Academic literature on the topic 'Experimental nuclear astrophysic'

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Journal articles on the topic "Experimental nuclear astrophysic"

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Basu, Chinmay. "FRENA, a facility for research in experimental nuclear astrophysics at SINP, Kolkata." EPJ Web of Conferences 297 (2024): 01002. http://dx.doi.org/10.1051/epjconf/202429701002.

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FRENA is a new low energy high current accelerator facility commissioned at the Saha Institute of Nuclear Physics, Kolkata, India. The primary goal of the facility is to perform nuclear astrophysics experiments and address key issues in the field. It is a unique facility in India and is the first accelerator dedicated for astrophysical studies.
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RAUSCHER, THOMAS. "THE PATH TO IMPROVED REACTION RATES FOR ASTROPHYSICS." International Journal of Modern Physics E 20, no. 05 (2011): 1071–169. http://dx.doi.org/10.1142/s021830131101840x.

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This review focuses on nuclear reactions in astrophysics and, more specifically, on reactions with light ions (nucleons and α particles) proceeding via the strong interaction. It is intended to present the basic definitions essential for studies in nuclear astrophysics, to point out the differences between nuclear reactions taking place in stars and in a terrestrial laboratory, and to illustrate some of the challenges to be faced in theoretical and experimental studies of those reactions. The discussion revolves around the relevant quantities for astrophysics, which are the astrophysical react
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Guardo, G. L., D. Lattuada, and T. Petruse. "Developing system arrays for new experimental approach in nuclear astrophysics." Journal of Physics: Conference Series 2619, no. 1 (2023): 012009. http://dx.doi.org/10.1088/1742-6596/2619/1/012009.

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Abstract The advent of facilities providing high-intensity and high-resolution gamma ray beams and/or ultra-short and high-repetition laser pulses can potentially open a new path of astrophysical research. Indeed, a pencil size gamma beams with tunable energies from few keV up to tens MeV will offer distinctive chances to conduct precise measurements of small cross sections (on the scale of μb or even smaller) pertaining to nuclear reactions in the field of astrophysics. Consequently, it provides essential data for modeling astrophysical S-factors crucial to stellar evolution. On the other han
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Rapisarda, G. G., R. Spartá, and A. Tumino. "Few-Body Reactions with the Trojan Horse Method." EPJ Web of Conferences 290 (2023): 09009. http://dx.doi.org/10.1051/epjconf/202329009009.

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The Trojan Horse method (THM) is a well-established experimental technique to measure nuclear reactions of astrophysical interest avoiding the suppression of the Coulomb barrier affecting experimental direct measurements. In this paper it will describe some of the THM studies involving few-body system of interest for both nuclear physics and nuclear astrophysics, such as the sub-Coulomb proton-proton elastic scattering and the deuteron-deuteron fusion at energies of interest for primordial nucleosynthesis. Moreover, the role of the intercluster motion in nuclei used for THM measurement will be
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CHAMPAGNE, A. E., and C. ILIADIS. "FIRST RESULTS FROM LENA." Modern Physics Letters A 22, no. 04 (2007): 243–57. http://dx.doi.org/10.1142/s0217732307022724.

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We review the first results from the Laboratory for Experimental Nuclear Astrophysics (LENA), which is a dedicated accelerator facility for measuring reactions of astrophysical interest. We also briefly describe the facility itself and the detector system. The reactions that have been measured have relevance for both stellar evolution and for classical nova explosions.
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Shotter, A. C. "Experimental Nuclear Physics for Astrophysics." EAS Publications Series 11 (2004): 191–97. http://dx.doi.org/10.1051/eas:2004013.

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Wiescher, M. "Experimental Challenges in Nuclear Astrophysics." Nuclear Physics A 751 (April 2005): 285–300. http://dx.doi.org/10.1016/j.nuclphysa.2005.02.110.

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Cosentino, Luigi, and Cristian Massimi. "The n_ToF facility for Nuclear Astrophysics." EPJ Web of Conferences 331 (2025): 01002. https://doi.org/10.1051/epjconf/202533101002.

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Neutron-induced reactions involved in cosmological and stellar nucleosynthesis processes, represent key inputs for astrophysical models of the chemical evolution of the universe. Accurate knowledge of cross sections is essential to ensure high reliability of these models and to address discrepancies that still exist between models and observations. The availability of neutron beams with both high flux and energy resolution, combined with a large variety of innovative detectors, makes the n_TOF facility at CERN a unique tool for performing accurate measurements of astrophysical interest, even f
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Prati, 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.

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The aim of experimental nuclear astrophysics is to provide information on the nuclear processes involved in astrophysical scenarios at the relevant energy range. However, the measurement of the cross section of nuclear reactions at low energies present formidable difficulties due to the very low reaction rates often overwhelmed by the background. Several approaches have been proposed and exploited to overcome such severe obstacles: in such frame, the idea to install a low energy - high intensity ion accelerator deep underground, to gain high luminosity while reducing the cosmic ray background,
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Guardo, Giovanni Luca, Dario Lattuada та Teodora Petruse. "Developing system arrays for Nuclear Astrophysics with γ beams". EPJ Web of Conferences 331 (2025): 01003. https://doi.org/10.1051/epjconf/202533101003.

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The advent of advanced facilities capable of generating high-intensity, high-resolution gamma-ray beams unlocks exciting opportunities for astrophysical research. Tunable gamma-ray beams with energies spanning from a few keV to tens of MeV offer the precision needed to measure extremely small cross sections (on the order of µb or smaller) critical to nuclear reactions in astrophysics. These measurements will provide essential data for accurately modeling astrophysical S-factors, which play a key role in understanding stellar evolution. In photonuclear reactions of astrophysical significance, p
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Dissertations / Theses on the topic "Experimental nuclear astrophysic"

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MASHA, ELIANA. "ASTROPHYSICAL NUCLEAR REACTIONS ON NEON ISOTOPES AT LUNA." Doctoral thesis, Università degli Studi di Milano, 2022. http://hdl.handle.net/2434/899089.

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This thesis reports the direct measurements of the 22Ne(α,γ)26Mg and 20Ne(p,γ)21Na reactions at astrophysical energies of interest. The 22Ne(α,γ)26Mg reaction competes with the 22Ne(α,n)25Mg reaction which is the main source of neutrons for the s-process in low-mass Asymptotic Giant Branch and massive stars. At temperatures T < 300 MK where the (α,γ) channel becomes dominant, the rate of the 22Ne(α,γ)26Mg reaction is influenced by several resonances studied only indirectly. The first part of this thesis concerns the direct measurement of one of these resonances, Er = 334 keV, which so f
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Doherty, Daniel Thomas. "Experimental studies for explosive nuclear astrophysics." Thesis, University of Edinburgh, 2014. http://hdl.handle.net/1842/18022.

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In the ejecta from ONe novae outbursts nuclei up to A~40 are observed. The 30P(p,γ)31S reaction is thought to be the bottleneck for the production of all elements heavier than sulphur. However, due to uncertainties in the properties of key proton-unbound resonances the reaction rate is not well determined. In this thesis work, excited states in 31S were populated via the 28Si(4He,n) light-ion fusion-evaporation reaction and the prompt electromagnetic radiation was then detected with the GAMMASPHERE detector array. This γ-ray spectroscopy study, and comparisons with the stable mirror nucleus 31
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Álvarez, Pastor José Manuel. "Focal plane detectors of a Laue lens telescope for Nuclear Astrophysics." Doctoral thesis, Universitat Autònoma de Barcelona, 2012. http://hdl.handle.net/10803/83940.

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centenares de keV hasta unos pocos MeV), presenta un extraordinario potencial para comprender los procesos más extremos que tienen lugar en el Universo, como las explosiones estelares o los aceleradores de partículas. No obstante, a pesar de los enormes esfuerzos realizados por los observatorios de rayos gamma (en el pasado y en la actualidad), se requiere una mejora en la sensibilidad instrumental para aprovechar el enorme potencial científico contenido en este rango energético. Durante las dos últimas décadas se han buscado formas de mejorar la sensibilidad de los instrumentos, increm
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Depalo, Rosanna. "The neon-sodium cycle: Study of the 22Ne(p,gamma)23Na reaction at astrophysical energies." Doctoral thesis, Università degli studi di Padova, 2015. http://hdl.handle.net/11577/3424304.

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The 22Ne(p,gamma)23Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle plays a crucial role for the synthesis of the elements with mass A = 20-25 in asymptotic giant branch stars, classical novae explosions and type Ia supernovae, where hydrogen burning occurs at high temperatures. The 22Ne(p,gamma)23Na thermonuclear reaction rate is highly uncertain because of a large number of poorly known resonances lying at astrophysical energies. This thesis reports on a new experimental study of the 22Ne(p,gamma)23Na reaction. In particular, two experiments have been perfo
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Kamil, Mohamed. "Spectroscopy of proton unbound states in 32Cl." University of the Western Cape, 2019. http://hdl.handle.net/11394/6615.

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>Magister Scientiae - MSc<br>This project aimed to investigate proton unbound states in 32Cl using the 32S(3He; t) charge-exchange reaction. This research is relevant both in the context of nuclear structure and astrophysics. Excited states in 32Cl up to Ex 6 MeV were produced using a 50 MeV 3He++ beam from the K200 separated sector cyclotron at iThemba LABS. The triton ejectiles were mass analysed and detected at the focal plane of the K600 magnetic spectrometer. An additional segmented silicon detector array called CAKE was used to detect the unbound protons from states in 32Cl in
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Singh, Bhivek. "The design and simulation of a new experimental set up to measure nuclear level lifetimes." University of the Western Cape, 2016. http://hdl.handle.net/11394/5659.

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>Magister Scientiae - MSc<br>Measurements of nuclear level lifetimes are an important aspect of experimental nuclear physics. Such measurements determine transition matrix elements for nuclear structure research and also provide the widths of relevant excited states in nuclei that are of astrophysical interest. In the latter, the measured widths are used to obtain reaction rates in main sequence stars such as the Sun and in binary-star systems where the accretion of material from one star to another provides an opportunity to study extreme stellar environments such as novae and x-ray bursts. T
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Schmidt, Konrad. "Experimente zur Entstehung von Titan-44 in Supernovae." Forschungszentrum Dresden, 2012. http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-93636.

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In dieser Diplomarbeit wurde das astrophysikalisch interessante Resonanztriplett der Reaktion 40Ca(α,γ)44Ti bei 4,5MeV untersucht. Am 3-MV-Tandetron des Helmholtz-Zentrums Dresden-Rossendorf wurden dafür die Energien von Protonen- und -Strahlen kalibriert, Anregungsfunktionen im Energiebereich der drei Resonanzen aufgenommen, vier CaOTargets aktiviert und deren Struktur mittels der Reaktion 40Ca(p,γ)41Sc überprüft. Im Felsenkeller-Niederniveaumesslabor wurde anschließend die Aktivität der Proben gemessen. Schließlich konnte die Summe der Resonanzstärken bei 4497 und 4510 keV -Energie im Labors
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Howard, Meredith E. "The Joy of CEX: Sharpening the (t,3He) probe at 345 MeV for the charge-exchange knife drawer." Columbus, Ohio : Ohio State University, 2008. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1222168015.

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Chabert, Laurent. "Etude du bruit de fond neutron induit par les muons dans l'expérience EDELWEISS-II." Phd thesis, Université Claude Bernard - Lyon I, 2004. http://tel.archives-ouvertes.fr/tel-00007093.

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Plusieurs observations astronomiques indiquent que la densité de matière dans notre Univers est dominée par sa composante invisible. Parmi les particules pouvant constituer cette matière, le neutralino est un candidat supersymétrique favorisé. Cette thèse s'est faite dans le cadre de la collaboration EDELWEISS. Cette expérience tente de mettre en évidence l'interaction d'un neutralino avec un noyau cible. Les bolomètres utilisés par EDELWEISS associent à la détection des phonons celle des charges créées par le dépôt d'énergie. Cette double détection permet de rejeter une partie importante du b
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Anders, Michael. "S-factor measurement of the 2H(α,γ)6Li reaction at energies relevant for Big-Bang nucleosynthesis". Forschungszentrum Dresden, 2014. http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-141091.

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For about 20 years now, observations of 6Li in several old metal-poor stars inside the halo of our galaxy have been reported, which are largely independent of the stars’ metallicity, and which point to a possible primordial origin. The observations exceed the predictions of the Standard Big-Bang Nucleosynthesis model by a factor of 500. In the relevant energy range, no directly measured S-factors were available yet for the main production reaction 2H(α,γ)6Li, while different theoretical estimations have an uncertainty of up to two orders of magnitude. The very small cross section in the picoba
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Books on the topic "Experimental nuclear astrophysic"

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Klapdor-Kleingrothaus, H. V. Particle astrophysics. Institute of Physics Publ., 1997.

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Kyrala, George A. High energy density laboratory astrophysics. Springer, 2005.

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M, Kuster, Beltrán B, Raffelt Georg G, and European Organization for Nuclear Research., eds. Axions: Theory, cosmology, and experimental searches. Springer, 2008.

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Italy) European Summer School on Experimental Nuclear Astrophysics (3rd 2005 Santa Tecla. The Third European Summer School on Experimental Nuclear Astrophysics: Santa Tecla, Sicily, Itally, October 2-9, 2005. EDP Sciences, 2007.

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Topical Seminar on Experimental Apparatus for High Energy Particle Physics and Astrophysics (6th 1996 San Miniato, Italy). Experimental apparatus for particle physics and astrophysics: Proceedings of the 6th Topical Seminar on Experimental Apparatus for Particle Physics and Astrophysics, Centro Studi 'I Cappucini' della Cassa di Risparmo di San Miniato, San Miniato al Todesco, Italy, 20-24 May 1996. North-Holland, 1997.

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Topical Seminar on Experimental Apparatus for High Energy Particle Physics and Astrophysics (6th 1996 San Miniato, Italy). Experimental apparatus for particle physics and astrophysics: Proceedings of the 6th Topical Seminar on Experimental Apparatus for Particle Physics and Astrophysics, Centro Studi 'I Cappucini' della Cassa di Risparmo di San Miniato, San Miniato al Todesco, Italy, 20-24 May 1996. North-Holland, 1997.

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(Claudio), Spitaleri C., Rolfs Claus E, and Pizzone Rosario Gianluca, eds. Fifth European Summer School on Experimental Nuclear Astrophysics, Santa Tecla, Sicily, Italy, 20-27 September 2009. American Institute of Physics, 2010.

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1941-, Chaichian M., Huitu Katri, and Orava R. 1951-, eds. The First Arctic Workshop on Future Physics and Accelerators: Saariselkä, Finland, 21-26 August 1994. World Scientific, 1995.

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Klapdor-Kleingrothaus, H. V. Non-accelerator particle physics. Institute of Physics Pub., 1998.

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San Miniato Topical Seminar on Experimental Apparatus for High Energy Particle Physics and Astrophysics (1990 San Miniato, Italy). Experimental apparatus for high energy particle physics and astrophysics: 4th San Miniato Topical Seminar, San Miniato, Tuscany, Italy, 28 May-1 June 1990. Edited by Giusti Paolo, Navarria F. -L, and Pelfer P. G. World Scientific, 1991.

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Book chapters on the topic "Experimental nuclear astrophysic"

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Wiescher, Michael, Richard James deBoer, and René Reifarth. "Experimental Nuclear Astrophysics." In Handbook of Nuclear Physics. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-15-8818-1_116-1.

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Wiescher, Michael, Richard James deBoer, and René Reifarth. "Experimental Nuclear Astrophysics." In Handbook of Nuclear Physics. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-6345-2_116.

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Angulo, C. "Experimental Tools for Nuclear Astrophysics." In The Euroschool Lectures on Physics with Exotic Beams, Vol. III. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-85839-3_7.

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Leleux, Pierre. "Nuclear Astrophysics Experiments with Radioactive Beams." In Nuclei Far from Stability and Astrophysics. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0708-5_24.

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Kankainen, Anu, and Stephane Goriely. "Nuclear Data and Experiments for Astrophysics." In The Euroschool on Exotic Beams, Vol. VI. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-10751-1_4.

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Wiedeking, Mathis. "Experimental Facilities at iThemba LABS and Measurements to Constrain Astrophysical Processes." In Compound-Nuclear Reactions. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-58082-7_40.

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Halloin, Hubert. "Laue diffraction lenses for astrophysics: From theory to experiments." In Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands, 2006. http://dx.doi.org/10.1007/978-1-4020-5304-7_18.

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Takahashi, Tadayuki. "A Si/CdTe Compton Camera for gamma-ray lens experiment." In Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands, 2006. http://dx.doi.org/10.1007/978-1-4020-5304-7_32.

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Montagnani, Giovanni Ludovico. "Development of a 3” LaBr3 SiPM-Based Detection Module for High Resolution Gamma Ray Spectroscopy and Imaging." In Special Topics in Information Technology. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-62476-7_7.

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AbstractGamma radiation detection finds many applications in different fields, including astrophysics, nuclear physics and medical diagnostics. Nowadays large Lanthanum Bromide crystals coupled to Photomultiplier Tubes (PMTs) represent the state of the art for gamma detection modules, in particular for spectroscopic measurements. Nevertheless, there is an interest in substituting photomultiplier tubes with solid state photodetectors like Silicon Photomultipliers (SiPMs), owing to the latter’s significant advantages. These include insensitivity to magnetic fields, low bias voltage, compactness,
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Liu, WeiPing. "Progress of Underground Nuclear Astrophysics Experiment JUNA in China." In Springer Proceedings in Physics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-13876-9_39.

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Conference papers on the topic "Experimental nuclear astrophysic"

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Iliadis, Christian, Claudi Spitaleri, Claus Rolfs, and Rosario G. Pizzone. "Introduction to Nuclear Astrophysics." In FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3362604.

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Kubono, Shigeru. "Nuclear Clusters in Astrophysics." In VI European Summer School on Experimental Nuclear Astrophysics. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0036.

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Kubono, Shigeru, Claudi Spitaleri, Claus Rolfs, and Rosario G. Pizzone. "Nuclear Cluster Aspects in Astrophysics." In FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3362557.

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Fujita, Yoshitaka. "Weak interaction in nuclear astrophysics." In VI European Summer School on Experimental Nuclear Astrophysics. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0031.

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Trache, Livius. "Decay spectroscopic for nuclear astrophysics." In VI European Summer School on Experimental Nuclear Astrophysics. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0033.

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Trache, Livius, Claudi Spitaleri, Claus Rolfs, and Rosario G. Pizzone. "Indirect Methods For Nuclear Astrophysics With Radioactive Nuclear Beams." In FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3362561.

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Trache, Livius. "The ANC method in nuclear astrophysics." In VI European Summer School on Experimental Nuclear Astrophysics. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0030.

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Guglielmetti, Alessandra. "Nuclear astrophysics at LUNA: recent results." In VI European Summer School on Experimental Nuclear Astrophysics. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0057.

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Utsunomiya, Hiroaki. "Laser-Compton backscattering for nuclear astrophysics." In SEVENTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS: Proceedings of the 7th European Summer School on Experimental Nuclear Astrophysics. AIP Publishing LLC, 2014. http://dx.doi.org/10.1063/1.4875298.

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Barbui, M., W. Bang, A. Bonasera, et al. "A laser application to nuclear astrophysics." In SEVENTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS: Proceedings of the 7th European Summer School on Experimental Nuclear Astrophysics. AIP Publishing LLC, 2014. http://dx.doi.org/10.1063/1.4875305.

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Reports on the topic "Experimental nuclear astrophysic"

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Estrade, Alfredo. Time-of-flight experiments for nuclear structure and astrophysics. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1903697.

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Junghans, A., S. S. Westerdale, and P. Dimitriou. (alpha,n) Nuclear Data Evaluations and Data Needs. IAEA Nuclear Data Section, 2024. http://dx.doi.org/10.61092/iaea.d2d0-encd.

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The second IAEA Technical Meeting addressing (α,n) data needs for applications spanning reactor operation and safeguards, nonproliferation and spent fuel management, low-background experiments, and nuclear astrophysics was organized by the IAEA from 27 November to 1 December 2023. Fifty-six participants from thirteen Member States attended the virtual event. Participants reviewed the progress in (α,n) measurements, models, codes and evaluated libraries since the previous meeting of 2021. A summary of the presentations, technical discussions and recommendations is given in this report. The pres
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Westerdale, S. S., A. Junghans, R. J. deBoer, M. Pigni, and P. Dimitriou. Summary Report of the Technical Meeting on (alpha,n) Nuclear Data Evaluations and Data Needs. IAEA Nuclear Data Section, 2022. http://dx.doi.org/10.61092/iaea.vdj4-pakp.

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A Technical Meeting addressing (α,n) data needs for applications spanning reactor operation and safeguards, nonproliferation and spent fuel management, low-background experiments, and nuclear astrophysics was organised by the IAEA from 8 to 12 November 2021. Over 60 participants from fifteen Member States attended the virtual event. Participants reviewed the status of (α,n) measurements, models, codes and evaluated libraries with a view to identifying the gaps in the above areas and proposing the necessary actions to address them and produce reliable (α,n) data for the applications. A summary
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