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Journal articles on the topic 'Nuclear Reactions'

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Published: 4 June 2021
Last updated: 29 July 2024

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1

S., M. "Nuclear questions, nuclear reactions." Psychological Perspectives 16, no. 1 (March 1985): 5–12. http://dx.doi.org/10.1080/00322928508407939.

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2

Frank, Patrick. "Nuclear Reactions." Afterimage 18, no. 8 (March 1, 1991): 7. http://dx.doi.org/10.1525/aft.1991.18.8.7.

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3

Bowdley, David, and Derek Swiffen. "Nuclear reactions." Physics World 7, no. 5 (May 1994): 21. http://dx.doi.org/10.1088/2058-7058/7/5/18.

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4

Dupont, Daniel G. "Nuclear Reactions." Scientific American 287, no. 2 (August 2002): 17–18. http://dx.doi.org/10.1038/scientificamerican0802-17.

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5

Howard, Brenda. "Nuclear reactions." Nature 437, no. 7061 (October 2005): 955. http://dx.doi.org/10.1038/437955a.

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6

SATCHLER, R. "Nuclear Reactions." Science 252, no. 5010 (May 31, 1991): 1325–26. http://dx.doi.org/10.1126/science.252.5010.1325.

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7

Spatafora, Alessandro, Diana Carbone, Francesco Cappuzzello, Manuela Cavallaro, Luis E. Acosta, Clementina Agodi, Paulina Amador-Valenzuela, et al. "The multichannel experimental and theoretical study of the 12C(18O,18F)12B single charge exchange reaction mechanism." EPJ Web of Conferences 292 (2024): 05003. http://dx.doi.org/10.1051/epjconf/202429205003.

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The study of a network of nuclear reactions populated in the 18O + 12C collision is the main topic of the present paper. It was performed to test nuclear structure and reaction theories in describing the full reaction mechanism occurring in the (18O, 18F) single charge exchange nuclear reaction. From the experimental side, an 18O beam was produced at 275 MeV incident energy by the K800 superconducting cyclotron and the MAGNEX magnetic spectrometer was used at the Laboratori Nazionali del Sud of the Istituto Nazionale di Fisica Nucleare to momentum analyse the ejectiles produced in the nuclear reactions within the same experimental setup. From the theoretical side, the proposed approach consists of analysing the whole network of nuclear reactions in the framework of a unique comprehensive and coherent theoretical calculation. This holistic approach, applied both to the experimental and theoretical analysis, is the main feature and novelty of the work presented here.
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8

Feshbach, Herman, and Ernest M. Henley. "Theoretical Nuclear Physics: Nuclear Reactions." Physics Today 45, no. 12 (December 1992): 84–85. http://dx.doi.org/10.1063/1.2809918.

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9

Babich, Leonid. "Thunderous nuclear reactions." Nature 551, no. 7681 (November 2017): 443–44. http://dx.doi.org/10.1038/d41586-017-07266-w.

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10

Glendenning, Norman K., and Ernest Rost. "Direct Nuclear Reactions." Physics Today 38, no. 6 (June 1985): 79. http://dx.doi.org/10.1063/1.2814602.

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11

Landowne, Stephen. "Direct nuclear reactions." Nuclear Physics A 435, no. 3-4 (March 1985): 860. http://dx.doi.org/10.1016/0375-9474(85)90193-9.

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12

De, Anuradha, Siddhartha Ray, and Sudip Kumar Ghosh. "Nuclear excitation and precompound nuclear reactions." Physical Review C 37, no. 6 (June 1, 1988): 2441–50. http://dx.doi.org/10.1103/physrevc.37.2441.

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13

Cardone, F., R. Mignani, and A. Petrucci. "Generalized Nuclear Reactions KEYWORDS: Piezonuclear Reactions, Local Lorentz Invariance, Nuclear Cycle." Journal of Advanced Physics 3, no. 2 (June 1, 2014): 150–52. http://dx.doi.org/10.1166/jap.2014.1113.

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14

Shaker Mehdy, Hala, Nariman Jabbar Qasim, Haider Hadi Abbas, Israa Al_Barazanchi, and Hassan Muwafaq Gheni. "Efficient time-series forecasting of nuclear reactions using swarm intelligence algorithms." International Journal of Electrical and Computer Engineering (IJECE) 12, no. 5 (October 1, 2022): 5093. http://dx.doi.org/10.11591/ijece.v12i5.pp5093-5103.

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In this research paper, we focused on the developing a secure and efficient time-series forecasting of nuclear reactions using swarm intelligence (SI) algorithm. Nuclear radioactive management and efficient time series for casting of nuclear reactions is a problem to be addressed if nuclear power is to deliver a major part of our energy consumption. This problem explains how SI processing techniques can be used to automate accurate nuclear reaction forecasting. The goal of the study was to use swarm analysis to understand patterns and reactions in the dataset while forecasting nuclear reactions using swarm intelligence. The results obtained by training the SI algorithm for longer periods of time for predicting the efficient time series events of nuclear reactions with 94.58 percent accuracy, which is higher than the deep convolution neural networks (DCNNs) 93% accuracy for all predictions, such as the number of active reactions, to see how the results can improve. Our earliest research focused on determining the best settings and preprocessing for working with a certain nuclear reaction, such as fusion and fusion task: forecasting the time series as the reactions took 0-500 ticks being trained on 300 epochs
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15

Spatafora, A., D. Carbone, F. Cappuzzello, M. Cavallaro, L. Acosta, C. Agodi, P. Amador-Valenzuela, et al. "Multi-channel experimental and theoretical approach to study the 12C(18O,18F)12B single charge exchange reaction." Journal of Physics: Conference Series 2453, no. 1 (March 1, 2023): 012019. http://dx.doi.org/10.1088/1742-6596/2453/1/012019.

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Abstract The broad network of nuclear reactions populated in the 18O + 12C collision was studied to test the capability of state-of-art nuclear structure and reaction theories to describe both the direct and sequential components of the (18O, 18F) single charge exchange nuclear reaction. The experiment was performed using the 18O beam at 275 MeV incident energy produced by the K800 superconducting cyclotron and the MAGNEX magnetic spectrometer at the Laboratori Nazionali del Sud of the Istituto Nazionale di Fisica Nucleare. A unique comprehensive and coherent theoretical calculation, able to describe the whole network of direct reactions, is the approach proposed for the first time to analyse this large set of experimental data. This holistic approach, applied both to the experimental and theoretical analysis, is the main feature and novelty of the work here presented.
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16

Carbone, D., C. Agodi, J. I. Bellone, S. Burrello, S. Calabrese, F. Cappuzzello, M. Cavallaro, et al. "The NUMEN project: probing nuclear response to weak interaction by nuclear reactions." Journal of Physics: Conference Series 2586, no. 1 (September 1, 2023): 012133. http://dx.doi.org/10.1088/1742-6596/2586/1/012133.

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Abstract Different reactions channels induced by the 18O + 40Ca collisions at 275 MeV incident energy are simultaneously measured and analysed consistently within the same reaction and structure frameworks within the NUMEN project. The project aims to provide data-driven information for the determination of the nuclear matrix elements involved in the neutrinoless double beta decay. In particular, the elastic and inelastic scattering, one- and two-proton transfer, one-neutron transfer, and single charge exchange reactions are explored. The full quantum-mechanical calculations, performed by including microscopic nuclear structure inputs, describe well all the experimental data, giving support to a multi-channel strategy for the analysis of heavy-ion induced direct reactions.
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17

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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18

Rumyantsev, B. A. "Turbulence in nuclear reactions." Physics of Atomic Nuclei 65, no. 5 (May 2002): 841–42. http://dx.doi.org/10.1134/1.1481475.

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19

Filippone, B. W. "Nuclear Reactions in Stars." Annual Review of Nuclear and Particle Science 36, no. 1 (December 1986): 717–43. http://dx.doi.org/10.1146/annurev.ns.36.120186.003441.

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20

Sitenko, A. G., and Ernest M. Henley. "Theory of Nuclear Reactions." Physics Today 44, no. 5 (May 1991): 64. http://dx.doi.org/10.1063/1.2810114.

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21

Langanke, K., H. Feldmeier, G. Martínez-Pinedo, and T. Neff. "Astrophysically important nuclear reactions." Progress in Particle and Nuclear Physics 59, no. 1 (July 2007): 66–73. http://dx.doi.org/10.1016/j.ppnp.2006.12.010.

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22

Rolfs, C. "Nuclear reactions in stars." Progress in Particle and Nuclear Physics 46, no. 1 (January 2001): 23–35. http://dx.doi.org/10.1016/s0146-6410(01)00104-1.

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23

Deltuva, A. "Few-body nuclear reactions." Journal of Physics: Conference Series 205 (January 1, 2010): 012017. http://dx.doi.org/10.1088/1742-6596/205/1/012017.

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24

Arnould, M., and M. Rayet. "Nuclear reactions in astrophysics." Annales de Physique 15, no. 3 (1990): 183–254. http://dx.doi.org/10.1051/anphys:01990001503018300.

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25

Fröbrich, Peter, Reinhard Lipperheide, and Ray Satchler. "Theory of Nuclear Reactions." Physics Today 50, no. 9 (September 1997): 68. http://dx.doi.org/10.1063/1.881917.

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26

De, A., A. Mitra, A. Ray, SR Banerjee, M. Sengupta, A. Chatterjee, S. Kailas, HS Patel, MG Betigiri, and SK Dutta. "Nuclear orbiting and anomalies in nuclear reactions." Pramana 53, no. 3 (September 1999): 549–52. http://dx.doi.org/10.1007/s12043-999-0029-4.

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27

RAUSCHER, 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.

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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 reaction rates. The sensitivity of the reaction rates to the uncertainties in the prediction of various nuclear properties is explored and some guidelines for experimentalists are also provided.
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28

NAVRÁTIL, PETR. "AB INITIO NUCLEAR STRUCTURE AND NUCLEAR REACTIONS IN LIGHT NUCLEI." International Journal of Modern Physics E 14, no. 01 (February 2005): 85–93. http://dx.doi.org/10.1142/s0218301305002801.

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There has been significant progress in the ab initio approaches to the structure of light nuclei. One such method is the ab initio no-core shell model (NCSM). Starting from the realistic two- and three-nucleon interactions, this method can predict the low-lying levels in p-shell nuclei. It is a challenging task to extend the ab initio methods to describe nuclear reactions. In this contribution, we present a brief overview of the NCSM with examples of recent applications as well as the first steps taken toward nuclear reaction applications.
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29

Nakamura, K., T. Takiwaki, K. Kotake, and N. Nishimura. "Neutrino-driven supernova explosions powered by nuclear reactions." Proceedings of the International Astronomical Union 7, S279 (April 2011): 365–66. http://dx.doi.org/10.1017/s1743921312013373.

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AbstractWe have investigated the revival of a shock wave by nuclear burning reactions at the central region of core-collapse supernovae. For this purpose, we performed hydrodynamic simulations of core collapse and bounce for 15 M⊙ progenitor model, using ZEUS-MP code in axi-symmetric coordinates. Our numerical code is equipped with a simple nuclear reaction network including 13 α nuclei form 4He to 56Ni, and accounting for energy feedback from nuclear reactions as well as neutrino heating and cooling. We found that the energy released by nuclear reactions is significantly helpful in accelerating shock waves and is able to produce energetic explosion even if the input neutrino luminosity is low.
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30

Azarkin, Maxim, Martin Kirakosyan, and Vladimir Ryabov. "Study of Nuclear Reactions in Therapy of Tumors with Proton Beams." International Journal of Molecular Sciences 24, no. 17 (August 29, 2023): 13400. http://dx.doi.org/10.3390/ijms241713400.

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This paper presents an assessment of nuclear reaction yields of protons, α-particles, and neutrons in human tissue-equivalentmaterial in proton therapy using a simulation with Geant 4. In this study, we also check an enhancement of nuclear reactions due to the presence of Bi, Au, 11B, and 10B radiosensitizer nanoparticles. We demonstrate that a proton beam induces a noticeable amount of nuclear reactions in the tissue. Nevertheless, the enhancement of nuclear reaction products due to radiosensitizer nanoparticles is found to be negligible.
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31

Hammache, Fairouz. "Transfer reactions for nuclear astrophysics." EPJ Web of Conferences 184 (2018): 01009. http://dx.doi.org/10.1051/epjconf/201818401009.

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Direct measurements of cross sections at stellar energies are very challenging - if at all possible. This is essentially due to the very low cross-sections of the reactions of interest (especially when it involves charged particles), and/or to the radioactive nature of many key nuclei. Direct measurements with charged particles are often performed at higher energies and then extrapolated down to stellar energies using R-matrix calculations. However, these extrapolations are delicate because of the possible existence of unobserved low-energy or sub-threshold resonances. In order to bypass the difficulties related to direct measurements, indirect methods such as transfer reactions are used. These experiments are usually performed at higher energies and their conditions are relatively less stringent than in direct measurements. However, these methods rely on theoretical models for which the input parameters may be an important source of systematic uncer-tainties and thus need to be determined carefully. In this manuscript, a short overview on the difficulties related to direct measurements will be given as well as a description of thetransfer reaction method and the theoretical concept behind. Finally, the method will be illustrated through two recent performed studies.
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32

LIU, WEI-PING, ZHI-HONG LI, XI-XIANG BAI, YOU-BAO WANG, GANG LIAN, BING GUO, SHENG ZENG, et al. "INDIRECT MEASUREMENTS OF NUCLEAR ASTROPHYSICS REACTIONS USING UNSTABLE NUCLEAR BEAMS." International Journal of Modern Physics E 15, no. 08 (November 2006): 1899–907. http://dx.doi.org/10.1142/s0218301306005514.

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This paper described the nuclear astrophysical studies using the unstable ion beam facility GIRAFFE, by indirect measurements. We measured the angular distributions for some single proton or neutron transfer reactions, such as 7 Be ( d,n )8 B , 11 C ( d,n )12 N , 8 Li ( d,n )9 Be , 8 Li ( d,p )9 Li and 13 N ( d,n )14 O in inverse kinematics, and derived the astrophysical S-factors or reaction rates of 7 Be ( p ,γ)8 B , 11 C ( p ,γ)12 N , 8 Li ( n ,γ)9 Li , 13 N ( p ,γ)14 O by asymptotic normalization coefficient, spectroscopic factor, and R-matrix approach at astrophysically relevant energies.
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33

E. Escher, J., J. T. Burke, R. J. Casperson, R. O. Hughes, and N. D. Scielzo. "One-nucleon pickup reactions and compound-nuclear decays." EPJ Web of Conferences 178 (2018): 03002. http://dx.doi.org/10.1051/epjconf/201817803002.

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One-nucleon transfer reactions, long used as a tool to study the structure of nuclei, are potentially valuable for determining reaction cross sections indirectly. This is significant, as many reactions of interest to astrophysics and other applications involve short-lived isotopes and cannot be measured directly. We describe a procedure for obtaining constraints for calculations of neutron capture cross sections using observables from experiments with transfer reactions. As a first step toward demonstrating the method, we outline the theory developments used to properly describe the production of the compound nucleus 88Y* via the one-nucleon pickup reaction 89Y(p,d)88Y* and test the description with data from a recent experiment. We indicate how this development can be used to extract the unknown 87Y(n,γ) cross section from 89Y(p,dγ) data. The example illustrates a more generally applicable method for determining unknown cross sections via a combination of theory and transfer (or inelastic scattering) experiments.
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34

Liu, Z. Y., K. Li, Y. L. Yao, Z. Lei, C. T. Zhou, S. P. Zhu, X. T. He, and B. Qiao. "Enhancement of nuclear reactions via the kinetic Weibel instability in plasmas." Plasma Physics and Controlled Fusion 63, no. 12 (November 15, 2021): 125030. http://dx.doi.org/10.1088/1361-6587/ac2e41.

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Abstract Nuclear reactions in the plasma environment can be substantially different from those in conventional laboratory non-plasma cases, which have attracted considerable attention in the fields of fusion and astrophysics. To self-consistently model the nuclear reaction process during plasma dynamic evolution, an extended nuclear reaction calculation module is developed and included in two-dimensional particle-in-cell simulations. Through the self-consistent simulations, we systematically show that, apart from the plasma screening, the kinetic Weibel instability (WI) occurring in plasmas also results in significant enhancement of nuclear reactions, where the self-generated magnetic fields play a key role. Specifically, the self-generated magnetic fields in WI deflect ion motions, decreasing the relative velocity, and convert plasma kinetic energy to thermal energy, increasing the ion temperature. The simulation results show that, for the t ( d , n ) α reaction with a sharp resonance peak in the cross section, the reaction product yield is enhanced four times due to the WI. For nuclear reactions that have more prominent resonance peaks in the cross section, like 12 C ( p , γ ) 13 N , it is expected that such enhancements can reach up to one or several orders of magnitude.
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35

Lenske, Horst. "Heavy Ion Charge Exchange Reactions as Probes for Beta–Decay." EPJ Web of Conferences 223 (2019): 01031. http://dx.doi.org/10.1051/epjconf/201922301031.

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Peripheral heavy ion single and double charge reactions are described by fully quantum mechanical distorted wave methods. A special class of nuclear double charge exchange (DCE) reactions proceeding as a one-step reaction through a two-body process are shown to proceed by nuclear matrix elements of a diagrammatic structure as found also in 0ν2ß decay. These hadronic Majorana-type DCE reactions (MDCE) have to be distinguished from second order DCE reactions, given by double single charge exchange (DSCE) processes, resembling 2ν2ß decay. The theoretical concepts of MDCE are discussed. First results show that ion-ion DCE reactions are the ideal testing grounds for investigations of rare second order nuclear processes, giving insight into nuclear in-medium two-body correlation.
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36

Petrescu, Relly Victoria Virgil, Raffaella Aversa, Antonio Apicella, and Florian Ion Petrescu. "Proposed Solutions to Achieve Nuclear Fusion." Engevista 19, no. 5 (December 4, 2017): 1496. http://dx.doi.org/10.22409/engevista.v19i5.968.

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Despite research carried out around the world since the 1950s, no industrial application of fusion to energy production has yet succeeded, apart from nuclear weapons with the H-bomb, since this application does not aims at containing and controlling the reaction produced. There are, however, some other less mediated uses, such as neutron generators. The fusion of light nuclei releases enormous amounts of energy from the attraction between the nucleons due to the strong interaction (nuclear binding energy). Fusion it is with nuclear fission one of the two main types of nuclear reactions applied. The mass of the new atom obtained by the fusion is less than the sum of the masses of the two light atoms. In the process of fusion, part of the mass is transformed into energy in its simplest form: heat. This loss is explained by the Einstein known formula E=mc2. Unlike nuclear fission, the fusion products themselves (mainly helium 4) are not radioactive, but when the reaction is used to emit fast neutrons, they can transform the nuclei that capture them into isotopes that some of them can be radioactive. In order to be able to start and to be maintained with the success the nuclear fusion reactions, it is first necessary to know all this reactions very well. This means that it is necessary to know both the main reactions that may take place in a nuclear reactor and their sense and effects. The main aim is to choose and coupling the most convenient reactions, forcing by technical means for their production in the reactor. Taking into account that there are a multitude of possible variants, it is necessary to consider in advance the solutions that we consider them optimal. The paper takes into account both variants of nuclear fusion, and cold and hot. For each variant will be mentioned the minimum necessary specifications.
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37

Jin, Shilun. "Nuclear Reaction Sensitivity in Magnetohydrodynamically Driven Supernovae." Astrophysical Journal 927, no. 1 (March 1, 2022): 116. http://dx.doi.org/10.3847/1538-4357/ac4f4a.

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Abstract The weak r-process offers an explanation of the formation of lighter heavy elements 36 ≤ Z ≤ 47 in ultra-metal-poor stars. Magnetohydrodynamically driven supernovae are thought to be a robust astronomical site of the weak r-process and recently gave a good description of the observational abundance pattern of an extremely metal-poor star. However, the characteristics of nuclear reactions in the MHD nucleosynthesis are not as clear as in another site, that of core-collapse supernovae. In this paper, the trajectories of the MHD model are implemented into SkyNet network calculations. By varying the reaction rates of each type, the (α,n) reactions are much more active than other types of reactions, such as (n,γ), (p,γ), (n,p), and (α,p). A further detailed sensitivity study investigates the (α,n) reactions and lists the most influential ones over the whole range, and the impactful reactions on each element from Sr to Ag are tabulated.
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38

Escher, Jutta, Kirana Bergstrom, Emanuel Chimanski, Oliver Gorton, Eun Jin In, Michael Kruse, Sophie Péru, et al. "Improving nuclear data evaluations with predictive reaction theory and indirect measurements." EPJ Web of Conferences 284 (2023): 03012. http://dx.doi.org/10.1051/epjconf/202328403012.

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Nuclear reaction data required for astrophysics and applications is incomplete, as not all nuclear reactions can be measured or reliably predicted. Neutron-induced reactions involving unstable targets are particularly challenging, but often critical for simulations. In response to this need, indirect approaches, such as the surrogate reaction method, have been developed. Nuclear theory is key to extract reliable cross sections from such indirect measurements. We describe ongoing efforts to expand the theoretical capabilities that enable surrogate reaction measurements. We focus on microscopic predictions for charged-particle inelastic scattering, uncertainty-quantified optical nucleon-nucleus models, and neural-network enhanced parameter inference.
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39

Spatafora, A., L. Acosta, C. Agodi, P. Amador-Valenzuela, G. A. Brischetto, S. Calabrese, D. Calvo, et al. "Experimental and theoretical multi-channel study of direct nuclear reactions: a tool to provide data driven information on the 76Ge neutrino-less double-beta decay." Journal of Physics: Conference Series 2586, no. 1 (September 1, 2023): 012134. http://dx.doi.org/10.1088/1742-6596/2586/1/012134.

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Abstract The study of heavy-ions induced double charge-exchange (HI-DCE) nuclear reactions is a promising way to access data-driven information on neutrino-less double-beta decay nuclear matrix elements. In the following, particular attention is given to the (18O,18Ne) and (20Ne,20O) HI-DCE reactions as tools for β + β + and β − β − decays, respectively. The experiments are performed in Catania at the Laboratori Nazionali del Sud of the Istituto Nazionale di Fisica Nucleare (INFN-LNS). The MAGNEX magnetic spectrometer is used to momentum analyse the ejectiles of a large network of nuclear reactions. New preliminary experimental data for the 76Se(18O,18F)76As and 76Ge(20Ne,20F)76As single charge exchange (SCE) and for the 76Se(18O,18Ne)76Ge and 76Ge(20Ne,20O)76Se DCE nuclear reactions were also investigated.
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40

Ciraldo, Irene, F. Cappuzzello, M. Cavallaro, D. Carbone, S. Burrello, A. Spatafora, A. Gargano, et al. "Study of the one-neutron transfer reaction in 18O + 76Se collision at 275 MeV in the context of the NUMEN project." Journal of Physics: Conference Series 2453, no. 1 (March 1, 2023): 012013. http://dx.doi.org/10.1088/1742-6596/2453/1/012013.

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Abstract Heavy-ion one-nucleon transfer reactions are promising tools to investigate single-particle configurations in nuclear states, with and without the excitation of the core degrees of freedom. An accurate determination of the spectroscopic amplitudes of these configurations is essential for the study of other direct reactions as well as beta-decays. In this context, the 76Se(18O,17O)77Se one-neutron transfer reaction gives a quantitative access to the relevant single particle orbitals and core polarization transitions built on 76Se. This is particularly relevant, since it provides data-driven information to constrain nuclear structure models for the 76Se nucleus. The excitation energy spectrum and the differential cross section angular distributions of this nucleon transfer reaction was measured at 275 MeV incident energy for the first time using the MAGNEX large acceptance magnetic spectrometer. The data are compared with calculations based on distorted wave Born approximation and coupled channel Born approximation adopting spectroscopic amplitudes for the projectile and target overlaps derived by large-scale shell model calculations and interacting boson-fermion model. These reactions are studied in the frame of the NUMEN project. The NUMEN (NUclear Matrix Elements for Neutrinoless double beta decay) project was conceived at the Istituto Nazionale di Fisica Nucleare–Laboratori Nazionali del Sud (INFN-LNS) in Catania, Italy, aiming at accessing information about the nuclear matrix elements (NME) of neutrinoless double beta decay (0νββ) through the study of the heavy-ion induced double charge exchange (DCE) reactions on various 0νββ decay candidate targets. Among these, the 76Se nucleus is under investigation since it is the daughter nucleus of 76Ge in the 0νββ decay process.
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41

Yamaguchi, H., S. Hayakawa, N. R. Ma, H. Shimizu, K. Okawa, L. Yang, D. Kahl, et al. "Experimental studies on astrophysical reactions at the low-energy RI beam separator CRIB." EPJ Web of Conferences 260 (2022): 03003. http://dx.doi.org/10.1051/epjconf/202226003003.

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Experimental studies on astrophysical reactions involving radioactive isotopes (RI) often accompany technical challenges. Studies on such nuclear reactions have been conducted at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study, the University of Tokyo. We discuss two cases of astrophysical reaction studies at CRIB; one is for the 7Be+n reactions which may affect the primordial 7Li abundance in the Big-Bang nucleosynthesis, and the other is for the 22Mg(α, p) reaction relevantin X-raybursts.
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42

Nunes, F. M., G. Potel, T. Poxon-Pearson, and J. A. Cizewski. "Nuclear Reactions in Astrophysics: A Review of Useful Probes for Extracting Reaction Rates." Annual Review of Nuclear and Particle Science 70, no. 1 (October 19, 2020): 147–70. http://dx.doi.org/10.1146/annurev-nucl-020620-063734.

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Astrophysical simulations require knowledge of a wide array of reaction rates. For a number of reasons, many of these reaction rates cannot be measured directly and instead are probed with indirect nuclear reactions. We review the current state of the art regarding the techniques used to extract reaction information that is relevant to describe stars, including their explosions and collisions. We focus on the theoretical developments over the last decade that have had an impact on the connection between the laboratory indirect measurement and the astrophysical desired reaction. This review includes three major probes that have been, and will continue to be, widely used in our community: transfer reactions, breakup reactions, and charge-exchange reactions.
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43

Hodgson, P. E. "Multistep processes in nuclear reactions." Acta Physica Hungarica A) Heavy Ion Physics 2, no. 3-4 (October 1995): 175–97. http://dx.doi.org/10.1007/bf03055106.

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44

Gaal, J. C., and C. K. Pearson. "Eukaryotic nuclear ADP-ribosylation reactions." Biochemical Journal 230, no. 1 (August 15, 1985): 1–18. http://dx.doi.org/10.1042/bj2300001.

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45

Shyam, Radhey. "Nuclear reactions at intermediate energies." EPJ Web of Conferences 117 (2016): 02002. http://dx.doi.org/10.1051/epjconf/201611702002.

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46

Nishioka, Hidetoshi. "Statistical Theory of Nuclear Reactions." Progress of Theoretical Physics Supplement 116 (1994): 451–56. http://dx.doi.org/10.1143/ptps.116.451.

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47

Christie, Daniel J., and Linden Nelson. "Student reactions to nuclear education." Bulletin of the Atomic Scientists 44, no. 6 (July 1988): 22–23. http://dx.doi.org/10.1080/00963402.1988.11456178.

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48

Langanke, K., and M. Wiescher. "Nuclear reactions and stellar processes." Reports on Progress in Physics 64, no. 12 (November 8, 2001): 1657–701. http://dx.doi.org/10.1088/0034-4885/64/12/202.

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49

Briceño, Raúl A., Zohreh Davoudi, and Thomas C. Luu. "Nuclear reactions from lattice QCD." Journal of Physics G: Nuclear and Particle Physics 42, no. 2 (January 13, 2015): 023101. http://dx.doi.org/10.1088/0954-3899/42/2/023101.

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50

Bardayan, D. W. "Transfer reactions in nuclear astrophysics." Journal of Physics G: Nuclear and Particle Physics 43, no. 4 (February 22, 2016): 043001. http://dx.doi.org/10.1088/0954-3899/43/4/043001.

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