Literatura académica sobre el tema "Nuclear astrophysic"
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Artículos de revistas sobre el tema "Nuclear astrophysic"
Gyürky, György. "Challenges and Requirements in High-Precision Nuclear Astrophysics Experiments". Universe 8, n.º 4 (28 de marzo de 2022): 216. http://dx.doi.org/10.3390/universe8040216.
Texto completoDepalo, Rosanna. "Nuclear Astrophysics Deep Underground". International Journal of Modern Physics: Conference Series 46 (enero de 2018): 1860003. http://dx.doi.org/10.1142/s2010194518600030.
Texto completoAdsley, Philip. "Transfer Reactions in Nuclear Astrophysics". EPJ Web of Conferences 275 (2023): 01001. http://dx.doi.org/10.1051/epjconf/202327501001.
Texto completoDescouvemont, P. "Astrophysica for Windows: a PC software for nuclear astrophysics". Nuclear Physics A 688, n.º 1-2 (mayo de 2001): 557–59. http://dx.doi.org/10.1016/s0375-9474(01)00786-2.
Texto completoLépine-Szily, Alinka y Pierre Descouvemont. "Nuclear astrophysics: nucleosynthesis in the Universe". International Journal of Astrobiology 11, n.º 4 (9 de mayo de 2012): 243–50. http://dx.doi.org/10.1017/s1473550412000158.
Texto completoRAUSCHER, THOMAS. "THE PATH TO IMPROVED REACTION RATES FOR ASTROPHYSICS". International Journal of Modern Physics E 20, n.º 05 (mayo de 2011): 1071–169. http://dx.doi.org/10.1142/s021830131101840x.
Texto completoBroggini, Carlo. "Origin and status of LUNA at Gran Sasso". Modern Physics Letters A 29, n.º 34 (6 de noviembre de 2014): 1430038. http://dx.doi.org/10.1142/s0217732314300389.
Texto completoShen, Yang-Ping, Bing Guo y 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.
Texto completoCHAMPAGNE, A. E. y C. ILIADIS. "FIRST RESULTS FROM LENA". Modern Physics Letters A 22, n.º 04 (10 de febrero de 2007): 243–57. http://dx.doi.org/10.1142/s0217732307022724.
Texto completoPrati, 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.
Texto completoTesis sobre el tema "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.
Texto completoGNECH, 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.
Texto completoMarta, 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.
Texto completoMARCELLI, 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.
Texto completoPAMELA (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.
Texto completoDoherty, Daniel Thomas. "Experimental studies for explosive nuclear astrophysics". Thesis, University of Edinburgh, 2014. http://hdl.handle.net/1842/18022.
Texto completoMumby-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.
Texto completoTABASSAM, UZMA. "A Pair Spectrometer for Nuclear Astrophysics Applications". Doctoral thesis, Università degli Studi di Camerino, 2012. http://hdl.handle.net/11581/401785.
Texto completoRuiz, C. "Aspects of nuclear phenomena under explosive astrophysical conditions". Thesis, University of Edinburgh, 2003. http://hdl.handle.net/1842/11338.
Texto completoLuis, 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.
Texto completoThis 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.
Libros sobre el tema "Nuclear astrophysic"
Hillebrandt, Wolfgang, Rudolf Kuhfuß, Ewald Müller y James W. Truran, eds. Nuclear Astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016562.
Texto completoE, Vangioni-Flam y Institut d'astrophysique (Paris France), eds. Advances in nuclear astrophysics. Gif-sur-Yvette, France: Editions Frontières, 1986.
Buscar texto completoParticle astrophysics. 2a ed. Oxford: Oxford University Press, 2008.
Buscar texto completoParticle astrophysics. Oxford: Oxford University Press, 2003.
Buscar texto completoPerkins, Donald H. Particle astrophysics. 2a ed. Oxford: Oxford University Press, 2009.
Buscar texto completoS, Beskin V., North Atlantic Treaty Organization. Scientific Affairs Division. y 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.
Buscar texto completoRelativistic jets from active galactic nuclei. Weinheim, Germany: Wiley-VCH, 2012.
Buscar texto completoHigh energy astrophysics. 3a ed. Cambridge: Cambridge University Press, 2011.
Buscar texto completoParticle astrophysics. Bristol, UK: Institute of Physics Pub., 2000.
Buscar texto completoKlapdor-Kleingrothaus, H. V. Particle astrophysics. Bristol, UK: Institute of Physics Publ., 1997.
Buscar texto completoCapítulos de libros sobre el tema "Nuclear astrophysic"
Paetz gen. Schieck, Hans. "Nuclear Astrophysics". En Nuclear Reactions, 231–40. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-53986-2_14.
Texto completoLanganke, K. "Nuclear Astrophysics: Selected Topics". En 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.
Texto completovon Ballmoos, P. "Instruments for Nuclear Astrophysics". En High-Energy Spectroscopic Astrophysics, 82–197. Berlin, Heidelberg: Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/3-540-27013-2_2.
Texto completoBenhar, Omar y Stefano Fantoni. "Constraints from Astrophysical Data". En Nuclear Matter Theory, 121–34. Boca Raton: CRC Press, 2020.: CRC Press, 2020. http://dx.doi.org/10.1201/9781351175340-7.
Texto completoRebel, H. "Coulomb dissociation as a source of information on radiative capture processes of astrophysical interest". En Nuclear Astrophysics, 38–53. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016566.
Texto completoTornambè, A., F. Matteucci, I. Iben y K. Nomoto. "Binary systems as supernova progenitors (some frequency estimates)". En Nuclear Astrophysics, 283–92. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/bfb0016589.
Texto completoHashimoto, M., M. Kamimura y K. Arai. "Crucial Nuclear Reactions of Light Nuclei in Astrophysics". En Few-Body Problems in Physics ’99, 92–97. Vienna: Springer Vienna, 2000. http://dx.doi.org/10.1007/978-3-7091-6287-3_15.
Texto completoKubono, Shigeru. "Nuclear clustering aspects in astrophysics". En Atomic and Nuclear Clusters, 73–76. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79696-8_16.
Texto completoDescouvemont, P. "Cluster Models in Nuclear Astrophysics". En 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.
Texto completoWong, S. S. M. "Nuclear Astrophysics with Radioactive Beams". En Stellar Astrophysics, 51–60. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-010-0878-5_7.
Texto completoActas de conferencias sobre el tema "Nuclear astrophysic"
Litvinov, Yuri A. y Klaus Blaum. "Weighing exotic nuclei for nuclear astrophysics". En ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763375.
Texto completoRehm, K. E., Lídia S. Ferreira y Paramasivan Arumugan. "Proton-Rich Nuclei in Nuclear Astrophysics". En Proton Emitting Nuclei and Related Topics. AIP, 2007. http://dx.doi.org/10.1063/1.2827261.
Texto completode Oliveira Santos, François, Paraskevi Demetriou, Rauno Julin y Sotirios Harissopulos. "Nuclear astrophysics with light nuclei at GANIL". En FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 3. AIP, 2011. http://dx.doi.org/10.1063/1.3628360.
Texto completoSCHATZ, H. "NUCLEAR ASTROPHYSICS AND NUCLEI FAR FROM STABILITY". En Proceedings of the Eighteenth Lake Louise Winter Institute. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702777_0004.
Texto completoSpitaleri, 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". En 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.
Texto completoBOMBACI, IGNAZIO. "NUCLEAR ASTROPHYSICS". En Proceedings of the 9th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812705143_0003.
Texto completoMeyer, Mikko y Kai Zuber. "Nuclear Astrophysics". En 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_others04.
Texto completoVIGEZZI, E. "NUCLEAR ASTROPHYSICS". En Proceedings of the 11th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812708793_0015.
Texto completoHaxton, W. C. "Nuclear Astrophysics". En INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 9th Conference CIPAN2006. AIP, 2006. http://dx.doi.org/10.1063/1.2402595.
Texto completoDRAGO, ALESSANDRO. "NUCLEAR ASTROPHYSICS". En Proceedings of the 10th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701985_0009.
Texto completoInformes sobre el tema "Nuclear astrophysic"
Miller, Jonah. Nuclear Astrophysics and Astrophysical Transients. Office of Scientific and Technical Information (OSTI), noviembre de 2022. http://dx.doi.org/10.2172/1900461.
Texto completoArcones, Almudena, Jutta E. Escher y M. Others. White Paper on Nuclear Astrophysics and Low Energy Nuclear Physics - Part 1. Nuclear Astrophysics. Office of Scientific and Technical Information (OSTI), abril de 2016. http://dx.doi.org/10.2172/1248270.
Texto completoCooperstein, J. Nuclear astrophysics of supernovae. Office of Scientific and Technical Information (OSTI), enero de 1988. http://dx.doi.org/10.2172/6034283.
Texto completoPenionzhkevich, Yu E. Nuclear reactions in astrophysics. Physico-Technical Society of Kazakhstan, diciembre de 2017. http://dx.doi.org/10.29317/ejpfm.2017010202.
Texto completoSchramm, D. N. y A. V. Olinto. Nuclear physics and astrophysics. Office of Scientific and Technical Information (OSTI), septiembre de 1992. http://dx.doi.org/10.2172/7073919.
Texto completoJones, Katherine Louise. Direct Reactions for Nuclear Structure and Nuclear Astrophysics. Office of Scientific and Technical Information (OSTI), diciembre de 2014. http://dx.doi.org/10.2172/1166766.
Texto completoPalumbo, A. EMPIRE: A code for nuclear astrophysics. Office of Scientific and Technical Information (OSTI), diciembre de 2013. http://dx.doi.org/10.2172/1121215.
Texto completoMoeller, P., J. R. Nix y K. L. Kratz. Nuclear properties for astrophysical applications. Office of Scientific and Technical Information (OSTI), septiembre de 1994. http://dx.doi.org/10.2172/147731.
Texto completoWu, J. Theoretical nuclear physics and astrophysics. Final report. Office of Scientific and Technical Information (OSTI), marzo de 1998. http://dx.doi.org/10.2172/631234.
Texto completoMisch, Gordon, Matthew Mumpower, Yang Sun, Surja Ghorui y Projjwal Banerjee. Astromers: Nuclear Isomers with Astrophysical Consequences. Office of Scientific and Technical Information (OSTI), agosto de 2020. http://dx.doi.org/10.2172/1648047.
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