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Статті в журналах з теми "Nuclear astrophysic"
Gyürky, György. "Challenges and Requirements in High-Precision Nuclear Astrophysics Experiments." Universe 8, no. 4 (March 28, 2022): 216. http://dx.doi.org/10.3390/universe8040216.
Повний текст джерелаDepalo, Rosanna. "Nuclear Astrophysics Deep Underground." International Journal of Modern Physics: Conference Series 46 (January 2018): 1860003. http://dx.doi.org/10.1142/s2010194518600030.
Повний текст джерелаAdsley, Philip. "Transfer Reactions in Nuclear Astrophysics." EPJ Web of Conferences 275 (2023): 01001. http://dx.doi.org/10.1051/epjconf/202327501001.
Повний текст джерелаDescouvemont, P. "Astrophysica for Windows: a PC software for nuclear astrophysics." Nuclear Physics A 688, no. 1-2 (May 2001): 557–59. http://dx.doi.org/10.1016/s0375-9474(01)00786-2.
Повний текст джерелаLépine-Szily, Alinka, and Pierre Descouvemont. "Nuclear astrophysics: nucleosynthesis in the Universe." International Journal of Astrobiology 11, no. 4 (May 9, 2012): 243–50. http://dx.doi.org/10.1017/s1473550412000158.
Повний текст джерелаRAUSCHER, THOMAS. "THE PATH TO IMPROVED REACTION RATES FOR ASTROPHYSICS." International Journal of Modern Physics E 20, no. 05 (May 2011): 1071–169. http://dx.doi.org/10.1142/s021830131101840x.
Повний текст джерелаBroggini, Carlo. "Origin and status of LUNA at Gran Sasso." Modern Physics Letters A 29, no. 34 (November 6, 2014): 1430038. http://dx.doi.org/10.1142/s0217732314300389.
Повний текст джерелаShen, Yang-Ping, Bing Guo, and Wei-Ping Liu. "An indirect technique in nuclear astrophysics: alpha-cluster transfer reaction." EPJ Web of Conferences 260 (2022): 01001. http://dx.doi.org/10.1051/epjconf/202226001001.
Повний текст джерелаCHAMPAGNE, A. E., and C. ILIADIS. "FIRST RESULTS FROM LENA." Modern Physics Letters A 22, no. 04 (February 10, 2007): 243–57. http://dx.doi.org/10.1142/s0217732307022724.
Повний текст джерелаPrati, Paolo. "Underground Nuclear Astrophysics: pushing direct measurements toward the Gamow window." EPJ Web of Conferences 227 (2020): 01015. http://dx.doi.org/10.1051/epjconf/202022701015.
Повний текст джерелаДисертації з теми "Nuclear astrophysic"
MASHA, ELIANA. "ASTROPHYSICAL NUCLEAR REACTIONS ON NEON ISOTOPES AT LUNA." Doctoral thesis, Università degli Studi di Milano, 2022. http://hdl.handle.net/2434/899089.
Повний текст джерелаGNECH, ALEX. "Theoretical calculation of nuclear reactions of interest for Big Bang Nucleosynthesis." Doctoral thesis, Gran Sasso Science Institute, 2020. http://hdl.handle.net/20.500.12571/14971.
Повний текст джерелаMarta, Michele. "The 14N(p,γ)O15 reaction studied at low and high beam energy". Forschungszentrum Dresden, 2012. http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-93642.
Повний текст джерелаMARCELLI, LAURA. "PAMELA mission: in flight perfomances and preliminary measurements of nuclear abundances." Doctoral thesis, Università degli Studi di Roma "Tor Vergata", 2008. http://hdl.handle.net/2108/639.
Повний текст джерелаPAMELA (a “Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics”) experiment is a satellite-borne apparatus designed for precision studies of the charged particles in the cosmic radiation. The primary scientific goal is the study of the antimatter component of the cosmic radiation (antiprotons, 80 MeV - 190 GeV; and positrons, 50 MeV - 270 GeV) in order to search for evidence of dark matter particle annihilations. PAMELA will also search for primordial antinuclei (in particular, anti-helium), and test cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and studies of light nuclei and their isotopes. In addition, it will measure the light nuclear component of cosmic rays and investigate phenomena connected with Solar and Earth physics. PAMELA is installed inside a pressurized container attached to a Russian Resurs DK1 earth-observation satellite that was launched into space in an elliptical (350 - 600 km of altitude) orbit with an inclination of 70.0 degrees by a Soyuz-U rocket on June 15th 2006 from the Baikonur cosmodrome in Kazakhstan. The PAMELA apparatus comprises a magnetic spectrometer, a Time of Flight system, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. The combination of these devices allows antiparticles to be reliably identified from a large background of other charged particles. The semipolar orbit (70.0°) allows PAMELA to investigate a wide range of energies for antiprotons (80 MeV - 190 GeV) and positrons (50 MeV - 270 GeV). Three years of data taking will provide unprecedented statistics in this energy range and will set the upper limit for the ratio anti-He/He below 10^(-7). Before launch and during the first months of data taking, Quick Look Software (for mission monitoring in real time) and Data Analysis Software were developed. Furthermore measurements of the the light attenuation lengths and trigger efficiencies of the TOF scintillator system in the "flight" configuration were performed. Preliminary results of Boron to Carbon nuclear ratio in cosmic rays in the energy range from 200 MeV/n up to 25 GeV/n have been derived using combined data from Calorimeter, Tracker and TOF systems. This measurement is very important to put constraints to propagation parameters of cosmological models and, as a consequence, to make more easily visibile a possible small contamination from primary sources in antiprotons and positrons spectra. A better determination of the cosmic ray propagation is fundamental for the search of exotic matter, like dark matter candidates or antimatter produced in exotic processes, since the signature of such processes can be recognized only by knowing with great precision the fluxes due to the conventional production, acceleration and transport mechanisms.
Szabo, Anthony Paul. "High energy emissions for astrophysical objects." Title page, contents and abstract only, 1992. http://web4.library.adelaide.edu.au/theses/09PH/09phs996.pdf.
Повний текст джерелаDoherty, Daniel Thomas. "Experimental studies for explosive nuclear astrophysics." Thesis, University of Edinburgh, 2014. http://hdl.handle.net/1842/18022.
Повний текст джерелаMumby-Croft, Paul David. "Tactic : A New Detector for Nuclear Astrophysics." Thesis, University of York, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.507686.
Повний текст джерелаTABASSAM, UZMA. "A Pair Spectrometer for Nuclear Astrophysics Applications." Doctoral thesis, Università degli Studi di Camerino, 2012. http://hdl.handle.net/11581/401785.
Повний текст джерелаRuiz, C. "Aspects of nuclear phenomena under explosive astrophysical conditions." Thesis, University of Edinburgh, 2003. http://hdl.handle.net/1842/11338.
Повний текст джерелаLuis, Hélio Fernandes. "Study of nuclear reactions relevant for astrophysics by Micro-AMS." Doctoral thesis, Faculdade de Ciências e Tecnologia, 2013. http://hdl.handle.net/10362/11274.
Повний текст джерелаThis work of this thesis was dedicated to the application of the Micro-AMS(Accelerator Mass spectrometry with micro-beam) to the study of nuclear reactions relevant to Astrophysics, namely reactions involving the radioisotope 36Cl. Before this could be done, the system had to be installed, tested and optimized. During the installation and testing phase, several isotopes were measured, principally lead and platinum isotopes, which served to show the potential of this technique for applications to Material science and archeology. After this initial stage, the work with 36Cl began. 36Cl is one of several short to medium lived isotopes (as compared to the earth age) whose abundances in the earlier solar system may help to clarify its formation process. There are two generally accepted possible models for the production of this radionuclide: it originated from the ejecta of a nearby supernova (where 36Cl was most probably produced via the s-process by neutron irradiation of 35Cl) and/or it was produced by in-situ irradiation of nebular dust by energetic particles(mostly, p, a, 3He -X-wind irradiation model). The objective of the present work was to measure the cross section of the 35Cl(n,γ)36Cl nuclear reaction which opened the possibility to the future study of the 37Cl(p,d)36Cl and 35Cl(d,p)36Cl nuclear reactions, by measuring the 36Cl content of AgCl samples with Micro-AMS, taking advantage of the very low detection limits of this technique for chlorine measurements. For that, the micro-AMS system of the CTN-IST laboratory had to be optimized for chlorine measurements, as to our knowledge this type of measurements had never been performed in such a system (AMS with micro-beam). This thesis presents the results of these developments, namely the tests in terms of precision and reproducibility that were done by comparing AgCl blanks irradiated at the Portuguese National Reactor with standards produced by the dilution of the NIST SRM 4943 standard material. With these results the cross section of the 37Cl(n,γ)36Cl was calculated.
Книги з теми "Nuclear astrophysic"
Hillebrandt, Wolfgang, Rudolf Kuhfuß, Ewald Müller, and James W. Truran, eds. Nuclear Astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016562.
Повний текст джерелаE, Vangioni-Flam, and Institut d'astrophysique (Paris France), eds. Advances in nuclear astrophysics. Gif-sur-Yvette, France: Editions Frontières, 1986.
Знайти повний текст джерелаParticle astrophysics. 2nd ed. Oxford: Oxford University Press, 2008.
Знайти повний текст джерелаParticle astrophysics. Oxford: Oxford University Press, 2003.
Знайти повний текст джерелаPerkins, Donald H. Particle astrophysics. 2nd ed. Oxford: Oxford University Press, 2009.
Знайти повний текст джерелаS, Beskin V., North Atlantic Treaty Organization. Scientific Affairs Division., and Nato Advanced Study Institute (2002 : Les Houches, Haute-Savoie, France)., eds. Accretion discs, jets, and high energy phenomena in astrophysics =: Disques d'accrétion, jets et phénomènes de haute énergie en astrophysique : Ecole d'été de physique des Houches, Session LXXVIII, 29 July-23 August 2002 : Nato Advanced Study Institute, Euro Summer School, Ecole thématique du CNRS. Les Ulis: EDP Sciences, 2003.
Знайти повний текст джерелаRelativistic jets from active galactic nuclei. Weinheim, Germany: Wiley-VCH, 2012.
Знайти повний текст джерелаHigh energy astrophysics. 3rd ed. Cambridge: Cambridge University Press, 2011.
Знайти повний текст джерелаParticle astrophysics. Bristol, UK: Institute of Physics Pub., 2000.
Знайти повний текст джерелаKlapdor-Kleingrothaus, H. V. Particle astrophysics. Bristol, UK: Institute of Physics Publ., 1997.
Знайти повний текст джерелаЧастини книг з теми "Nuclear astrophysic"
Paetz gen. Schieck, Hans. "Nuclear Astrophysics." In Nuclear Reactions, 231–40. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-53986-2_14.
Повний текст джерелаLanganke, K. "Nuclear Astrophysics: Selected Topics." In The Hispalensis Lectures on Nuclear Physics Vol. 2, 173–216. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-44504-3_7.
Повний текст джерелаvon Ballmoos, P. "Instruments for Nuclear Astrophysics." In High-Energy Spectroscopic Astrophysics, 82–197. Berlin, Heidelberg: Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/3-540-27013-2_2.
Повний текст джерелаBenhar, Omar, and Stefano Fantoni. "Constraints from Astrophysical Data." In Nuclear Matter Theory, 121–34. Boca Raton: CRC Press, 2020.: CRC Press, 2020. http://dx.doi.org/10.1201/9781351175340-7.
Повний текст джерелаRebel, H. "Coulomb dissociation as a source of information on radiative capture processes of astrophysical interest." In Nuclear Astrophysics, 38–53. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016566.
Повний текст джерелаTornambè, A., F. Matteucci, I. Iben, and K. Nomoto. "Binary systems as supernova progenitors (some frequency estimates)." In Nuclear Astrophysics, 283–92. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016589.
Повний текст джерелаHashimoto, M., M. Kamimura, and K. Arai. "Crucial Nuclear Reactions of Light Nuclei in Astrophysics." In Few-Body Problems in Physics ’99, 92–97. Vienna: Springer Vienna, 2000. http://dx.doi.org/10.1007/978-3-7091-6287-3_15.
Повний текст джерелаKubono, Shigeru. "Nuclear clustering aspects in astrophysics." In Atomic and Nuclear Clusters, 73–76. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79696-8_16.
Повний текст джерелаDescouvemont, P. "Cluster Models in Nuclear Astrophysics." In Landolt-Börnstein - Group I Elementary Particles, Nuclei and Atoms, 27–45. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-22930-5_3.
Повний текст джерелаWong, S. S. M. "Nuclear Astrophysics with Radioactive Beams." In Stellar Astrophysics, 51–60. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-010-0878-5_7.
Повний текст джерелаТези доповідей конференцій з теми "Nuclear astrophysic"
Litvinov, Yuri A., and Klaus Blaum. "Weighing exotic nuclei for nuclear astrophysics." In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763375.
Повний текст джерелаRehm, K. E., Lídia S. Ferreira, and Paramasivan Arumugan. "Proton-Rich Nuclei in Nuclear Astrophysics." In Proton Emitting Nuclei and Related Topics. AIP, 2007. http://dx.doi.org/10.1063/1.2827261.
Повний текст джерелаde Oliveira Santos, François, Paraskevi Demetriou, Rauno Julin, and Sotirios Harissopulos. "Nuclear astrophysics with light nuclei at GANIL." In FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 3. AIP, 2011. http://dx.doi.org/10.1063/1.3628360.
Повний текст джерелаSCHATZ, H. "NUCLEAR ASTROPHYSICS AND NUCLEI FAR FROM STABILITY." In Proceedings of the Eighteenth Lake Louise Winter Institute. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702777_0004.
Повний текст джерелаSpitaleri, C., S. Cherubini, V. Crucillá, M. Gulino, M. La Cognata, L. Lamia, R. G. Pizzone, et al. "RECENT ASTROPHYSICAL APPLICATIONS OF THE TROJAN HORSE METHOD TO NUCLEAR ASTROPHYSICS." In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System. AIP, 2008. http://dx.doi.org/10.1063/1.2943570.
Повний текст джерелаBOMBACI, IGNAZIO. "NUCLEAR ASTROPHYSICS." In Proceedings of the 9th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812705143_0003.
Повний текст джерелаMeyer, Mikko, and Kai Zuber. "Nuclear Astrophysics." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_others04.
Повний текст джерелаVIGEZZI, E. "NUCLEAR ASTROPHYSICS." In Proceedings of the 11th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812708793_0015.
Повний текст джерелаHaxton, W. C. "Nuclear Astrophysics." In INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 9th Conference CIPAN2006. AIP, 2006. http://dx.doi.org/10.1063/1.2402595.
Повний текст джерелаDRAGO, ALESSANDRO. "NUCLEAR ASTROPHYSICS." In Proceedings of the 10th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701985_0009.
Повний текст джерелаЗвіти організацій з теми "Nuclear astrophysic"
Miller, Jonah. Nuclear Astrophysics and Astrophysical Transients. Office of Scientific and Technical Information (OSTI), November 2022. http://dx.doi.org/10.2172/1900461.
Повний текст джерелаArcones, Almudena, Jutta E. Escher, and M. Others. White Paper on Nuclear Astrophysics and Low Energy Nuclear Physics - Part 1. Nuclear Astrophysics. Office of Scientific and Technical Information (OSTI), April 2016. http://dx.doi.org/10.2172/1248270.
Повний текст джерелаCooperstein, J. Nuclear astrophysics of supernovae. Office of Scientific and Technical Information (OSTI), January 1988. http://dx.doi.org/10.2172/6034283.
Повний текст джерелаPenionzhkevich, Yu E. Nuclear reactions in astrophysics. Physico-Technical Society of Kazakhstan, December 2017. http://dx.doi.org/10.29317/ejpfm.2017010202.
Повний текст джерелаSchramm, D. N., and A. V. Olinto. Nuclear physics and astrophysics. Office of Scientific and Technical Information (OSTI), September 1992. http://dx.doi.org/10.2172/7073919.
Повний текст джерелаJones, Katherine Louise. Direct Reactions for Nuclear Structure and Nuclear Astrophysics. Office of Scientific and Technical Information (OSTI), December 2014. http://dx.doi.org/10.2172/1166766.
Повний текст джерелаPalumbo, A. EMPIRE: A code for nuclear astrophysics. Office of Scientific and Technical Information (OSTI), December 2013. http://dx.doi.org/10.2172/1121215.
Повний текст джерелаMoeller, P., J. R. Nix, and K. L. Kratz. Nuclear properties for astrophysical applications. Office of Scientific and Technical Information (OSTI), September 1994. http://dx.doi.org/10.2172/147731.
Повний текст джерелаWu, J. Theoretical nuclear physics and astrophysics. Final report. Office of Scientific and Technical Information (OSTI), March 1998. http://dx.doi.org/10.2172/631234.
Повний текст джерелаMisch, Gordon, Matthew Mumpower, Yang Sun, Surja Ghorui, and Projjwal Banerjee. Astromers: Nuclear Isomers with Astrophysical Consequences. Office of Scientific and Technical Information (OSTI), August 2020. http://dx.doi.org/10.2172/1648047.
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