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One of the most energetic events in the Universe are core-collapse Supernovae (SNe), where almost all the star's binding energy is released as neutrinos. These particles are direct probes of the processes occurring in the stellar core and…

Neutrino induced reactions on $^{12}$C, an ingredient of liquid scintillators, have been studied in several experiments. We show that for currently available neutrino energies, $E_{\nu} \le$ 300 MeV, calculated exclusive cross sections…

Nuclear Theory · Physics 2008-11-26 J. Engel , E. Kolbe , K. Langanke , P. Vogel

The cross sections of 110 radioactive nuclide with mass numbers 22 < A < 198 amu from the interaction of 2.2 GeV/nucleon deuterons from the Nuclotron of the Laboratory of High Energies (LHE), Joint Institute for Nuclear Research (JINR) at…

Ac electrical measurements have been reported for alkali halide mixed crystals that were melt grown from NaCl, KCl and KBr starting materials. They showed a nonlinear variation of all the electrical parameters with the bulk composition.…

Materials Science · Physics 2017-05-03 Vassiliki Katsika-Tsigourakou

We study electron-neutrino and electron-antineutrino signals from a supernova with strong magnetic field detected by a 100 kton liquid Ar detector. The change of neutrino flavors by resonant spin-flavor conversions, matter effects, and…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Takashi Yoshida , Akira Takamura , Keiichi Kimura , Shio Kawagoe , Toshitaka Kajino , Hidekazu Yokomakura

ZnO nanoparticles with Wurtzite structure were prepared by chemical methods at low temperature in aqueous solution. Nanoparticles are in the range from about 10 to 30 nm. Ferromagnetic properties were observed from 2 K to room temperature…

Mesoscale and Nanoscale Physics · Physics 2015-05-20 R. Escudero , R. Escamilla

Filled skutterudite compound EuFe$_4$As$_{12}$ shows the highest magnetic ordering temperature of $T_{\rm C}$ = 154 K among Eu-based skutterudite compounds, but its magnetic ground state has not been determined yet. Here, we performed…

Strongly Correlated Electrons · Physics 2020-08-26 Q. -P. Ding , H. -C. Lee , K. Nishine , Y. Kawamura , C. Sekine , Y. Furukawa

Using two different full-potential ab-initio techniques we introduce a simple, universal rule based on the number of broken first-neighbor bonds to determine the surface energies of the three noble metals Cu, Ag and Au. When a bond is…

Condensed Matter · Physics 2009-11-07 I. Galanakis , G. Bihlmayer , V. Bellini , N. Papanikolaou , R. Zeller , S. Bluegel , P. H. Dederichs

Neutrino interactions with lead produce neutrons in numbers that depend on neutrino energy and type. A detector based on lead perchlorate, for example, would be able to measure the energy deposited by electrons and gammas in coincidence…

Astrophysics · Physics 2011-07-19 S. R. Elliott

The properties of the relative abundances of rapid and slow neutron-capture elements are studied using a catalog containing spectroscopic abundance determinations for 14~elements produced in various nuclear-synthesis processes for 90~open…

Astrophysics of Galaxies · Physics 2016-02-22 V. A. Marsakov , M. L. Gozha , V. V. Koval' , L. V. Shpigel'

A preferred candidate for neutrinoless double-{\beta} decay, 150Nd, is present in natural neodymium at an abundance level of 5.64%. However, neodymium could be activated by cosmic rays during the period it spends on the Earth's surface. Its…

Nuclear Experiment · Physics 2012-02-24 O. Lebeda , V. Lozza , P. Schrock , J. Štursa , K. Zuber

The primary objective of this study is to accurately determine the abundances of Cu, Sr, Y, Zr, Ba, La, and Ce in selected solar-type stars. This will allow us to establish observational abundance-metallicity and abundance-age relations and…

Solar and Stellar Astrophysics · Physics 2024-07-23 Valentina Sheminova , Martina Baratella , Valentina D'Orazi

All existing positive results on two-neutrino double beta decay and two-neutrino double electron capture in different nuclei have been analyzed. Weighted average and recommended half-life values for $^{48}$Ca, $^{76}$Ge, $^{82}$Se,…

Nuclear Experiment · Physics 2020-10-01 Alexander Barabash

The first three electronically excited states in the alkaline-earth-metal atoms magnesium, calcium, and strontium comprise the (nsnp) triplet P^o_J (J=0,1,2) fine-structure manifold. All three states are metastable and are of interest for…

Atomic Physics · Physics 2009-11-10 Robin Santra , Kevin V. Christ , Chris H. Greene

The astrophysical origin of the rapid neutron-capture process (r-process), which produces about half of the elements heavier than iron, remains uncertain. The oldest, most metal-poor stars preserve the chemical signatures of early…

Results of the BM@N experiment at the Nuclotron/NICA complex on the production of protons, deuterons and tritons in interactions of an argon beam of 3.2 AGeV with fixed targets of C, Al, Cu, Sn and Pb are presented. Transverse mass spectra,…

High Energy Physics - Experiment · Physics 2025-06-11 S. Afanasiev , G. Agakishiev , A. Aleksandrov , E. Aleksandrov , I. Aleksandrov , P. Alekseev , K. Alishina , V. Astakhov , T. Aushev , V. Azorskiy , V. Babkin , N. Balashov , R. Barak , A. Baranov , D. Baranov , N. Baranova , N. Barbashina , S. Bazylev , M. Belov , D. Blau , V. Bocharnikov , G. Bogdanova , E. Bondar , E. Boos , E. Bozorov , M. Buryakov , S. Buzin , A. Chebotov , D. Chemezov , J. H. Chen , A. Demanov , D. Dementev , A. Dmitriev , J. Drnoyan , D. Dryablov , B. Dubinchik , P. Dulov , A. Egorov , D. Egorov , V. Elsha , A. Fediunin , A. Fedosimova , I. Filippov , I. Filozova , D. Finogeev , I. Gabdrakhmanov , O. Gavrischuk , K. Gertsenberger , O. Golosov , V. Golovatyuk , P. Grigoriev , M. Golubeva , F. Guber , S. Ibraimova , D. Idrisov , T. Idrissova , A. Ivashkin , A. Izvestnyy , V. Kabadzhov , A. Kakhorova , Sh. Kanokova , M. Kapishin , I. Kapitonov , V. Karjavin , D. Karmanov , N. Karpushkin , R. Kattabekov , V. Kekelidze , S. Khabarov , P. Kharlamov , G. Khudaiberdyev , A. Khvorostukhin , V. Kireyeu , Yu. Kiryushin , P. Klimai , V. Kolesnikov , A. Kolozhvari , Yu. Kopylov , M. Korolev , L. Kovachev , I. Kovalev , Yu. Kovalev , V. Kozlov , I. Kruglova , S. Kuklin , E. Kulish , A. Kurganov , V. Kutergina , A. Kuznetsov , E. Ladygin , D. Lanskoy , N. Lashmanov , I. Lebedev , V. Lenivenko , R. Lednicky , V. Leontiev , E. Litvinenko , D. Lyapin , Y. G. Ma , A. Makankin , A. Makhnev , A. Malakhov , M. Mamaev , A. Martemianov , M. Merkin , S. Merts , S. Morozov , Yu. Murin , K. Musaev , G. Musulmanbekov , D. Myktybekov , R. Nagdasev , S. Nemnyugin , D. Nikitin , R. Nizamov , S. Novozhilov , A. Olimov , Kh. Olimov , K. Olimov , V. Palichik , P. Parfenov , I. Pelevanyuk , D. Peresunko , S. Piyadin , M. Platonova , V. Plotnikov , D. Podgainy , I. Pshenichnov , N. Pukhaeva , F. Ratnikov , S. Reshetova , V. Rogov , I. Romanov , I. Rufanov , P. Rukoyatkin , M. Rumyantsev , T. Rybakov , D. Sakulin , S. Savenkov , D. Serebryakov , A. Shabanov , S. Sergeev , A. Serikkanov , A. Sheremetev , A. Sheremeteva , A. Shchipunov , M. Shitenkov , M. Shodmonov , M. Shopova , A. Shutov , V. Shutov , I. Slepnev , V. Slepnev , I. Slepov , A. Smirnov , A. Solomin , A. Sorin , V. Spaskov , A. Stavinskiy , V. Stekhanov , Yu. Stepanenko , E. Streletskaya , O. Streltsova , M. Strikhanov , E. Sukhov , D. Suvarieva , A. Svetlichnyi , G. Taer , A. Taranenko , N. Tarasov , O. Tarasov , P. Teremkov , A. Terletsky , O. Teryaev , V. Tcholakov , V. Tikhomirov , A. Timoshenko , O. Tojiboev , N. Topilin , T. Tretyakova , V. Troshin , A. Truttse , I. Tserruya , V. Tskhay , I. Tyapkin , V. Ustinov , V. Vasendina , V. Velichkov , V. Volkov , A. Voronin , A. Voronin , N. Voytishin , B. Yuldashev , V. Yurevich , N. Zamiatin , M. Zavertyaev , S. Zhang , I. Zhavoronkova , N. Zhigareva , A. Zinchenko , R. Zinchenko , A. Zubankov , E. Zubarev , M. Zuev

We present Cu and Ba abundances for 7 G-K dwarf stars, members of the solar-metallicity, 0.3 Gyr old Ursa Major Moving Group. All analyzed member stars show [Ba/Fe] excesses of +0.3-plus, associated with [Cu/Fe] deficiencies of up to -0.23…

Astrophysics · Physics 2009-10-31 S. Castro , G. F. Porto de Mello , L. da Silva

X-ray photoelectron spectroscopy (XPS) and energy-dispersive X-ray spectroscopy (EDX) are applied to investigate the properties of fine-grained concentrate on artisanal small-scale gold mining samples from the Kubi Gold Project of the…

Materials Science · Physics 2021-11-01 Gabriel K. Nzulu , Babak Bakhit , Hans Högberg , Lars Hultman , Martin Magnuson

Supernova (SN) neutrinos can excite the nuclei of various detector materials beyond their neutron emission thresholds through charged current (CC) and neutral current (NC) interactions. The emitted neutrons, if detected, can be a signal for…

High Energy Astrophysical Phenomena · Physics 2017-03-29 Abhijit Bandyopadhyay , Pijushpani Bhattacharjee , Sovan Chakraborty , Kamales Kar , Satyajit Saha

The paper considers an opportunity of detecting explosives by using radiation capture of a neutron with nitrogen nucleus. Proton LINAC is offered as the neutron source with the following parameters: proton energy five Mega electron Volts ,…

Accelerator Physics · Physics 2016-06-27 S. N. Dolya
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