field (ISRF) do not produce a Maxwell field. Here, the recent model of the ISRF as a Maxwell field is improved by considering separately the different frequencies at the stage of the…

General Physics · Physics 2023-08-29 Mayeul Arminjon

A precise measurement of the cosmic-ray proton spectrum with the Calorimetric Electron Telescope (CALET) is presented in the energy interval from 50 GeV to 60 TeV, and the observation of a softening of the spectrum above 10 TeV is reported.…

The HypHI collaboration aims to perform a precise hypernuclear spectroscopy with stable heavy ion beams and rare isotope beams at GSI and fAIR in order to study hypernuclei at extreme isospin, especially neutron rich hypernuclei to look…

The Askaryan Radio Array (ARA) experiment aims to detect ultra-high-energy cosmic neutrinos (>10 PeV) using radio detection techniques. To enhance ARA's capabilities, a new RFSoC-based DAQ, ARA-Next, is in the early stages of development.…

High Energy Astrophysical Phenomena · Physics 2024-09-13 Pawan Giri , Ilya Kravchenko , Patrick Allison , Amy L. Connolly

This article presents a review about the main CERN n\_TOF contributions to the field of neutron-capture experiments of interest for $s$-process nucleosynthesis studies over the last 25 years, with special focus on the measurement of…

Nuclear Experiment · Physics 2025-02-17 C. Domingo-Pardo , O. Aberle , V. Alcayne , G. Alpar , M. Al Halabi , S. Amaducci , V. Babiano , M. Bacak , J. Balibrea-Correa , J. Bartolomé , A. P. Bernardes , B. Bernardino Gameiro , E. Berthoumieux , R. Beyer , M. Birch , M. Boromiza , D. Bosnar , B. Brusasco , M. Caamaño , A. Cahuzac , F. Calviño , M. Calviani , D. Cano-Ott , A. Casanovas , D. M. Castelluccio , D. Catlett , F. Cerutti , G. Cescutti , E. Chiaveri , G. Claps , P. Colombetti , N. Colonna , P. Console Camprini , G. Cortés , M. A. Cortés-Giraldo , L. Cosentino , S. Cristallo , A. D'Ottavi , G. de la Fuente Rosales , S. F. Dellmann , M. Diakaki , M. Di Castro , A. Di Chicco , M. Dietz , E. Dupont , I. Durán , Z. Eleme , M. Eslami , S. Fargier , B. Fernández-Domínguez , P. Finocchiaro , W. Flanagan , V. Furman , A. Gandhi , F. García-Infantes , A. Gawlik-Ramiega , G. Gervino , S. Gilardoni , E. González-Romero , S. Goula , E. Griesmayer , C. Guerrero , F. Gunsing , C. Gustavino , J. Heyse , W. Hillman , D. G. Jenkins , E. Jericha , A. Junghans , Y. Kadi , K. Kaperoni , I. Kelly , M. Kokkoris , Y. Kopatch , M. Krtička , N. Kyritsis , C. Lederer-Woods , J. Lerendegui-Marco , A. Manna , T. Martínez , M. Martínez-Cañada , A. Masi , C. Massimi , P. Mastinu , M. Mastromarco , E. A. Maugeri , A. Mazzone , E. Mendoza , A. Mengoni , V. Michalopoulou , P. M. Milazzo , J. Moldenhauer , R. Mucciola , E. Musacchio González , A. Musumarra , A. Negret , E. Odusina , D. Papanikolaou , N. Patronis , J. A. Pavón-Rodríguez , M. G. Pellegriti , P. Pérez-Maroto , A. Pérez de Rada Fiol , G. Perfetto , J. Perkowski , C. Petrone , N. Pieretti , L. Piersanti , E. Pirovano , I. Porras , J. Praena , J. M. Quesada , R. Reifarth , D. Rochman , Y. Romanets , A. Rooney , G. Rovira , C. Rubbia , A. Sánchez-Caballero , R. N. Sahoo , D. Scarpa , P. Schillebeeckx , A. G. Smith , N. V. Sosnin , M. Spelta , M. E. Stamati , K. Stasiak , G. Tagliente , A. Tarifeño-Saldivia , D. Tarrío , P. Torres-Sánchez , S. Tosi , G. Tsiledakis , S. Valenta , P. Vaz , G. Vecchio , D. Vescovi , V. Vlachoudis , R. Vlastou , A. Wallner , C. Weiss , P. J. Woods , T. Wright , R. Wu , P. Žugec , The n\_TOF Collaboration

The FAIR[1] facility is an international accelerator centre for research with ion and antiproton beams. It is being built at Darmstadt, Germany as an extension to the current GSI research institute. One major part of the facility will be…

A Free Electron Laser (FEL) facility utilizing a recirculated Superconducting Radio Frequency (SRF) linear accelerator (linac) provides the opportunity to achieve about five times greater photon energy than an unrecirculated linac of…

Accelerator Physics · Physics 2015-06-17 R. C. York

While SNRs have been considered the most relevant Galactic CR accelerators for decades, CCSNe could accelerate particles during the earliest stages of their evolution and hence contribute to the CR energy budget in the Galaxy. Some SNRs…

High Energy Astrophysical Phenomena · Physics 2024-04-17 G. Martí-Devesa , C. C. Cheung , N. Di Lalla , M. Renaud , G. Principe , N. Omodei , F. Acero

An outline is explained for hadron-physics projects at J-PARC, which is considered to be one of the flagship facilities in hadron physics from 2008. The facility provides an intensity frontier with 50 GeV proton beam for nuclear and…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Kumano

Contemporary ultraintense, short-pulse laser systems provide extremely compact setups for the production of high-flux neutron beams, such as those required for nondestructive probing of dense matter, research on neutron-induced damage in…

This paper reports on the conclusions of a 2013 Joint DOE/NCI Workshop, and translates clinical accelerator facility requirements into accelerator and beam-delivery technical specifications. Available or feasible accelerator technologies…

Accelerator Physics · Physics 2017-04-17 C. Johnstone , J. Taylor , R. Edgecock , R. Schulte

We report the experimental results of the commissioning phase in the 10 PW laser beamline of Shanghai Superintense Ultrafast Laser Facility (SULF). The peak power reaches 2.4 PW on target without the last amplifying during the experiment.…

The global availability of high-intensity neutron sources is restricted by the prohibitive costs of spallation facilities and the decommissioning of aging research reactors, while compact accelerator-driven sources (CANS) are fundamentally…

Accelerator Physics · Physics 2026-02-11 Antonio Cammi , Lorenzo Loi , Andrea Missaglia , David Alesini , Hans Heinrich Braun

There is demand for the construction of a medium-energy ion linear accelerator based on superconducting rf (SRF) technology. It must be capable of producing several hundred kilowatts of CW beams ranging from protons to uranium. A…

Accelerator Physics · Physics 2011-07-18 P. N. Ostroumov , J. A. Nolen , K. W. Shepard

The Medley setup is planned to be moved to and used at the new neutron facility NFS where measurements of light-ion production and fission cross-sections are planned at 1-40 MeV. Medley has eight detector telescopes providing Delta E-Delta…

Instrumentation and Detectors · Physics 2014-09-09 K. Jansson , C. Gustavsson , S. Pomp , A. V. Prokofiev , G. Scian , D. Tarrío , U. Tippawan

An upgrade of the Jefferson Lab IR FEL is now under construction. It will provide 10 kW output light power in a wavelength range of 2-10 microns. The FEL will be driven by a modest-sized 80-210 MeV, 10 mA energy-recovering superconducting…

Accelerator Physics · Physics 2014-11-18 D. Douglas , S. V. Benson , G. A. Krafft , R. Li , L. Merminga , B. C. Yunn

The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) is dedicated to the fine spectroscopy (Delta-E: 2 keV FWHM @ 1.3 MeV) and fine imaging (angular resolution: 12 arcmin FWHM) of celestial gamma-ray sources in the energy range 15…

Astrophysics · Physics 2007-05-23 C. Winkler

The development of a new RFQ Cooler, named SHIRaC, was carried out to handle and cool typical SPIRAL 2 beams of large emittances (up to 80 {\pi}.mm.mrad) and high currents (up to 1 {\micro}A). SHIRaC is a part of SPIRAL 2 facility at GANIL…

Accelerator Physics · Physics 2015-07-23 Ramzi Boussaid