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RHIC is the only spin-polarized proton collider ever built. With a special optics run of $\beta^\star \approx 22$ m STAR detector system is suitable for an investigation of the spin dependence of elastic proton-proton scattering. This is a…

High Energy Physics - Experiment · Physics 2015-01-07 Leszek Adamczyk

Intending to solve the decade old problem of solar opacity, we report substantial photoabsorption uncertainty due to the effect of ion-ion correlations. By performing detailed opacity calculations of the solar mixture, we find that taking…

Solar and Stellar Astrophysics · Physics 2018-03-01 Menahem Krief , Yair Kurzweil , Alexander Feigel , Doron Gazit

Directional detection of nuclear recoils is broadly desirable in nuclear and particle physics. At low recoil energies, this capability may be used to confirm the cosmological origin of a dark matter signal, to penetrate the so-called…

Instrumentation and Detectors · Physics 2021-10-13 Majd Ghrear , Sven E. Vahsen , Cosmin Deaconu

In the present paper, we aim to constrain the properties of the ionisation region in a star from the oscillation frequency variation (a so-called glitch) caused by rapid structural variations in this very region. In particular, we seek to…

Solar and Stellar Astrophysics · Physics 2022-07-13 Pierre S. Houdayer , Daniel R. Reese , Marie-Jo Goupil

The sustained increase of emissions of artificial light is causing a progressive brightening of the night sky in most of the world. This process represents a threat for the long-term sustainability of the scientific and educational activity…

Instrumentation and Methods for Astrophysics · Physics 2020-12-29 Fabio Falchi , Salvador Bará

Photonic Time Crystals (PTCs) - dielectric media with their refractive index modulated periodically in time, offer new opportunities in photonics arising from time reflections and momentum bandgaps. Here, we study the emission of light from…

Interpixel capacitance (IPC) between adjacent pixels in hybridized arrays gives rise to an electrostatic cross talk. This cross talk causes MTF degradation and blurring of images or spectra collected using these devices. As pixel size is…

Instrumentation and Methods for Astrophysics · Physics 2019-12-19 Kevan Donlon , Zoran Ninkov , Stefi Baum

We evaluate the effects of high-energy ionizing particles on the Si:As impurity band conduction (IBC) mid-infrared detector on board AKARI, the Japanese infrared astronomical satellite. IBC-type detectors are known to be little influenced…

Instrumentation and Methods for Astrophysics · Physics 2015-05-27 Akio Mouri , Hidehiro Kaneda , Daisuke Ishihara , Shinki Oyabu , Mituyoshi Yamagishi , Tatuya Mori , Takashi Onaka , Takehiko Wada , Hirokazu Kataza

We report on a polarization measurement of inclusive $J/\psi$ mesons in the di-electron decay channel at mid-rapidity at 2 $<p_{T}<$ 6 GeV/$c$ in $p+p$ collisions at $\sqrt{s}$ = 200 GeV. Data were taken with the STAR detector at RHIC. The…

Nuclear Experiment · Physics 2014-11-19 STAR Collaboration , L. Adamczyk , J. K. Adkins , G. Agakishiev , M. M. Aggarwal , Z. Ahammed , I. Alekseev , J. Alford , C. D. Anson , A. Aparin , D. Arkhipkin , E. C. Aschenauer , G. S. Averichev , J. Balewski , A. Banerjee , Z. Barnovska , D. R. Beavis , R. Bellwied , A. Bhasin , A. K. Bhati , P. Bhattarai , H. Bichsel , J. Bielcik , J. Bielcikova , L. C. Bland , I. G. Bordyuzhin , W. Borowski , J. Bouchet , A. V. Brandin , S. G. Brovko , S. Bültmann , I. Bunzarov , T. P. Burton , J. Butterworth , H. Caines , M. Calderón de la Barca Sánchez , D. Cebra , R. Cendejas , M. C. Cervantes , P. Chaloupka , Z. Chang , S. Chattopadhyay , H. F. Chen , J. H. Chen , L. Chen , J. Cheng , M. Cherney , A. Chikanian , W. Christie , J. Chwastowski , M. J. M. Codrington , R. Corliss , J. G. Cramer , H. J. Crawford , X. Cui , S. Das , A. Davila Leyva , L. C. De Silva , R. R. Debbe , T. G. Dedovich , J. Deng , A. A. Derevschikov , R. Derradi de Souza , S. Dhamija , B. di Ruzza , L. Didenko , C. Dilks , F. Ding , P. Djawotho , X. Dong , J. L. Drachenberg , J. E. Draper , C. M. Du , L. E. Dunkelberger , J. C. Dunlop , L. G. Efimov , J. Engelage , K. S. Engle , G. Eppley , L. Eun , O. Evdokimov , R. Fatemi , S. Fazio , J. Fedorisin , P. Filip , E. Finch , Y. Fisyak , C. E. Flores , C. A. Gagliardi , D. R. Gangadharan , D. Garand , F. Geurts , A. Gibson , M. Girard , S. Gliske , D. Grosnick , Y. Guo , A. Gupta , S. Gupta , W. Guryn , B. Haag , O. Hajkova , A. Hamed , L-X. Han , R. Haque , J. W. Harris , J. P. Hays-Wehle , S. Heppelmann , A. Hirsch , G. W. Hoffmann , D. J. Hofman , S. Horvat , B. Huang , H. Z. Huang , X. Huang , P. Huck , T. J. Humanic , G. Igo , W. W. Jacobs , H. Jang , E. G. Judd , S. Kabana , D. Kalinkin , K. Kang , K. Kauder , H. W. Ke , D. Keane , A. Kechechyan , A. Kesich , Z. H. Khan , D. P. Kikola , I. Kisel , A. Kisiel , D. D. Koetke , T. Kollegger , J. Konzer , I. Koralt , W. Korsch , L. Kotchenda , P. Kravtsov , K. Krueger , I. Kulakov , L. Kumar , R. A. Kycia , M. A. C. Lamont , J. M. Landgraf , K. D. Landry , J. Lauret , A. Lebedev , R. Lednicky , J. H. Lee , W. Leight , M. J. LeVine , C. Li , W. Li , X. Li , X. Li , Y. Li , Z. M. Li , L. M. Lima , M. A. Lisa , F. Liu , T. Ljubicic , W. J. Llope , R. S. Longacre , X. Luo , G. L. Ma , Y. G. Ma , D. M. M. D. Madagodagettige Don , D. P. Mahapatra , R. Majka , S. Margetis , C. Markert , H. Masui , H. S. Matis , D. McDonald , T. S. McShane , N. G. Minaev , S. Mioduszewski , B. Mohanty , M. M. Mondal , D. A. Morozov , M. G. Munhoz , M. K. Mustafa , B. K. Nandi , Md. Nasim , T. K. Nayak , J. M. Nelson , L. V. Nogach , S. Y. Noh , J. Novak , S. B. Nurushev , G. Odyniec , A. Ogawa , K. Oh , A. Ohlson , V. Okorokov , E. W. Oldag , R. A. N. Oliveira , M. Pachr , B. S. Page , S. K. Pal , Y. X. Pan , Y. Pandit , Y. Panebratsev , T. Pawlak , B. Pawlik , H. Pei , C. Perkins , W. Peryt , P. Pile , M. Planinic , J. Pluta , D. Plyku , N. Poljak , J. Porter , A. M. Poskanzer , N. K. Pruthi , M. Przybycien , P. R. Pujahari , H. Qiu , A. Quintero , S. Ramachandran , R. Raniwala , S. Raniwala , R. L. Ray , C. K. Riley , H. G. Ritter , J. B. Roberts , O. V. Rogachevskiy , J. L. Romero , J. F. Ross , A. Roy , L. Ruan , J. Rusnak , N. R. Sahoo , P. K. Sahu , I. Sakrejda , S. Salur , A. Sandacz , J. Sandweiss , E. Sangaline , A. Sarkar , J. Schambach , R. P. Scharenberg , A. M. Schmah , W. B. Schmidke , N. Schmitz , J. Seger , P. Seyboth , N. Shah , E. Shahaliev , P. V. Shanmuganathan , M. Shao , B. Sharma , W. Q. Shen , S. S. Shi , Q. Y. Shou , E. P. Sichtermann , R. N. Singaraju , M. J. Skoby , D. Smirnov , N. Smirnov , D. Solanki , P. Sorensen , U. G. deSouza , H. M. Spinka , B. Srivastava , T. D. S. Stanislaus , J. R. Stevens , R. Stock , M. Strikhanov , B. Stringfellow , A. A. P. Suaide , M. Sumbera , X. Sun , X. M. Sun , Y. Sun , Z. Sun , B. Surrow , D. N. Svirida , T. J. M. Symons , A. Szanto de Toledo , J. Takahashi , A. H. Tang , Z. Tang , T. Tarnowsky , J. H. Thomas , A. R. Timmins , D. Tlusty , M. Tokarev , S. Trentalange , R. E. Tribble , P. Tribedy , B. A. Trzeciak , O. D. Tsai , J. Turnau , T. Ullrich , D. G. Underwood , G. Van Buren , G. van Nieuwenhuizen , J. A. Vanfossen, , R. Varma , G. M. S. Vasconcelos , A. N. Vasiliev , R. Vertesi , F. Videbæk , Y. P. Viyogi , S. Vokal , A. Vossen , M. Wada , M. Walker , F. Wang , G. Wang , H. Wang , J. S. Wang , X. L. Wang , Y. Wang , Y. Wang , G. Webb , J. C. Webb , G. D. Westfall , H. Wieman , S. W. Wissink , R. Witt , Y. F. Wu , Z. Xiao , W. Xie , K. Xin , H. Xu , N. Xu , Q. H. Xu , Y. Xu , Z. Xu , W. Yan , C. Yang , Y. Yang , Y. Yang , Z. Ye , P. Yepes , L. Yi , K. Yip , I-K. Yoo , Y. Zawisza , H. Zbroszczyk , W. Zha , J. B. Zhang , J. L. Zhang , S. Zhang , X. P. Zhang , Y. Zhang , Z. P. Zhang , F. Zhao , J. Zhao , C. Zhong , X. Zhu , Y. H. Zhu , Y. Zoulkarneeva , M. Zyzak

The spatial resolution along the pad-row direction was measured with a GEM-based TPC prototype for the future linear collider experiment in order to understand its performance for tracks with finite projected angles with respect to the…

Observation of redshifted 21-cm signals from neutral hydrogen holds the key to understanding the structure formation and its evolution during the reionization and post-reionization era. Apart from the presence of orders of magnitude larger…

Instrumentation and Methods for Astrophysics · Physics 2022-03-02 Jais Kumar , Prasun Dutta , Samir Choudhuri , Nirupam Roy

The 21cm background from the epoch of reionization is a promising cosmological probe: line-of-sight velocity fluctuations distort redshift, so brightness fluctuations in Fourier space depend upon angle, which linear theory shows can…

Cosmology and Nongalactic Astrophysics · Physics 2013-04-17 Paul R. Shapiro , Yi Mao , Ilian T. Iliev , Garrelt Mellema , Kanan K. Datta , Kyungjin Ahn , Jun Koda

The ICARUS liquid argon time projection chamber (LArTPC) neutrino detector has been taking physics data since 2022 as part of the Short-Baseline Neutrino (SBN) Program. This paper details the equalization of the response to charge in the…

High Energy Physics - Experiment · Physics 2024-08-06 ICARUS collaboration , P. Abratenko , N. Abrego-Martinez , A. Aduszkiewic , F. Akbar , L. Aliaga Soplin , M. Artero Pons , J. Asaadi , W. F. Badgett , B. Baibussinov , B. Behera , V. Bellini , R. Benocci , J. Berger , S. Berkman , S. Bertolucci , M. Betancourt , M. Bonesini , T. Boone , B. Bottino , A. Braggiotti , D. Brailsford , S. J. Brice , V. Brio , C. Brizzolari , H. S. Budd , A. Campani , A. Campos , D. Carber , M. Carneiro , I. Caro Terrazas , H. Carranza , F. Castillo Fernandez , A. Castro , S. Centro , G. Cerati , A. Chatterjee , D. Cherdack , S. Cherubini , N. Chitirasreemadam , M. Cicerchia , T. E. Coan , A. Cocco , M. R. Convery , L. Cooper-Troendle , S. Copello , A. A. Dange , A. de Roeck , S. Di Domizio , L. Di Noto , C. Di Stefano , D. Di Ferdinando , M. Diwan , S. Dolan , L. Domine , S. Donati , F. Drielsma , J. Dyer , S. Dytman , A. Falcone , C. Farnese , A. Fava , A. Ferrari , N. Gallice , F. G. Garcia , C. Gatto , D. Gibin , A. Gioiosa , W. Gu , A. Guglielmi , G. Gurung , H. Hausner , A. Heggestuen , B. Howard , R. Howell , I. Ingratta , C. James , W. Jang , Y. -J. Jwa , L. Kashur , W. Ketchum , J. S. Kim , D. -H. Koh , J. Larkin , Y. Li , C. Mariani , C. M. Marshall , S. Martynenko , N. Mauri , K. S. McFarland , D. P. Méndez , A. Menegolli , G. Meng , O. G. Miranda , A. Mogan , N. Moggi , E. Montagna , C. Montanari , A. Montanari , M. Mooney , G. Moreno-Granados , J. Mueller , M. Murphy , D. Naples , V. C. L. Nguyen , S. Palestini , M. Pallavicini , V. Paolone , R. Papaleo , L. Pasqualini , L. Patrizii , L. Paudel , G. Petrillo , C. Petta , V. Pia , F. Pietropaolo , F. Poppi , M. Pozzato , G. Putnam , X. Qian , A. Rappoldi , G. L. Raselli , S. Repetto , F. Resnati , A. M. Ricci , G. Riccobene , E. Richards , M. Rosenberg , M. Rossella , P. Roy , C. Rubbia , M. Saad , S. Saha , P. Sala , S. Samanta , P. Sapienza , A. Scaramelli , A. Scarpelli , D. Schmitz , A. Schukraft , D. Senadheera , S-H. Seo , F. Sergiampietri , G. Sirri , J. S. Smedley , J. Smith , L. Stanco , J. Stewart , H. A. Tanaka , F. Tapia , M. Tenti , K. Terao , F. Terranova , V. Togo , D. Torretta , M. Torti , F. Tortorici , R. Triozzi , Y. -T. Tsai , S. Tufanli , T. Usher , F. Varanini , S. Ventura , M. Vicenzi , C. Vignoli , B. Viren , Z. Williams , R. J. Wilson , P. Wilson , J. Wolfs , T. Wongjirad , A. Wood , E. Worcester , M. Wospakrik , H. Yu , J. Yu , A. Zani , J. Zennamo , J. Zettlemoyer , C. Zhang , S. Zucchelli

We report the serendipitous discovery of a faint (M_UV > -12.2), low-metallicity (Z ~ 0.02 Zsun), ionizing source (dubbed T2c) with a spectroscopic redshift of z=6.146. T2c is part of a larger structure amplified by the Hubble Frontier…

The ICARUS T600 LAr TPC is the far detector of the Short Baseline Program at FNAL. As it will have to work at shallow depth in the Booster Neutrino Beam, a large cosmic rays background ($\sim 11$ kHz) will be present. To reduce it, precise…

Instrumentation and Detectors · Physics 2020-06-24 M. Bonesini , R. Benocci , R. Bertoni , A. Falcone , R. Mazza , M. Torti , A. Menegolli , G. L. Raselli , M. Rossella

Besides the need of Stark broadening parameters for a number of problems in physics, and plasma technology, in hot star atmospheres the conditions exist where Stark widths are comparable and even larger than the thermal Doppler widths.…

Solar and Stellar Astrophysics · Physics 2018-03-14 Z. Simic , M. S. Dimitrijevic , A. B. Kovacevic , S. Sahal-Brechot

We present a physical-optics based theory of the physical mechanism for aberration of starlight. We apply non-relativistic and relativistic theories for wavefront image formation and include the effects of optically transmitting media…

Instrumentation and Methods for Astrophysics · Physics 2013-06-28 Robert A. Woodruff

The heavy ion physics approach to global event characterization has led us to instrument the forward region in the PHENIX experiment at RHIC. In heavy ion collisions this coverage yields a measurement of the "spectator" energy and its…

Nuclear Experiment · Physics 2008-11-26 Sebastian N. White

Neutrinos, elusive and abundant, interact weakly with matter, making detection challenging. This thesis explores neutrino physics, focusing on mass hierarchy and oscillations, with emphasis on India's upcoming INO facility. The Iron…

Instrumentation and Detectors · Physics 2025-07-31 Tanay Dey

The ability to observe extrasolar planets transiting their stars has profoundly changed our understanding of these planetary systems. However, these measurements depend on how well we understand the properties of the host star, such as…

Solar and Stellar Astrophysics · Physics 2022-06-15 Hilding R. Neilson , John B. Lester , Fabien Baron
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