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Electromagnetically induced transparency (EIT) is predicted for x rays in laser-dressed neon gas. The x-ray photoabsorption cross section and polarizability near the Ne K edge are calculated using an ab initio theory suitable for optical…

Atomic Physics · Physics 2008-11-26 Christian Buth , Robin Santra , Linda Young

Small-angle neutron scattering (SANS) is a powerful technique for probing the nanoscale structure of materials. However, the fundamental limitations of neutron flux pose significant challenges for rapid, high-fidelity data acquisition…

Entangled photon sources (EPSs) are pivotal in advancing quantum communication, computing and sensing. The demand for deploying efficient, robust EPSs in the field, characterized by exceptional (phase) stability, has become increasingly…

Quantum Physics · Physics 2024-07-12 Giacomo Paganini , Alvaro Cuevas , Robin Camphausen , Alexander Demuth , Valerio Pruneri

The design of a neutron source capable of producing 24 and 70 keV neutron beams with narrow energy spread is presented. The source exploits near-threshold kinematics of the $^{7}$Li(p,n)$^{7}$Be reaction while taking advantage of the…

Instrumentation and Detectors · Physics 2014-05-22 T. H. Joshi , S. Sangiorgio , V. Mozin , E. B. Norman , P. Sorensen , M. Foxe , G. Bench , A. Bernstein

An efficient silicon based light source presents an unreached goal in the field of photonics, due to Silicons indirect electronic band structure preventing direct carrier recombination and subsequent photon emission. Here we utilize…

Applied Physics · Physics 2017-11-06 Hasan Göktaş Fikri Serdar Gökhan , Volker J. Sorger

In previous work a different and powerful, analytical, technique was used to get data, such as the absolute atom concentration (AAC), specimen thickness etc., from public domain boron nitride EELS spectrum collected under a collection…

Materials Science · Physics 2020-09-24 Noureddine Hadji

Deep-UV ~ 250 nm (4.96 eV) tilted in-situ co-illumination of the sample under imaging by scanning electron microscope (SEM) is developed at a robust and practical instrument level. Precise mechanical control of the lateral position and tilt…

There is currently a big effort put into the operation and construction of world class neutron scattering facilities (SNS and SNS-TS2 in the US, J-PARC in Japan, ESS in Europe, CSS in China, PIK in Russia). On the other hand, there exists a…

The extragalactic background light (EBL) in the IR to UV bands partly absorbs very high energy (VHE, $E \geq$ 100GeV) $\gamma-$ray photons travelling over cosmological distances via pair production. In this paper, to get stronger…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Longhua Qin , Jiancheng Wang , Quangui Gao , Weiwei Na , Huaizhen Li , Ao Wang , Chuyuan Yang , Jianping Yang

The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a…

Accelerator Physics · Physics 2013-05-20 T. R. Edgecock , O. Caretta , T. Davenne , C. Densham , M. Fitton , D. Kelliher , P. Loveridge , S. Machida , C. Prior , C. Rogers , M. Rooney , J. Thomason , D. Wilcox , E. Wildner , I. Efthymiopoulos , R. Garoby , S. Gilardoni , C. Hansen , E. Benedetto , E. Jensen , A. Kosmicki , M. Martini , J. Osborne , G. Prior , T. Stora , T. Melo-Mendonca , V. Vlachoudis , C. Waaijer , P. Cupial , A. Chancé , A. Longhin , J. Payet , M. Zito , E. Baussan , C. Bobeth , E. Bouquerel , M. Dracos , G. Gaudiot , B. Lepers , F. Osswald , P. Poussot , N. Vassilopoulos , J. Wurtz , V. Zeter , J. Bielski , M. Kozien , L. Lacny , B. Skoczen , B. Szybinski , A. Ustrycka , A. Wroblewski , M. Marie-Jeanne , P. Balint , C. Fourel , J. Giraud , J. Jacob , T. Lamy , L. Latrasse , P. Sortais , T. Thuillier , S. Mitrofanov , M. Loiselet , Th. Keutgen , Th. Delbar , F. Debray , C. Trophine , S. Veys , C. Daversin , V. Zorin , I. Izotov , V. Skalyga , G. Burt , A. C. Dexter , V. L. Kravchuk , T. Marchi , M. Cinausero , F. Gramegna , G. De Angelis , G. Prete , G. Collazuol , M. Laveder , M. Mazzocco , M. Mezzetto , C. Signorini , E. Vardaci , A. Di Nitto , A. Brondi , G. La Rana , P. Migliozzi , R. Moro , V. Palladino , N. Gelli , D. Berkovits , M. Hass , T. Y. Hirsh , M. Schaumann , A. Stahl , J. Wehner , A. Bross , J. Kopp , D. Neuffer , R. Wands , R. Bayes , A. Laing , P. Soler , S. K. Agarwalla , A. Cervera Villanueva , A. Donini , T. Ghosh , J. J. Gómez Cadenas , P. Hernández , J. Martín-Albo , O. Mena , J. Burguet-Castell , L. Agostino , M. Buizza-Avanzini , M. Marafini , T. Patzak , A. Tonazzo , D. Duchesneau , L. Mosca , M. Bogomilov , Y. Karadzhov , R. Matev , R. Tsenov , E. Akhmedov , M. Blennow , M. Lindner , T. Schwetz , E. Fernández Martinez , M. Maltoni , J. Menéndez , C. Giunti , M. C. González García , J. Salvado , P. Coloma , P. Huber , T. Li , J. López-Pavón , C. Orme , S. Pascoli , D. Meloni , J. Tang , W. Winter , T. Ohlsson , H. Zhang , L. Scotto-Lavina , F. Terranova , M. Bonesini , L. Tortora , A. Alekou , M. Aslaninejad , C. Bontoiu , A. Kurup , L. J. Jenner , K. Long , J. Pasternak , J. Pozimski , J. J. Back , P. Harrison , K. Beard , A. Bogacz , J. S. Berg , D. Stratakis , H. Witte , P. Snopok , N. Bliss , M. Cordwell , A. Moss , S. Pattalwar , M. Apollonio

A laser ablation ion source (LAS) is a powerful tool by which diverse species of ions can be produced for mass spectrometer calibration, or surface study applications. It is necessary to frequently shift the laser position on the target to…

A structure, used as a complex source of X-rays and neutron source, is designed with the assistance of CST module tool. Particles of -H and electron, attracted from a plasma source, are designed to be separated by an energy selector. Soon…

Accelerator Physics · Physics 2020-02-13 X. B. Yang , X. B. Qin , P. H. Liu , T. Li , K. Zhuang

The Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was…

Instrumentation and Methods for Astrophysics · Physics 2025-04-30 J. -C. Cuillandre , E. Bertin , M. Bolzonella , H. Bouy , S. Gwyn , S. Isani , M. Kluge , O. Lai , A. Lançon , D. A. Lang , R. Laureijs , T. Saifollahi , M. Schirmer , C. Stone , Abdurro'uf , N. Aghanim , B. Altieri , F. Annibali , H. Atek , P. Awad , M. Baes , E. Bañados , D. Barrado , S. Belladitta , V. Belokurov , A. Boselli , F. Bournaud , J. Bovy , R. A. A. Bowler , G. Buenadicha , F. Buitrago , M. Cantiello , D. Carollo , S. Codis , M. L. M. Collins , G. Congedo , E. Dalessandro , V. de Lapparent , F. De Paolis , J. M. Diego , P. Dimauro , J. Dinis , H. Dole , P. -A. Duc , D. Erkal , M. Ezziati , A. M. N. Ferguson , A. Ferré-Mateu , A. Franco , R. Gavazzi , K. George , W. Gillard , J. B. Golden-Marx , B. Goldman , A. H. Gonzalez , R. Habas , W. G. Hartley , N. A. Hatch , R. Kohley , J. Hoar , J. M. Howell , L. K. Hunt , P. Jablonka , M. Jauzac , Y. Kang , J. H. Knapen , J. -P. Kneib , R. Kohley , P. B. Kuzma , S. S. Larsen , O. Marchal , J. Martín-Fleitas , P. Marcos-Arenal , F. R. Marleau , E. L. Martín , D. Massari , A. W. McConnachie , M. Meneghetti , M. Miluzio , J. Miro Carretero , H. Miyatake , M. Mondelin , M. Montes , A. Mora , O. Müller , C. Nally , K. Noeske , A. A. Nucita , P. A. Oesch , M. Oguri , R. F. Peletier , M. Poulain , L. Quilley , G. D. Racca , M. Rejkuba , J. Rhodes , P. -F. Rocci , J. Román , S. Sacquegna , E. Saremi , R. Scaramella , E. Schinnerer , S. Serjeant , E. Sola , J. G. Sorce , F. Tarsitano , I. Tereno , S. Toft , C. Tortora , M. Urbano , A. Venhola , K. Voggel , J. R. Weaver , X. Xu , M. Žerjal , R. Zöller , S. Andreon , N. Auricchio , M. Baldi , A. Balestra , S. Bardelli , A. Basset , R. Bender , C. Bodendorf , E. Branchini , S. Brau-Nogue , M. Brescia , J. Brinchmann , S. Camera , V. Capobianco , C. Carbone , J. Carretero , S. Casas , F. J. Castander , M. Castellano , S. Cavuoti , A. Cimatti , C. J. Conselice , L. Conversi , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , J. -G. Cuby , A. Da Silva , H. Degaudenzi , A. M. Di Giorgio , M. Douspis , C. A. J. Duncan , X. Dupac , S. Dusini , M. Fabricius , M. Farina , S. Farrens , S. Ferriol , S. Fotopoulou , M. Frailis , E. Franceschi , S. Galeotta , B. Garilli , B. Gillis , C. Giocoli , P. Gómez-Alvarez , A. Grazian , F. Grupp , L. Guzzo , S. V. H. Haugan , J. Hoar , H. Hoekstra , W. Holmes , I. Hook , F. Hormuth , A. Hornstrup , P. Hudelot , K. Jahnke , M. Jhabvala , E. Keihänen , S. Kermiche , A. Kiessling , M. Kilbinger , T. Kitching , B. Kubik , K. Kuijken , M. Kümmel , M. Kunz , H. Kurki-Suonio , O. Lahav , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , D. Maino , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , N. Martinet , F. Marulli , R. Massey , S. Maurogordato , H. J. McCracken , E. Medinaceli , Y. Mellier , G. Meylan , J. J. Mohr , M. Moresco , L. Moscardini , E. Munari , R. Nakajima , R. C. Nichol , S. -M. Niemi , C. Padilla , S. Paltani , F. Pasian , J. A. Peacock , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , R. Rebolo , A. Refregier , A. Renzi , G. Riccio , Hans-Walter Rix , E. Romelli , M. Roncarelli , E. Rossetti , R. Saglia , D. Sapone , P. Schneider , T. Schrabback , A. Secroun , G. Seidel , S. Serrano , C. Sirignano , G. Sirri , J. Skottfelt , L. Stanco , P. Tallada-Crespí , A. N. Taylor , H. I. Teplitz , R. Toledo-Moreo , A. Tsyganov , I. Tutusaus , E. A. Valentijn , L. Valenziano , T. Vassallo , G. Verdoes Kleijn , Y. Wang , J. Weller , O. R. Williams , G. Zamorani , E. Zucca , C. Baccigalupi , C. Burigana , P. Casenove , P. Liebing , V. Scottez , P. Simon , D. Scott

Spallation neutron production in proton induced reactions on Al, Fe, Zr, W, Pb and Th targets at 1.2 GeV and on Fe and Pb at 0.8, and 1.6 GeV measured at the SATURNE accelerator in Saclay is reported. The experimental double-differential…

We consider radio bursts that originate from extragalactic neutron stars (NSs) by addressing three questions about source distances. What are the physical limitations on coherent radiation at GHz frequencies? Do they permit detection at…

High Energy Astrophysical Phenomena · Physics 2016-01-21 J. M. Cordes , Ira Wasserman

The SKA PAthfinder Radio Continuum Surveys (SPARCS) are providing deep-field imaging of the faint (sub-mJy) extra-galactic radio source populations through a series of reference surveys. One of the key science goals for SPARCS is to…

We describe design studies for a pulsed quasi-monoenergetic 2-keV neutron source for calibration of sub-keV nuclear recoils. Such a calibration is required for detectors sensitive to sub-GeV dark matter and also the coherent elastic…

Observations of TeV--PeV-energy cosmic neutrinos by the IceCube observatory have suggested that extragalactic cosmic-ray sources should have an optical depth greater than $\sim$0.01 and contribute to more than 10\% of the observed bulk of…

High Energy Astrophysical Phenomena · Physics 2016-12-16 Shigeru Yoshida

A new picture of pulsar high-energy emission is proposed that is different from both the traditional polar cap and outer gap models, but combines elements of each. The slot gap model is based on electron acceleration along the edge of the…

Astrophysics · Physics 2009-11-10 Alice Harding , Alexander Muslimov
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