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KEK-ATF is doing R&D establishing high-current and low-emittance electron beam for the future linear colliders. In ATF, 15 ps length electron beam is generated by combination of a thermionic gun, a couple of 357 MHz SHBs, and a S-band TW…

Accelerator Physics · Physics 2007-05-23 Masao Kuriki , Hitoshi Hayano , Katsushi Hasegawa

The MAJORANA collaboration is actively pursuing research and development aimed at a tonne-scale 76Ge neutrinoless double-beta decay) experiment. The current, primary focus is the construction of the MAJORANA DEMONSTRATOR experiment, an R&D…

Nuclear Experiment · Physics 2012-08-27 The MAJORANA Collaboration

Tunka-Rex, the Tunka Radio extension at the TAIGA facility (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) in Siberia, has recently been expanded to a total number 63 SALLA antennas, most of them distributed on an…

We show, through modeling and simulation, that it is feasible to construct a storage ring that will store dense bunches of strong-field-seeking polar molecules at 30 m/s (kinetic energy of 2K) and hold them, for several minutes, against…

Accelerator Physics · Physics 2009-11-11 Hiroshi Nishimura , Glen Lambertson , Juris G. Kalnins , Harvey Gould

The term beta-beam has been coined for the production of a pure beam of electron neutrinos or their antiparticles through the decay of radioactive ions circulating in a storage ring. This concept requires radioactive ions to be accelerated…

The Tunka Radio Extension (Tunka-Rex) is an antenna array consisting of 63 antennas at the location of the TAIGA facility (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) in Eastern Siberia, nearby Lake Baikal.…

China Spallation Neutron Source (CSNS) is a high intensity beam facility being built now in China. Three kicker assemblies, eight pulsed magnets, will be used in the CSNS rapid circle synchrotron (RCS). The physical and structural designs…

Accelerator Physics · Physics 2013-12-13 Wang Lei , Kang Wen , Hao Yao-Dou , Chen Yuan , Huo Li-Hua

The European XFEL is a new research facility currently under construction at DESY in the Hamburg area in Germany. From 2015 on, it will generate extremely intense X-ray flashes that will be used by researchers from all over the world. The…

Accelerator Physics · Physics 2015-06-16 J. Schaffran , Y. Bozhko , B. Petersen , D. Meissner , M. Chorowski , J. Polinski

The Radio-Frequency Quadrupole (RFQ) linac that will accelerate a 20mA proton beam from 50keV to 3MeV has been designed and is being fabricated as the first phase, KOMAC Test Facility (KTF), of the Korea Multipurpose Accelerator Complex…

Accelerator Physics · Physics 2007-05-23 J. M. Han

MITICA (Megavolt ITER Injector & Concept Advancement), the full scale prototype of ITER Heating Neutral Beam, is under realization at the Neutral Beam Test Facility (Padova, Italy). It is designed to deliver 16.5 MW to ITER plasma, obtained…

Investigation of neutrino oscillations and rare meson decays are main physics goals of Project X. The successful physics outcome relies on the feasibility of high-intensity neutrino and meson (K+ and \mu) beams. In order to meet this goal…

Accelerator Physics · Physics 2012-05-09 Henryk Piekarz

We are considering a two-beam accelerator (TBA) scheme with ion or proton beam as a driver. By comparison of the proposed scheme and the one with electron driver, we concluded, that TBA with ion/proton driver beam looks preferable.…

Accelerator Physics · Physics 2010-09-17 E. G. Bessonov , A. A. Mikhailichenko

The INTENTAS project aims to develop an atomic sensor utilizing entangled Bose-Einstein condensates (BECs) in a microgravity environment. This key achievement is necessary to advance the capability for measurements that benefit from both…

The Square Kilometer Array will be operating at the same time with several new large optical, X-ray and Gamma-ray facilities currently under construction or planned. Fostering synergies in astrophysical research made across different…

Astrophysics · Physics 2015-06-24 Andrei P. Lobanov

The Cherenkov Telescope Array (CTA) is the future instrument in ground-based gamma-ray astronomy in the energy range from 20 GeV to 300 TeV. Its sensitivity will surpass that of current generation experiments by a factor $\sim$10,…

Instrumentation and Methods for Astrophysics · Physics 2017-08-09 A. Schulz , M. Garczarczyk , L. Oakes , S. Schlenstedt , U. Schwanke , the CTA Consortium

There is X-ray, optical, and mid-infrared imaging and spectroscopic evidence that the late-stage ultraluminous infrared galaxy merger Mrk 273 hosts a powerful active galactic nucleus (AGN). However, the exact location of the AGN and the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Vivian U , Anne Medling , David Sanders , Claire Max , Lee Armus , Kazushi Iwasawa , Aaron Evans , Lisa Kewley , Giovanni Fazio

GRAND (the Giant Radio Array for Neutrino Detection) is a proposed next-generation observatory targetting primarily the detection of ultra-high-energy neutrinos, with energies exceeding about 100 PeV. GRAND is envisioned as a collection of…

Instrumentation and Methods for Astrophysics · Physics 2025-07-11 Olivier Martineau-Huynh

The Facility for Antiproton and Ion Research (FAIR) in Darmstadt, Germany, provides unique possibilities for a new generation of hadron-, nuclear- and atomic physics experiments. The future antiProton ANnihilations at DArmstadt (PANDA or…

High Energy Physics - Experiment · Physics 2021-06-10 G. Barucca , F. Davì , G. Lancioni , P. Mengucci , L. Montalto , P. P. Natali , N. Paone , D. Rinaldi , L. Scalise , B. Krusche , M. Steinacher , Z. Liu , C. Liu , B. Liu , X. Shen , S. Sun , G. Zhao , J. Zhao , M. Albrecht , W. Alkakhi , S. Bökelmann , S. Coen , F. Feldbauer , M. Fink , J. Frech , V. Freudenreich , M. Fritsch , J. Grochowski , R. Hagdorn , F. H. Heinsius , T. Held , T. Holtmann , I. Keshk , H. Koch , B. Kopf , M. Kümmel , M. Küßner , J. Li , L. Linzen , S. Maldaner , J. Oppotsch , S. Pankonin , M. Pelizäus , S. Pflüger , J. Reher , G. Reicherz , C. Schnier , M. Steinke , T. Triffterer , C. Wenzel , U. Wiedner , H. Denizli , N. Er , U. Keskin , S. Yerlikaya , A. Yilmaz , R. Beck , V. Chauhan , C. Hammann , J. Hartmann , B. Ketzer , J. Müllers , B. Salisbury , C. Schmidt , U. Thoma , M. Urban , A. Bianconi , M. Bragadireanu , D. Pantea , S. Rimjaem , M. Domagala , G. Filo , E. Lisowski , F. Lisowski , M. Michałek , P. Poznański , J. Płażek , K. Korcyl , P. Lebiedowicz , K. Pysz , W. Schäfer , A. Szczurek , M. Firlej , T. Fiutowski , M. Idzik , J. Moron , K. Swientek , P. Terlecki , G. Korcyl , R. Lalik , A. Malige , P. Moskal , K. Nowakowski , W. Przygoda , N. Rathod , P. Salabura , J. Smyrski , I. Augustin , R. Böhm , I. Lehmann , L. Schmitt , V. Varentsov , M. Al-Turany , A. Belias , H. Deppe , R. Dzhygadlo , H. Flemming , A. Gerhardt , K. Götzen , A. Heinz , P. Jiang , R. Karabowicz , S. Koch , U. Kurilla , D. Lehmann , J. Lühning , U. Lynen , H. Orth , K. Peters , J. Ritman , G. Schepers , C. J. Schmidt , C. Schwarz , J. Schwiening , A. Täschner , M. Traxler , B. Voss , P. Wieczorek , V. Abazov , G. Alexeev , M. Yu. Barabanov , V. Kh. Dodokhov , A. Efremov , A. Fechtchenko , A. Galoyan , G. Golovanov , E. K. Koshurnikov , Y. Yu. Lobanov , A. G. Olshevskiy , A. A. Piskun , A. Samartsev , S. Shimanski , N. B. Skachkov , A. N. Skachkova , E. A. Strokovsky , V. Tokmenin , V. Uzhinsky , A. Verkheev , A. Vodopianov , N. I. Zhuravlev , D. Watts , M. Böhm , W. Eyrich , A. Lehmann , D. Miehling , M. Pfaffinger , K. Seth , T. Xiao , A. Ali , A. Hamdi , M. Himmelreich , M. Krebs , S. Nakhoul , F. Nerling , P. Gianotti , V. Lucherini , G. Bracco , S. Bodenschatz , K. T. Brinkmann , L. Brück , S. Diehl , V. Dormenev , M. Düren , T. Erlen , C. Hahn , A. Hayrapetyan , J. Hofmann , S. Kegel , F. Khalid , I. Köseoglu , A. Kripko , W. Kühn , V. Metag , M. Moritz , M. Nanova , R. Novotny , P. Orsich , J. Pereira-de-Lira , M. Sachs , M. Schmidt , R. Schubert , M. Strickert , T. Wasem , H. G. Zaunick , E. Tomasi-Gustafsson , D. Glazier , D. Ireland , B. Seitz , R. Kappert , M. Kavatsyuk , H. Loehner , J. Messchendorp , V. Rodin , K. Kalita , G. Huang , D. Liu , H. Peng , H. Qi , Y. Sun , X. Zhou , M. Kunze , K. Azizi , A. T. Olgun , Z. Tavukoglu , A. Derichs , R. Dosdall , W. Esmail , A. Gillitzer , F. Goldenbaum , D. Grunwald , L. Jokhovets , J. Kannika , P. Kulessa , S. Orfanitski , G. Perez-Andrade , D. Prasuhn , E. Prencipe , J. Pütz , E. Rosenthal , S. Schadmand , R. Schmitz , A. Scholl , T. Sefzick , V. Serdyuk , T. Stockmanns , D. Veretennikov , P. Wintz , P. Wüstner , H. Xu , Y. Zhou , X. Cao , Q. Hu , Y. Liang , V. Rigato , L. Isaksson , P. Achenbach , O. Corell , A. Denig , M. Distler , M. Hoek , W. Lauth , H. H. Leithoff , H. Merkel , U. Müller , J. Petersen , J. Pochodzalla , S. Schlimme , C. Sfienti , M. Thiel , S. Bleser , M. Bölting , L. Capozza , A. Dbeyssi , A. Ehret , R. Klasen , R. Kliemt , F. Maas , C. Motzko , O. Noll , D. Rodríguez Piñeiro , F. Schupp , M. Steinen , S. Wolff , I. Zimmermann , D. Kazlou , M. Korzhik , O. Missevitch , P. Balanutsa , V. Chernetsky , A. Demekhin , A. Dolgolenko , P. Fedorets , A. Gerasimov , A. Golubev , A. Kantsyrev , D. Y. Kirin , N. Kristi , E. Ladygina , E. Luschevskaya , V. A. Matveev , V. Panjushkin , A. V. Stavinskiy , A. Balashoff , A. Boukharov , M. Bukharova , O. Malyshev , E. Vishnevsky , D. Bonaventura , P. Brand , B. Hetz , N. Hüsken , J. Kellers , A. Khoukaz , D. Klostermann , C. Mannweiler , S. Vestrick , D. Bumrungkoh , C. Herold , K. Khosonthongkee , C. Kobdaj , A. Limphirat , K. Manasatitpong , T. Nasawad , S. Pongampai , T. Simantathammakul , P. Srisawad , N. Wongprachanukul , Y. Yan , C. Yu , X. Zhang , W. Zhu , E. Antokhin , A. Yu. Barnyakov , K. Beloborodov , V. E. Blinov , I. A. Kuyanov , S. Pivovarov , E. Pyata , Y. Tikhonov , A. E. Blinov , S. Kononov , E. A. Kravchenko , M. Lattery , G. Boca , D. Duda , M. Finger , M. Finger, , A. Kveton , I. Prochazka , M. Slunecka , M. Volf , V. Jary , O. Korchak , M. Marcisovsky , G. Neue , J. Novy , L. Tomasek , M. Tomasek , M. Virius , V. Vrba , V. Abramov , S. Bukreeva , S. Chernichenko , A. Derevschikov , V. Ferapontov , Y. Goncharenko , A. Levin , E. Maslova , Y. Melnik , A. Meschanin , N. Minaev , V. Mochalov , V. Moiseev , D. Morozov , L. Nogach , S. Poslavskiy , A. Ryazantsev , S. Ryzhikov , P. Semenov , I. Shein , A. Uzunian , A. Vasiliev , A. Yakutin , S. Belostotski , G. Fedotov , A. Izotov , S. Manaenkov , O. Miklukho , B. Cederwall , M. Preston , P. E. Tegner , D. Wölbing , K. Gandhi , A. K. Rai , S. Godre , V. Crede , S. Dobbs , P. Eugenio , M. P. Bussa , S. Spataro , D. Calvo , P. De Remigis , A. Filippi , G. Mazza , R. Wheadon , F. Iazzi , A. Lavagno , A. Akram , H. Calen , W. Ikegami Andersson , T. Johansson , A. Kupsc , P. Marciniewski , M. Papenbrock , J. Regina , J. Rieger , K. Schönning , M. Wolke , A. Chlopik , G. Kesik , D. Melnychuk , J. Tarasiuk , M. Wojciechowski , S. Wronka , B. Zwieglinski , C. Amsler , P. Bühler , J. Marton , S. Zimmermann , C. S. Fischer , J. Haidenbauer , C. Hanhart , M. F. M. Lutz , Sinéad M. Ryan

We report ALMA observations of molecular gas and continuum emission in the 90 and 350 GHz bands toward a nearby Seyfert galaxy NGC 613. Radio continuum emissions were detected at 95 and 350 GHz from both the circum-nuclear disk (CND)…

Astrophysics of Galaxies · Physics 2018-02-05 Yusuke Miyamoto , Naomasa Nakai , Masumichi Seta , Dragan Salak , Makoto Nagai , Hiroyuki Kaneko
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