English
Related papers

Related papers: Emittance growth in linear induction accelerators

200 papers

The so-called aromatic infrared bands are attributed to emission of polycyclic aromatic hydrocarbons. The observed variations toward different regions in space are believed to be caused by contributions of different classes of PAH…

Astrophysics of Galaxies · Physics 2021-04-14 Shreyak Banhatti , Julianna Palotás , Pavol Jusko , Britta Redlich , Jos Oomens , Stephan Schlemmer , Sandra Brünken

The radiative instability of the relativistic electron beam in a periodic dielectric-filled cylindrical waveguide is considered. The dependence of the beam instability increment on the radiated wave frequency near the region of dispersion…

Accelerator Physics · Physics 2011-05-17 V. G. Baryshevsky , E. A. Gurnevich

In order to study the acceleration and propagation of bremsstrahlung-producing electrons in solar flares, we analyze the evolution of the flare loop size with respect to energy at a variety of times. A GOES M3.7 loop-structured flare…

Solar and Stellar Astrophysics · Physics 2015-06-05 Jingnan Guo , A. Gordon Emslie , Eduard P. Kontar , Federico Benvenuto , Anna Maria Massone , Michele Piana

This paper analyzes astrophysical scenarios that may be detected at the upper end of the energy range of the Gamma Ray Large Area Space Telescope (GLAST), as a result of cosmic-ray (CR) diffusion in the interstellar medium (ISM). Hadronic…

Proportional electroluminescence (EL) in noble gases is used in two-phase detectors for dark matter searches to record (in the gas phase) the ionization signal induced by particle scattering in the liquid phase. The "standard" EL mechanism…

Instrumentation and Detectors · Physics 2021-03-01 The DarkSide collaboration , C. E. Aalseth , S. Abdelhakim , P. Agnes , R. Ajaj , I. F. M. Albuquerque , T. Alexander , A. Alici , A. K. Alton , P. Amaudruz , F. Ameli , J. Anstey , P. Antonioli , M. Arba , S. Arcelli , R. Ardito , I. J. Arnquist , P. Arpaia , D. M. Asner , A. Asunskis , M. Ave , H. O. Back , V. Barbaryan , A. Barrado Olmedo , G. Batignani , M. G. Bisogni , V. Bocci , A. Bondar , G. Bonfini , W. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , R. Bunker , S. Bussino , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Candela , C. Cantini , M. Caravati , M. Cariello , F. Carnesecchi , A. Castellani , P. Castello , P. Cavalcante , D. Cavazza , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , B. Celano , R. Cereseto , S. Chashin , W. Cheng , A. Chepurnov , C. Cicalò , L. Cifarelli , M. Citterio , F. Coccetti , V. Cocco , M. Colocci , E. Conde Vilda , L. Consiglio , F. Cossio , G. Covone , P. Crivelli , I. D'Antone , M. D'Incecco , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , S. De Cecco , M. De Deo , A. De Falco , D. De Gruttola , G. De Guido , G. De Rosa , G. Dellacasa , P. Demontis , S. De Pasquale , A. V. Derbin , A. Devoto , F. Di Eusanio , L. Di Noto , G. Di Pietro , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , M. Downing , F. Edalatfar , A. Empl , M. Fernandez Diaz , C. Filip , G. Fiorillo , K. Fomenko , A. Franceschi , D. Franco , E. Frolov , G. E. Froudakis , N. Funicello , F. Gabriele , A. Gabrieli , C. Galbiati , M. Garbini , P. Garcia Abia , D. Gascón Fora , A. Gendotti , C. Ghiano , A. Ghisi , P. Giampa , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , M. L. Gligan , O. Gorchakov , M. Grab , R. Graciani Diaz , M. Grassi , J. W. Grate , A. Grobov , M. Gromov , M. Guan , M. B. B. Guerra , M. Guerzoni , M. Gulino , R. K. Haaland , B. R. Hackett , A. Hallin , M. Haranczyk , B. Harrop , E. W. Hoppe , S. Horikawa , B. Hosseini , F. Hubaut , P. Humble , E. V. Hungerford , An. Ianni , A. Ilyasov , V. Ippolito , C. Jillings , K. Keeter , C. L. Kendziora , I. Kochanek , K. Kondo , G. Kopp , D. Korablev , G. Korga , A. Kubankin , R. Kugathasan , M. Kuss , M. La Commara , L. La Delfa , M. Lai , M. Lebois , B. Lehnert , N. Levashko , X. Li , Q. Liqiang , M. Lissia , G. U. Lodi , G. Longo , R. Lussana , L. Luzzi , A. A. Machado , I. N. Machulin , A. Mandarano , S. Manecki , L. Mapelli , A. Margotti , S. M. Mari , M. Mariani , J. Maricic , M. Marinelli , D. Marras , M. Martínez , A. D. Martinez Rojas , M. Mascia , J. Mason , A. Masoni , A. B. McDonald , A. Messina , T. Miletic , R. Milincic , A. Moggi , S. Moioli , J. Monroe , M. Morrocchi , T. Mroz , W. Mu , V. N. Muratova , S. Murphy , C. Muscas , P. Musico , R. Nania , T. Napolitano , A. Navrer Agasson , M. Nessi , I. Nikulin , V. Nosov , J. A. Nowak , A. Oleinik , V. Oleynikov , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , S. Palmas , L. Pandola , E. Pantic , E. Paoloni , F. Pazzona , S. Peeters , P. A. Pegoraro , K. Pelczar , L. A. Pellegrini , C. Pellegrino , N. Pelliccia , F. Perotti , V. Pesudo , E. Picciau , F. Pietropaolo , A. Pocar , T. R. Pollmann , D. Portaluppi , S. S. Poudel , P. Pralavorio , D. Price , B. Radics , F. Raffaelli , F. Ragusa , M. Razeti , C. Regenfus , A. L. Renshaw , S. Rescia , M. Rescigno , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , J. Rode , A. Romani , L. Romero , N. Rossi , A. Rubbia , P. Sala , P. Salatino , O. Samoylov , E. Sánchez García , E. Sandford , S. Sanfilippo , M. Sant , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , B. Schlitzer , G. Scioli , E. Segreto , A. Seifert , D. A. Semenov , A. Shchagin , A. Sheshukov , S. Siddhanta , M. Simeone , P. N. Singh , P. Skensved , M. D. Skorokhvatov , O. Smirnov , G. Sobrero , A. Sokolov , A. Sotnikov , R. Stainforth , A. Steri , S. Stracka , V. Strickland , G. B. Suffritti , S. Sulis , Y. Suvorov , A. M. Szelc , R. Tartaglia , G. Testera , T. Thorpe , A. Tonazzo , A. Tosi , M. Tuveri , E. V. Unzhakov , G. Usai , A. Vacca , E. Vázquez-Jáuregui , T. Viant , S. Viel , F. Villa , A. Vishneva , R. B. Vogelaar , J. Wahl , J. J. Walding , H. Wang , Y. Wang , S. Westerdale , R. J. Wheadon , R. Williams , J. Wilson , Ma. M. Wojcik , Ma. Wojcik , S. Wu , X. Xiao , C. Yang , Z. Ye , M. Zuffa , G. Zuzel

In this work we analyze the longitudinal instabilities of propagating acceleration structures that are driven by a relativistically intense laser at the moving plasma critical layer [1]. These instabilities affect the energy-spectra of the…

Plasma Physics · Physics 2014-11-11 Aakash Ajit Sahai , Thomas C. Katsouleas

For the assessment of radiation effects of clinical ion-beams, dosimetry has to be complemented by information on particle-energy distribution or related quantities. Fluorescence nuclear track detectors made from C,Mg-doped alumina single…

Medical Physics · Physics 2017-09-22 Steffen Greilich , Leonie Ulrich , Jasper J. M. Kouwenberg , Shirin Rahmanian

Advanced linear accelerator design may use Optical Transition Radiation (OTR) screens to measure beam spot size; for instance, such screens are foreseen in plasma based accelerators (EuPRAXIA@SPARC_LAB) or Compton machines (Gamma Beam…

Plasma outflows from gamma-ray bursts (GRB), pulsar winds, relativistic jets, and ultra-intense laser targets radiate high energy photons. However, radiation damping is ignored in conventional PIC simulations. In this letter, we study the…

Astrophysics · Physics 2007-05-23 Koichi Noguchi , Edison Liang , Kazumi Nishimura

The scaled momentum distributions of charged particles in jets have been measured for dijet photoproduction with the ZEUS detector at HERA using an integrated luminosity of 359 pb-1. The distributions are compared to predictions based on…

High Energy Physics - Experiment · Physics 2012-08-27 ZEUS Collaboration

In a Low Energy Beam Transport line (LEBT), the emittance growth due to the beam's own space charge is typically suppressed by way of neutralization from either electrons or ions, which originate from ionization of the background gas. In…

Accelerator Physics · Physics 2017-04-20 L. Prost , J. -P. Carneiro , A. Shemyakin

The acceleration and radiative processes active in low-power radio hotspots are investigated by means of new deep near-infrared (NIR) and optical VLT observations, complemented with archival, high-sensitivity VLT, radio VLA and X-ray…

High Energy Astrophysical Phenomena · Physics 2020-05-20 G. Migliori , M. Orienti , L. Coccato , G. Brunetti , F. D'Ammando , K. -H. Mack , M. A. Prieto

This work reports a peculiar and interesting train of microwave type III pair bursts in the impulsive rising phase of a solar flare on 2011 September 26. The observations include radio spectrometers at frequency of 0.80 - 2.00 GHz, hard…

Solar and Stellar Astrophysics · Physics 2016-09-28 Baolin Tan , Marian Karlicky , Hana Meszarosova , Larisa Kashapova , Jing Huang , Yan Yan , Eduard P. Kontar

We study the release of energy during the gradual phase of a flare, characterized by faint bursts of non-thermal hard X-ray (HXR) emission associated with decimetric radio spikes and type III radio bursts starting at high frequencies and…

Solar and Stellar Astrophysics · Physics 2021-01-20 Sophie Musset , Eduard Kontar , Lindsay Glesener , Nicole Vilmer , Abdallah Hamini

In this paper we present new observational evidence that supports the presence of an extra source of continuum emission in the binary system beta Lyrae. New VLA and IRAM observations, together with published data from the literature and ISO…

Astrophysics · Physics 2009-11-07 G. Umana , F. Leone , C. Trigilio

The Ultra Luminous InfraRed Galaxy Mrk 231 reveals up to seven rotational lines of water (H2O) in emission, including a very high-lying (E_{upper}=640 K) line detected at a 4sigma level, within the Herschel/SPIRE wavelength range, whereas…

The ADS accelerator in China is a CW (Continuous-Wave) proton linac with 1.5 GeV in beam energy, 10 mA in beam current, and 15 MW in beam power. To meet the extremely low beam loss rate requirement and high reliability, it is very important…

Accelerator Physics · Physics 2015-09-30 Cai Meng , Jing-Yu Tang , Shi-Lun Pei , Yan Fang

Secondary electron (SE) imaging techniques, such as scanning electron microscopy and helium ion microscopy (HIM), use electrons emitted by a sample in response to a focused beam of charged particles incident at a grid of raster scan…

Signal Processing · Electrical Eng. & Systems 2026-03-12 Vaibhav Choudhary , Akshay Agarwal , Vivek K Goyal

The direct measurements of the cosmic electron-positron spectrum around 1 TeV made by DAMPE have induced many theoretical speculations about possible excesses in the data above the standard astrophysical predictions that might have the dark…

High Energy Astrophysical Phenomena · Physics 2019-07-01 Konstantin Belotsky , Airat Kamaletdinov , Maxim Laletin , Maxim Solovyov