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Artykuły w czasopismach na temat „Low energy nuclear reactions”

Autor: Grafiati

Data publikacji: 3 czerwca 2025

Data aktualizacji: 31 lipca 2025

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1

Martel, Ismael. "Low energy reactions of halo nuclei." EPJ Web of Conferences 252 (2021): 04003. http://dx.doi.org/10.1051/epjconf/202125204003.

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Halo nuclei are extreme nuclear states consisting of one or more weakly-bound valence nucleons spatially decoupled from a tightly bound nuclear core. The weakly bound nature of the halo dominates the reaction probability, but the specific reaction mechanisms depend also on the core and target nuclei. Despite of the inherent complexity of the reaction process, simple two-body models and direct reaction theories can be used to extract useful information of the structure of the halo nucleus and its dynamics. These ideas are discussed using selected experiments of Coulomb barrier reactions with on

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2

Kasagi, Jirohta. "Low-Energy Nuclear Reactions in Metals." Progress of Theoretical Physics Supplement 154 (2004): 365–72. http://dx.doi.org/10.1143/ptps.154.365.

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3

Mayer, Frederick J. "Superconductivity and low-energy nuclear reactions." Results in Physics 12 (March 2019): 2075–77. http://dx.doi.org/10.1016/j.rinp.2019.02.027.

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4

Bencze, Gy, and C. Chandler. "Coulomb screening in low-energy nuclear reactions." Physical Review C 45, no. 2 (1992): 532–39. http://dx.doi.org/10.1103/physrevc.45.532.

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5

Bagulya, A. V., O. D. Dalkarov, M. A. Negodaev, and A. S. Rusetskii. "Low-energy nuclear reactions in crystal structures." Physics of Particles and Nuclei 48, no. 5 (2017): 691–97. http://dx.doi.org/10.1134/s1063779617050045.

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6

Mayer, Frederick J., and John R. Reitz. "On Very Low Energy Hydrogenic Nuclear Reactions." Fusion Technology 20, no. 3 (1991): 367–72. http://dx.doi.org/10.13182/fst91-a29680.

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7

Jarmie, Nelson, and Ronald E. Brown. "Low-Energy nuclear reactions with hydrogen isotopes." Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms 10-11 (May 1985): 405–10. http://dx.doi.org/10.1016/0168-583x(85)90279-4.

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8

Storms, Edmund. "Efforts to explain low-energy nuclear reactions." Naturwissenschaften 100, no. 11 (2013): 1103. http://dx.doi.org/10.1007/s00114-013-1101-y.

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9

Ideguchi, E. "Energy-degraded RI beam for low-energy nuclear reactions." Progress of Theoretical and Experimental Physics 2012, no. 1 (2012): 3C005–0. http://dx.doi.org/10.1093/ptep/pts040.

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10

Yamaguchi, H., S. Hayakawa, N. R. Ma, 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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11

Cavanna, Francesca. "Nuclear Astrophysics at the Low-Energy Frontiers: Updates from underground laboratories." EPJ Web of Conferences 290 (2023): 10005. http://dx.doi.org/10.1051/epjconf/202329010005.

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Nuclear fusion reactions are the heart of nuclear astrophysics: they sensitively influence the nucleosynthesis of the elements in the earliest stages of the Universe and in all the objects formed thereafter; control the associated energy generation and neutrino luminosity; influence the evolution of stars. Unfortunately, measuring reaction cross sections at astrophysically relevant energies is exceptionally challenging due to Coulomb repulsion between nuclei, resulting in cross section values as low as fbar. Laboratorial measurements of these cross sections are often unfeasible due to overwhel

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12

Dasso, C. H., and A. Vitturi. "Low-energy nuclear reactions with weakly-bound systems." Journal of Physics G: Nuclear and Particle Physics 31, no. 10 (2005): S1449—S1453. http://dx.doi.org/10.1088/0954-3899/31/10/012.

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13

Kim, Yeong E., Yong Joo Kim, Alexander L. Zubarev, and Jin-Hee Yoon. "Optical theorem formulation of low-energy nuclear reactions." Physical Review C 55, no. 2 (1997): 801–9. http://dx.doi.org/10.1103/physrevc.55.801.

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14

Ostrowski, A. N., A. C. Shotter, W. Bradfield-Smith, et al. "Low-energy radioactive ion beam induced nuclear reactions." Journal of Physics G: Nuclear and Particle Physics 24, no. 8 (1998): 1553–59. http://dx.doi.org/10.1088/0954-3899/24/8/033.

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15

Belyaev, V. B., S. A. Rakityansky, H. Fiedeldey, and S. A. Sofianos. "Low-energy nuclear transfer reactions in muonic molecules." Physical Review A 50, no. 1 (1994): 305–10. http://dx.doi.org/10.1103/physreva.50.305.

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16

Lombardo, I., L. Campajola, D. Dell'Aquila, et al. "Study of Nuclear Structure of13C and20Ne by Low Energy Nuclear Reactions." Journal of Physics: Conference Series 569 (December 8, 2014): 012068. http://dx.doi.org/10.1088/1742-6596/569/1/012068.

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17

Guimarães, Valdir. "Low-energy nuclear reactions with double-solenoid-based radioactive nuclear beam." Pramana 75, no. 1 (2010): 137–47. http://dx.doi.org/10.1007/s12043-010-0073-0.

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18

Vesić, Jelena. "Electron Screening in Laboratory Nuclear Reactions." Particles 7, no. 3 (2024): 834–55. http://dx.doi.org/10.3390/particles7030050.

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A thorough understanding of nuclear reaction rates at low energies is essential for improving our understanding of energy generation in stars and primordial and stellar nucleosynthesis. At low energies, fusion reactions between charged particles are strongly suppressed by the presence of the Coulomb barrier, which classically inhibits the penetration of one nucleus into another. The barrier penetration causes the cross section to have a steep energy dependence at low energies, making cross section measurements very challenging. Furthermore, little is known about the impact of surrounding elect

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19

Dubinko, Vladimir. "Radiation-induced catalysis of low energy nuclear reactions in solids." Journal of Micromechanics and Molecular Physics 01, no. 01 (2016): 1650006. http://dx.doi.org/10.1142/s2424913016500065.

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The Schwinger model of nuclear fusion extended with account of localized anharmonic vibrations (LAV) has been applied to the nuclear reaction presumably taking place in the metal hydrides/deuterides. LAV excited in NiH lattice can enhance the fusion rate by 25 orders of magnitude. New method of the low-temperature catalysis of low energy nuclear reactions (LENR) is proposed, which is based on the excitation of LAV in solids by Bremsstrahlung gamma and Characteristic X-rays produced by accelerated electrons hitting a metallic converter. The main advantage of the high-frequency electromagnetic i

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20

Nagel, David J., and Kamron C. Fazel. "Low Energy Nuclear Reactions: Exciting New Science and Potential Clean Energy." Fusion Science and Technology 61, no. 1T (2012): 463–68. http://dx.doi.org/10.13182/fst12-a13464.

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21

Yamaguchi, H., S. Hayakawa, N. R. Ma, et al. "RIB induced reactions: Studying astrophysical reactions with low-energy RI beam at CRIB." EPJ Web of Conferences 275 (2023): 01015. http://dx.doi.org/10.1051/epjconf/202327501015.

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Astrophysical reactions involving radioactive isotopes (RI) often play an important role in high-temperature stellar environments. The experimental studies on the reaction rates for those are still limited mainly due to the technical difficulties in producing high-quality RI beams. A direct measurement of those reactions would be still challenging in many cases, however, we can make a reliable evaluation of the reaction rates by an indirect method or by studying the resonance prorerties. Here we ntroduce recent examples of experimental studies on such RI-involving astrophysical reactions, perf

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22

TAKIGAWA, Noboru, and Sachie KIMURA. "Screening Effects in Low Energy Nuclear Reactions in Laboratories." Journal of Plasma and Fusion Research 79, no. 9 (2003): 891–96. http://dx.doi.org/10.1585/jspf.79.891.

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23

KASAGI, JIROTA. "Anomalous Nuclear Reactions Observed in Low-energy Deuteron Bombardment." RADIOISOTOPES 46, no. 8 (1997): 600–602. http://dx.doi.org/10.3769/radioisotopes.46.600.

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24

collaboration, D. J. Dean for the NSLER. "The nuclear structure and low-energy reactions (NSLER) collaboration." Journal of Physics: Conference Series 46 (September 1, 2006): 166–70. http://dx.doi.org/10.1088/1742-6596/46/1/024.

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25

Lombardo, I., D. Dell'Aquila, and M. Vigilante. "Spectroscopy of Light Nuclei with Low Energy Nuclear Reactions." Journal of Physics: Conference Series 730 (July 2016): 012016. http://dx.doi.org/10.1088/1742-6596/730/1/012016.

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26

Srivastava, Y. N., A. Widom, and L. Larsen. "A primer for electroweak induced low-energy nuclear reactions." Pramana 75, no. 4 (2010): 617–37. http://dx.doi.org/10.1007/s12043-010-0143-3.

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27

Pitard, Francis. "The Theory of Vacuoles and Low-energy Nuclear Reactions." TOS Forum 2020, no. 10 (2020): 46. http://dx.doi.org/10.1255/tosf.127.

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A new version of Francis Pitard’s book, The Theory of Vacuoles and Low-energy Nuclear Reactions: A Correct System of Dimensions and Units has just been announced, and is available from the author’s website: http://www.fpscsampling.com/publicationsnewsletter/books/. TOS Forum is glad to make its readers aware of this publication which takes us all into a very interesting place inside elementary particles, which on closer contemplation are claimed not to exist. What in the world of Physics is going on?

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28

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 (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 accelerati

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29

Stavek, Jiří. "Towards Reconciliation and Collaboration: Bridging Low Energy Nuclear Reactions and Mainstream Nuclear Physics." European Journal of Applied Physics 7, no. 2 (2025): 61–67. https://doi.org/10.24018/ejphysics.2025.7.2.377.

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Low Energy Nuclear Reactions (LENR), often associated with the controversial history of “cold fusion,” have persisted as a topic of scientific interest for over three decades, despite limited acceptance in mainstream nuclear physics. While the LENR community has documented anomalous thermal effects and transmutation phenomena in metal-hydrogen systems, these results remain underexplored by conventional nuclear theory and experimental frameworks. This paper proposes a constructive path forward: a call for interdisciplinary collaboration between LENR researchers and mainstream nuclear physicists

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30

BARU, VADIM. "πNN SYSTEM AT LOW ENERGY". International Journal of Modern Physics A 26, № 03n04 (2011): 586–88. http://dx.doi.org/10.1142/s0217751x11052116.

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With the advent of chiral perturbation theory, the low-energy effective field theory of QCD, high accuracy calculations for hadronic reactions have become possible. We review the recent developments in the reaction NN → NNπ in chiral EFT.

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31

Yamaguchi, H., S. Hayakawa, L. Yang, H. Shimizu, and D. Kahl. "Direct measurements and detection techniques with low-energy RIBs." EPJ Web of Conferences 184 (2018): 01017. http://dx.doi.org/10.1051/epjconf/201818401017.

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Astrophysical reactions involving radioactive isotopes (RI) are of importance for the stellar energy generation and nucleosynthesis especially in high-temperature astrophysical sites, such as X-ray bursts, core-collapse supernovae, and supermassive metalpoor stars. In spite of the essential diffculties in the experimental evaluation of those reaction rates, there are several successful approaches to study them, owing to the recent technical developments in the beam production, measurement method, and detectors. Among them, the measurements of α resonant scattering and (α, p) reactions using th

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32

DESCOUVEMONT, PIERRE. "CROSS SECTIONS FOR NUCLEAR ASTROPHYSICS." International Journal of Modern Physics E 17, no. 10 (2008): 2165–70. http://dx.doi.org/10.1142/s0218301308011288.

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General properties of low-energy cross sections and of reaction rates are presented. We describe different models used in nuclear astrophysics: microscopic models, the potential model, and the R-matrix method. Two important reactions, 7 Be ( p ,γ)8 B and 12 C (α,γ)16 O , are then briefly discussed.

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33

Samarin, Vyacheslav Vladimirovich. "Mathematical modeling of dinuclear systems in low energy nuclear reactions." Computer Research and Modeling 2, no. 4 (2010): 385–92. http://dx.doi.org/10.20537/2076-7633-2010-2-4-385-392.

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34

Vysotskii, Vladimir I., and Mikhail V. Vysotskyy. "UNIVERSAL MECHANISM OF REALIZATION OF NUCLEAR REACTIONS AT LOW ENERGY." Radioelectronics. Nanosystems. Information Technologies 9, no. 1 (2017): 21–36. http://dx.doi.org/10.17725/rensit.2017.09.021.

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35

Warner, Robert E. "Nuclear and Coulomb contributions to6,8He+Sidissociation reactions at low energy." Physical Review C 55, no. 1 (1997): 298–301. http://dx.doi.org/10.1103/physrevc.55.298.

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36

Nor Azman, Muhammad ‘Adli, Nur Syazwani Mohd Ali, Muhammad Syahir Sarkawi, Muhammad Arif Sazali, and Nor Afifah Basri. "Nuclear fuel materials and its sustainability for low carbon energy system: A review." IOP Conference Series: Materials Science and Engineering 1231, no. 1 (2022): 012016. http://dx.doi.org/10.1088/1757-899x/1231/1/012016.

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Abstract World energy generation for electricity is still dependent on fossil fuels since it is more reliable and secure than the current intermittent renewable energy systems. Although the integration of renewable energy as an energy mix is in progress, still it could not be able to replace fossil fuels. Dependency on fossil fuels will not only contribute to severe climate change but will also degrade future generation quality of life. Hence, the solution to quandary is by integrating nuclear power plants with those of renewable energy such as solar and wind to meet the energy demand and to e

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37

Morales-Gallegos, Lizeth, Marialuisa Aliotta, Andreas Best, et al. "¹²C+¹²C reactions for Nuclear Astrophysics." EPJ Web of Conferences 279 (2023): 11005. http://dx.doi.org/10.1051/epjconf/202327911005.

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12C fusion reactions are among the most important in stellar evolution since they determine the destiny of massive stars. Over the past fifty years, massive efforts have been done to measure these reactions at low energies. However, existing data present several discrepancies between sets and large uncertainties specially at the lowest energies. Factors such as beam/environmental backgrounds, extremely low cross sections and insufficient knowledge of the reaction mechanism contribute to these problems. Recently, the ERNA collaboration measured the 12C+12C reactions at Ec.m. = 2.51 - 4.36 MeV w

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38

La Cognata, Marco. "Using indirect methods to explore low-energy fusion cross sections in nuclear astrophysics." EPJ Web of Conferences 301 (2024): 02006. http://dx.doi.org/10.1051/epjconf/202430102006.

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Nuclear reactions within stellar environments typically manifest at energies well below 1 MeV. As a consequence, the Coulomb barrier strongly suppresses the cross section, diminishing it to values as minute as a few nanobarns for charged particles. This challenge in obtaining precise input data for astrophysics has prompted the utilization of indirect methodologies. Specifically, approaches such as ANC and THM have been employed to ascertain cross sections for reactions involving photons and charged particles in the exit channel, respectively, obviating the necessity for extrapolation. The dis

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39

Liu, Bing, Rui-zhi Yang, and Felix Aharonian. "Nuclear de-excitation lines as a probe of low-energy cosmic rays." Astronomy & Astrophysics 646 (February 2021): A149. http://dx.doi.org/10.1051/0004-6361/202039977.

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Low-energy cosmic rays (LECRs) contribute substantially to the energy balance of the interstellar medium. They play also significant role in the heating and chemistry of gas, and, consequently, on the star formation process. Because of the slow propagation coupled with enhanced energy losses of subrelativistic particles, LECRs are concentrated around their acceleration sites. LECRs effectively interact with the ambient gas through nuclear reactions. Although these processes are energetically less effective compared to heating and ionization, they are extremely important from the point of view

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40

Li, Xian. "The entropy of the Au + Au system in low energy nuclear reaction." Modern Physics Letters A 33, no. 33 (2018): 1850191. http://dx.doi.org/10.1142/s0217732318501912.

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Considering the boundary effect, we adopt the Tsallis entropy and compute the time evolution of the entropy in low energy reaction system for the first time, dealing with the initial, compression, expansion and fission stages with a consistent method. We find that it rises up in the compression period and reduces slightly after separation, because of the energy exchange between the collective motion and the internal excitation. The research shows that the entropy curves in binary, sequential or direct ternary fissions are distinct, which declares that the entropy may be a novel criterion to st

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41

Yamaguchi, H., S. Hayakawa, H. Shimizu, et al. "Nuclear Astrophysics with Exotic Beam; Thick-target Measurements at CRIB." EPJ Web of Conferences 297 (2024): 01017. http://dx.doi.org/10.1051/epjconf/202429701017.

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Astrophysical reactions involving radioactive isotopes (RI) often play an important role in high-temperature stellar environments. The experimental information on those reactions is still limited mainly due to the technical difficulties in producing high-quality and intense RI beams. Although a direct measurement of those reactions at astrophysical energy would be still challenging, we may take several alternative approaches to determine the reaction rates, by applying other mesurement methods or improving the target and detectors. Here we mainly discuss the thick-target method in inverse kine

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42

Kuchiev, M. Yu, B. L. Altshuler, and V. V. Flambaum. "Low-energy nuclear reactions boosted by collisions with environment (Carambole collisions)." Journal of Physics G: Nuclear and Particle Physics 28, no. 1 (2001): 47–65. http://dx.doi.org/10.1088/0954-3899/28/1/304.

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43

Kimura, Sachie, Noboru Takigawa, Masanori Abe, D. M. Brink, and A. Bonasera. "Influence of Tunneling on Electron Screening in Low Energy Nuclear Reactions." Progress of Theoretical Physics Supplement 154 (2004): 317–24. http://dx.doi.org/10.1143/ptps.154.317.

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44

Kawano, T., and P. Talou. "Numerical Simulations for Low Energy Nuclear Reactions to Validate Statistical Models." Nuclear Data Sheets 118 (April 2014): 183–86. http://dx.doi.org/10.1016/j.nds.2014.04.032.

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45

Osman, F., H. Hora, X. Z. Li, G. H. Miley, and J. C. Kelly. "Supporting the Josephson Interpretation of Low Energy Nuclear Reactions and Stabilization of Nuclear Waste." American Journal of Applied Sciences 2, no. 6 (2005): 1049–57. http://dx.doi.org/10.3844/ajassp.2005.1049.1057.

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46

Kim, Y. E., and A. L. Zubarev. "Optical theorem and effective finite-range nuclear interaction for low-energy nuclear-fusion reactions." Il Nuovo Cimento A 109, no. 12 (1996): 1721. http://dx.doi.org/10.1007/bf02773552.

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47

Kim, Y. E., and A. L. Zubarev. "Optical theorem and effective finite-range nuclear interaction for low-energy nuclear-fusion reactions." Il Nuovo Cimento A 108, no. 8 (1995): 1009–25. http://dx.doi.org/10.1007/bf02730852.

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48

YUSOF, NORHASLIZA, and HASAN ABU KASSIM. "MOST EFFECTIVE ENERGY IN THERMONUCLEAR REACTIONS OF SOME LIGHT NUCLEI." Modern Physics Letters A 24, no. 11n13 (2009): 1071–75. http://dx.doi.org/10.1142/s0217732309000620.

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Gamow peak describes the most effective energy E0 for a nonresonant nuclear reaction to occur. At astrophysical low energies much lower than the Coulomb barrier, the ability of the interacting nuclei to tunnel through the barrier depends on the primitive probability which is proportional to the Gamow factor. The reaction rate will then be determined by the primitive tunneling probability and the astrophysical S-factor. In the literature, tables on the thermonuclear reaction rates are compiled for many reactions of interest in astrophysics by using this low energy approximation. In this paper,

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49

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 d

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50

Kokkoris, M. "Evaluation of differential cross-sections for light element reactions at low energies using R-matrix calculations: The case of 12C." HNPS Proceedings 19 (January 1, 2020): 151. http://dx.doi.org/10.12681/hnps.2527.

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The theoretical evaluation of diÆerential cross-section values for low-energy re- actions of light elements is of great importance in the fields of IBA (Ion Beam Analysis) and nuclear astrophysics. R-matrix theory is generally accepted as the most appropriate one for the analysis of resonance reactions in low-energy nuclear physics. In this approach, the configuration space of the scattering problem is divided into an internal region, corresponding to the compound nucleus, where the total wave function can be expanded into a complete set of eigenstates (in terms of unknown base functions, with

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