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Journal articles on the topic 'Experimental nuclear astrophysic'

Author: Grafiati
Published: 9 March 2023
Last updated: 31 July 2025

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1

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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2

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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3

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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4

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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5

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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6

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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7

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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8

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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9

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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10

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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11

Rolfs, Claus. "Data needs in experimental nuclear astrophysics." Nuclear Physics News 4, no. 1 (1994): 17–20. http://dx.doi.org/10.1080/10506899408210217.

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12

Bardayan, D. W. "Recent Experimental Progress in Nuclear Astrophysics." Physics Procedia 66 (2015): 457–64. http://dx.doi.org/10.1016/j.phpro.2015.05.058.

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13

Aliotta, Marialuisa. "Experimental Nuclear Astrophysics in Underground Laboratories." Nuclear Physics News 22, no. 2 (2012): 13–17. http://dx.doi.org/10.1080/10619127.2012.683715.

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14

Cavanna, Francesca, and Paolo Prati. "Direct measurement of nuclear cross-section of astrophysical interest: Results and perspectives." International Journal of Modern Physics A 33, no. 09 (2018): 1843010. http://dx.doi.org/10.1142/s0217751x18430108.

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Stellar evolution and nucleosynthesis are interconnected by a wide network of nuclear reactions: the study of such connection is usually known as nuclear astrophysics. The main task of this discipline is the determination of nuclear cross-section and hence of the reaction rate in different scenarios, i.e. from the synthesis of a few very light isotopes just after the Big Bang to the heavy element production in the violent explosive end of massive stars. The experimental determination of reaction cross-section at the astrophysical relevant energies is extremely difficult, sometime impossible, d
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15

Frebel, Anna. "From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars." Annual Review of Nuclear and Particle Science 68, no. 1 (2018): 237–69. http://dx.doi.org/10.1146/annurev-nucl-101917-021141.

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Understanding the origin of the elements has been a decades-long pursuit, with many open questions remaining. Old stars found in the Milky Way and its dwarf satellite galaxies can provide answers because they preserve clean element abundance patterns of the nucleosynthesis processes that operated some 13 billion years ago, enabling reconstruction of the chemical evolution of the elements. This review focuses on the astrophysical signatures of heavy neutron-capture elements made in the s-, i-, and r-processes found in old stars. A highlight is the recently discovered r-process galaxy Reticulum
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16

Pizzone, R. G., C. Spampinato, M. L. Sergi, R. Spartá, and T. Zanatta-Martinez. "Investigating the Primordial Universe through nuclear physics." Journal of Physics: Conference Series 2619, no. 1 (2023): 012012. http://dx.doi.org/10.1088/1742-6596/2619/1/012012.

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Abstract Big Bang Nucleosynthesis (BBN) requires several nuclear physics inputs and nuclear reaction rates. An up-to-date compilation of direct cross sections of is given, being these ones among the most uncertain bare-nucleus cross sections. A particular attention is devoted to recently indirectly measured cross-section which give important hints for the nuclear astrophysics community. In reality, a significant experimental effort has been made over the past 10 years to explore reactions important to the BBN and determine their astrophysical S(E)-factor using the Trojan Horse Method (THM). Th
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17

Banu, Adriana. "Exploring the origin of the rarest stable isotopes naturally occurring on Earth with real photon beams." EPJ Web of Conferences 331 (2025): 01001. https://doi.org/10.1051/epjconf/202533101001.

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This lecture brings into focus research work that aims to advance fundamental knowledge on a forefront topic in nuclear astrophysics – the nucleosynthesis beyond Fe of the rarest stable isotopes naturally occurring on Earth (the origin of p-nuclei). The astrophysical phenomenon responsible for this synthesis is termed the p-process. Though modelling the p-process nucleosynthesis is a daunting task, significant progress can be made by performing key experimental studies, which can constrain Hauser-Feshbach statistical nuclear models used to calculate the many unknown astrophysically relevant st
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18

Goriely, S., A. Choplin, W. Ryssens, and I. Kullmann. "Progress in Nuclear Astrophysics: a multi-disciplinary field with still many open questions." Journal of Physics: Conference Series 2586, no. 1 (2023): 012104. http://dx.doi.org/10.1088/1742-6596/2586/1/012104.

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Abstract Nuclear astrophysics is a multi-disciplinary field with a huge demand for nuclear data. Among its various fields, stellar evolution and nucleosynthesis are clearly the most closely related to nuclear physics. The need for nuclear data for astrophysics applications challenges experimental techniques as well as the robustness and predictive power of present nuclear models. Despite impressive progress for the last years, major problems and puzzles remain. In the present contribution, only a few nuclear astrophysics specific aspects are discussed. These concern some experimental progress
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19

Saha, Sukhendu, Tanmoy Bar, and Chinmay Basu. "Background gamma measurement for low energy astrophysical reaction at FRENA." EPJ Web of Conferences 279 (2023): 13003. http://dx.doi.org/10.1051/epjconf/202327913003.

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The majority of astrophysical reactions have very low cross-sections (nanobarn to picobarn range) and significant error bars [1, 2]. Hence γ-ray background studies up to 3 MeV have been performed inside the Facility for Research in Experimental Nuclear Astrophysics (FRENA), Saha Institute of Nuclear Physics, Kolkata, India. A meticulous background calculation has been performed at different positions inside the accelerator hall and beam hall using two NaI(Tl) detectors [3]. An XPS measurement has been carried out to identify elements present in the FRENA wall concrete. Activity calculations do
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20

Su, Jun, Zhihong Li, Hao Zhang та ін. "Measurement of the low energy 25Mg(p,γ)26Al resonances". EPJ Web of Conferences 260 (2022): 08002. http://dx.doi.org/10.1051/epjconf/202226008002.

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The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The 26Al is mainly produced by the 25Mg(p,γ)26Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of 25Mg(p,γ)26Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy 25Mg(p,γ)26Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL).
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21

Axiotis, M., A. Lagoyannis, G. Provatas, et al. "New Instruments for Nuclear Astrophysics." HNPS Proceedings 23 (March 8, 2019): 8. http://dx.doi.org/10.12681/hnps.1900.

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A major task in experimental nuclear astrophysics is the measurement of cross sections of capture reactions. In the last years, the astrophysics group of NCSR “Demokritos” developed and used a method for conducting this kind of research using a 4π NaI γ-detector. Of great importance in this method is the determination of the efficiency of the detector, which depends on the average multiplicity of the γ-cascade de-exciting the entry state of the produced nucleus. Two new experimental setups have been studied and are in course of installation at the Tandem Laboratory of the Institute of Nuclear
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22

Wiescher, Michael. "Experimental Needs and Opportunities in Nuclear Astrophysics." Journal of Physics: Conference Series 420 (March 25, 2013): 012135. http://dx.doi.org/10.1088/1742-6596/420/1/012135.

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23

Wiescher, Michael. "Goals and challenges in experimental nuclear astrophysics." EPL (Europhysics Letters) 109, no. 6 (2015): 62001. http://dx.doi.org/10.1209/0295-5075/109/62001.

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24

Aliotta, M. "Experimental nuclear astrophysics with radioactive ion beams." European Physical Journal Special Topics 150, no. 1 (2007): 201–6. http://dx.doi.org/10.1140/epjst/e2007-00304-7.

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25

Bochum, C. Rolfs, C. Spitaleri Catania, and F. Terrasi Naples. "European summer school on experimental nuclear astrophysics." Nuclear Physics News 12, no. 1 (2002): 13. http://dx.doi.org/10.1080/10506890208235631.

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26

Bruno, C. G. "Experimental challenges in low-energy nuclear astrophysics." Journal of Physics: Conference Series 1078 (August 2018): 012007. http://dx.doi.org/10.1088/1742-6596/1078/1/012007.

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27

Fynbo, H. O. U. "Few-Body Problems in Experimental Nuclear Astrophysics." Few-Body Systems 54, no. 7-10 (2013): 843–48. http://dx.doi.org/10.1007/s00601-013-0646-9.

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28

Kubono, Shigeru. "Frontier in Experimental Nuclear Astrophysics in Japan." Journal of Nuclear Science and Technology 39, sup2 (2002): 524–29. http://dx.doi.org/10.1080/00223131.2002.10875155.

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29

Mascali, David, Domenico Santonocito, Simone Amaducci та ін. "A Novel Approach to β-Decay: PANDORA, a New Experimental Setup for Future In-Plasma Measurements". Universe 8, № 2 (2022): 80. http://dx.doi.org/10.3390/universe8020080.

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Theoretical predictions as well as experiments performed at storage rings have shown that the lifetimes of β-radionuclides can change significantly as a function of the ionization state. In this paper we describe an innovative approach, based on the use of a compact plasma trap to emulate selected stellar-like conditions. It has been proposed within the PANDORA project (Plasmas for Astrophysics, Nuclear Decay Observation and Radiation for Archaeometry) with the aim to measure, for the first time in plasma, nuclear β-decay rates of radionuclides involved in nuclear-astrophysics processes. To ac
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30

Khaliel, A., T. J. Mertzimekis, A. Psaltis, et al. "Experimental Investigation of radiative proton-capture reactions relevant to Nucleosynthesis." HNPS Proceedings 24 (April 1, 2019): 168. http://dx.doi.org/10.12681/hnps.1861.

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One of the primary objectives of the field of Nuclear Astrophysics is the study of the elemental and isotopic abundances in our solar system. Although a lot of progress has been made regarding a large number of nuclides, there is still a number of neutron-deficient nuclei, ie the p nuclei, which cannot be created via the s and r processes. These processes are responsible for the production of the bulk of heavy nuclides. The pre-explosive or explosive phases of massive stars are considered potential loci for p nuclides production via various combinations of photodisintegrations and nucleon capt
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31

Naselli, Eugenia, David Mascali, Claudia Caliri та ін. "Nuclear β-decays in plasmas: how to correlate plasma density and temperature to the activity". EPJ Web of Conferences 227 (2020): 02006. http://dx.doi.org/10.1051/epjconf/202022702006.

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Magnetized plasmas in compact traps may become experimental en-vironments for the investigation of nuclear beta-decays of astrophysical inter-est. In the framework of the project PANDORA (Plasmas for Astrophysics, Nuclear Decays Observation and Radiation for Archaeometry) the research ac-tivities are devoted to demonstrate the feasibility of an experiment aiming atmeasuring lifetimes of radionuclides of astrophysical interest when changing the charge state distribution of the in-plasma ions and the other plasma param- eters such as density and temperature. This contribution describes the multi
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32

Shubhchintak and Dinkar Sharma. "Theoretical applications to nuclear astrophysics." EPJ Web of Conferences 297 (2024): 01012. http://dx.doi.org/10.1051/epjconf/202429701012.

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Nuclear reaction study is important to understand elemental abundance in the universe and stability of stars. For several reactions due to the paucity of experimental data or diffculties in performing the direct measurements, we depend upon theoretical estimates and therefore one needs reliable theoretical models with minimum inputs. This paper is a short review of our work on nuclear reactions and their applications to astrophysics. In particular, we discuss the nuclear transfer and breakup reaction while focusing on our theoretical modelings and techniques involved.
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33

Käppeler, F., F. K. Thielemann, and M. Wiescher. "CURRENT QUESTS IN NUCLEAR ASTROPHYSICS AND EXPERIMENTAL APPROACHES." Annual Review of Nuclear and Particle Science 48, no. 1 (1998): 175–251. http://dx.doi.org/10.1146/annurev.nucl.48.1.175.

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34

Kubono, Shigeru. "Frontier in Experimental Nuclear Astrophysics with RI Beams." Progress of Theoretical Physics Supplement 146 (2002): 237–46. http://dx.doi.org/10.1143/ptps.146.237.

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35

Langanke, Karlheinz. "Nuclear data - an essential tool in nuclear astrophysics." EPJ Web of Conferences 284 (2023): 03001. http://dx.doi.org/10.1051/epjconf/202328403001.

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Nuclear processes play an essential role for the evolution of many astrophysical objects and they are key to the origin of the elements in the Universe. Our understanding of the Universe has benefitted from the tremendous progress in nuclear physics which became possible due to novel experimental facilities and improved instrumentation as well as due to advances in theoretical modelling. The talk exemplifies this progress for three selected topics: solar and stellar hydrostatic burning, neutron-star mergers as a site of heavy-element production by the r-process and the influence of electron ca
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36

Piatti, D. "The Study of the 6Li(p,γ)7Be Reaction at LUNA". Journal of Physics: Conference Series 1668, № 1 (2020): 012034. http://dx.doi.org/10.1088/1742-6596/1668/1/012034.

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Abstract The 6Li(p,γ)7Be reaction is mainly involved in two astrophysical scenarios: the primordial nucleosynthesis and 6Li consumption in pre-main and main sequence stars. A recent measurement of 6Li(p,γ)7Be reaction S-factor reported a resonance-like structure at Ecm = 195 keV, which has not been confirmed neither by other direct measurements nor by theoretical calculations. A new experiment was performed at the Laboratory for Underground Nuclear Astrophysics (LUNA). The extremely low background environment allowed to measure the 6Li(p,γ)7Be cross section down to low energies with unpreceden
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37

THIELEMANN, F. K., D. MOCELJ, I. PANOV, et al. "THE R-PROCESS: SUPERNOVAE AND OTHER SOURCES OF THE HEAVIEST ELEMENTS." International Journal of Modern Physics E 16, no. 04 (2007): 1149–63. http://dx.doi.org/10.1142/s0218301307006587.

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Rapid neutron capture in stellar explosions is responsible for the heaviest elements in nature, up to Th , U and beyond. This nucleosynthesis process, the r-process, is unique in the sense that a combination of nuclear physics far from stability (masses, half-lives, neutron-capture and photodisintegration, neutron-induced and beta-delayed fission and last but not least neutrino-nucleus interactions) is intimately linked to ejecta from astrophysical explosions (core collapse supernovae or other neutron star related events). The astrophysics and nuclear physics involved still harbor many uncerta
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38

Carmichael, Scott, Patrick O’Malley, Daniel Bardayan, et al. "The Enge Split-Pole Spectrograph at the University of Notre Dame." EPJ Web of Conferences 304 (2024): 02002. http://dx.doi.org/10.1051/epjconf/202430402002.

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Nuclear reactions play a crucial role in determining the nucleosynthesis that occurs in astrophysical events. The rates of many reactions that significantly impact certain nucleosynthesis processes can not be currently measured via direct means. These reactions must be constrained in another manner, such as determining the level energies and other structure properties of the compound nuclei. In order to measure level energies of nuclei relevant to nuclear astrophysics, the Enge split-pole spectrograph has been installed and commissioned at the University of Notre Dame’s Nuclear Science Laborat
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39

Chen, Meiyi. "Key Issues and Application Prospects in High-Temperature Plasma Physics." Academic Journal of Science and Technology 12, no. 3 (2024): 202–6. http://dx.doi.org/10.54097/ba0fpz05.

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High-temperature plasma physics is the core area of research into nuclear fusion energy, and it also has broad application potential in industry and astrophysics. The paper systematically reviews the fundamental definition, the formation mechanism, and research history of high-temperature plasma; analyzes focal problems including energy confinement, plasma instability, radiation cooling, material tolerance, turbulent dynamics; and discusses the technical progress and challenges of magnetic confinement and inertial confinement experimental devices. The comparison of tokamak against laser inerti
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40

Gning, Momar Talla, and Ibrahima Sakho. "Photoionization Study of Neutral Chlorine Atom." Atoms 11, no. 12 (2023): 152. http://dx.doi.org/10.3390/atoms11120152.

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Photoionization of neutral chlorine atom is investigated in this paper in the framework of the screening constant per unit nuclear charge (SCUNC) method. Resonance energies, quantum defects and effective charges of the 3s23p4 (3P2,1,0)ns and 3s23p4 (3P1,0)nd Rydberg series originating from both the 2P03/2 ground state and the 2P01/2 excited state of chlorine atom are reported. The present study believed to be the first theoretical investigation is compared with the recent experimental measurements (Yang et al., Astrophys. J. 810:132, 2015). Good agreements are obtained between theory and exper
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Demetriou, P. "Global predictions for astrophysics applications." HNPS Proceedings 13 (February 20, 2020): 18. http://dx.doi.org/10.12681/hnps.2953.

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Nuclear reaction rates play a crucial role in nuclear astrophysics. In the last decades there has been an enormous effort to measure reaction cross sections and extensive experimental databases have been compiled as a result. In spite of these efforts, most nuclear reaction network calculations still have to rely on theoretical predic- tions of experimentally unknown rates. In particular, in astrophysics applications such as the s-, r- and p-process nucleosynthesis involving a large number of nuclei and nuclear reactions (thousands). Moreover, most of the ingredients of the cal- culations of r
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42

Claudio, Spitaleri, Lamia Livio, and Pizzone Rosario Gianluca. "Preface: Eighth European Summer School on Experimental Nuclear Astrophysics." Journal of Physics: Conference Series 703 (April 2016): 011003. http://dx.doi.org/10.1088/1742-6596/703/1/011003.

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43

Wiescher, M. "Advances in experimental techniques and facilities for nuclear astrophysics." Nuclear Physics A 688, no. 1-2 (2001): 241–48. http://dx.doi.org/10.1016/s0375-9474(01)00707-2.

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44

Motobayashi, Tohru. "Experimental Studies of Nuclear Astrophysics with Fast RI beams." Journal of Nuclear Science and Technology 39, sup2 (2002): 558–61. http://dx.doi.org/10.1080/00223131.2002.10875162.

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45

Paradela, Carlos, Stefan Kopecky, and Peter Schillebeeckx. "Experimental work on Nuclear Astrophysics at JRC GELINA facility." EPJ Web of Conferences 279 (2023): 11008. http://dx.doi.org/10.1051/epjconf/202327911008.

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JRC Geel operates a neutron time-of-flight facility based on an electron accelerator, GELINA. Experimental setups to determine total and reaction cross sections (capture, elastic and inelastic scattering, fission and charged particle reactions) are available at measurement stations different flight-path length. While most of the experimental work is focussed on nuclear energy applications, regularly cross section of interest for astrophysical problems are measured. Examples of those are capture experiments of nuclei relevant for the s-process such as 89Y or the 16O (n,α) reaction which is the
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Erbacher, Philipp, Brückner Benjamin, Sophia Florence Dellmann, et al. "Direct reactions for nuclear astrophysics." EPJ Web of Conferences 279 (2023): 06005. http://dx.doi.org/10.1051/epjconf/202327906005.

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The neutron activation technique is a well established method to measure neutron capture cross sections relevant for the s-process. The 7Li(p,n) reaction at Ep = 1912 keV is often used as a neutron source since the energy distribution of the emitted neutrons closely resembles a Maxwell-Boltzmann spectrum of kBT = 25 keV, mimicking the 22Ne(α,n) phase in TP-AGB stars. The weak s-process, which takes place in massive stars, can reach energies up to kBT = 90 keV. Neutron spectra corresponding to a Maxwell-Boltzmann distribution with kBT > 25 keV cannot be produced by the 7Li(p,n) reaction dire
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47

Mrazek, J., V. Burjan, V. Kroha, et al. "ANC experiments for nuclear astrophysics in NPI CAS." EPJ Web of Conferences 184 (2018): 01014. http://dx.doi.org/10.1051/epjconf/201818401014.

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Asymptotic Normalization Coefficients method is one of the indirect methods used in nuclear astrophysics. The method allows to deduce a direct part of a radiative capture cross section from the measurement of a two body reaction under specific conditions. The experimental works started in collaboration of NPI CAS, TAMU and INFN LNS from 90-ties and continue till the present. The introduction to this method is presented and experimental experiences from NPI CAS and the collaboration are shared.
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48

Goriely, Stéphane, Wouter Ryssens, Stéphane Hilaire, and Sophie Péru. "Nuclear inputs relevant to nuclear astrophysics, status and perspectives." EPJ Web of Conferences 322 (2025): 09001. https://doi.org/10.1051/epjconf/202532209001.

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Nuclear physics influences are present throughout the Universe at every scale. Over the past decades, significant efforts have been dedicated to various fields related to nucleosynthesis and stellar evolution. These include both experimental and theoretical nuclear physics, as well as ground-and space-based astronomical observations and astrophysical modeling. Despite numerous successes, major challenges and unresolved questions persist. Concerning nuclear physics, despite the remarkable efforts of experimentalists in studying unstable targets, it remains unlikely that we will be able to measu
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49

Balabanski, Dimiter L. "Nuclear astrophysics studies with γ-ray beams: What do we expect to learn from them?" EPJ Web of Conferences 275 (2023): 01002. http://dx.doi.org/10.1051/epjconf/202327501002.

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An overview of the main directions of present-day studies with quasimonochromatic γ beams is discussed with an emphasis on the research opportunities which will be offered at the Extreme Light Infrastructure Nuclear Physics (ELI-NP) facility at Magurele near Bucharest in Romania. Experiments with γ beams at the extremes of high temperatures are outlined, with an emphasis on prospective studies related to nuclear astrophysics and astroparticle physics. Some of the experimental setups for nuclear structure, reaction, and astrophysics studies, which are available at ELI-NP, are described.
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50

Musumarra, Agatino. "From nuclear astrophysics to fundamental nuclear physics: challenging experimental approaches at n_TOF (CERN)." EPJ Web of Conferences 252 (2021): 05002. http://dx.doi.org/10.1051/epjconf/202125205002.

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The n_TOF installation at CERN is one of the leading neutron facilities worldwide undergoing a major update of the neutron spallation source. The update will provide improved n-TOF resolution in the experimental areas and the possibility to perform neutron cross section measurements at very high neutron flux (NEAR-Station). The renewed capabilities of the facility must be supported by smart and non-conventional experimental approaches. In this framework two examples will be reported. The first one concerns the measurement of a key reaction channel involved in Primordial Nucleosynthesis: the 7B
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