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Journal articles on the topic 'Light neutron-rich nuclei'

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Author: Grafiati

Published: 9 March 2023

Last updated: 10 March 2023

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1

Bang, J. M., F. A. Gareev, G. S. Kazacha, and A. M. Kalinin. "Neutron-rich light nuclei." Physica Scripta 41, no. 2 (February 1, 1990): 202–6. http://dx.doi.org/10.1088/0031-8949/41/2/003.

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2

Jelavić Malenica, D., M. Milin, A. Di Pietro, P. Figuera, M. Lattuada, D. Miljanić, A. Musumarra, et al. "Clusters in neutron-rich light nuclei." EPJ Web of Conferences 117 (2016): 07007. http://dx.doi.org/10.1051/epjconf/201611707007.

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3

HAGINO, K., H. SAGAWA, and P. SCHUCK. "DI-NEUTRON CORRELATION IN LIGHT NEUTRON-RICH NUCLEI." International Journal of Modern Physics E 18, no. 10 (November 2009): 2045–49. http://dx.doi.org/10.1142/s0218301309014263.

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Using a three-body model with density-dependent contact interaction, we discuss the root mean square distance between the two valence neutrons in 11 Li nuclues as a function of the center of mass of the neutrons relative to the core nucleus 9 Li . We show that the mean distance takes a pronounced minimum around the surface of the nucleus, indicating a strong surface di-neutron correlation. We demonstrate that the pairing correlation plays an essential role in this behavior. We also discuss the di-neutron structure in the 8 He nucleus.

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4

Torilov, S. Yu, K. A. Gridnev, and T. V. Korovitskaya. "Rotational bands in light neutron-rich nuclei." Bulletin of the Russian Academy of Sciences: Physics 76, no. 8 (August 2012): 854–56. http://dx.doi.org/10.3103/s1062873812080278.

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5

Sagawa, Hiroyuki, and C. A. Bertulani. "Multipole Excitations in Light Neutron-Rich Nuclei." Progress of Theoretical Physics Supplement 124 (1996): 143–53. http://dx.doi.org/10.1143/ptps.124.143.

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6

He, Chao, Hui Hua, Xiangqing Li, and Bo Wang. "β-Decay of Light Neutron-Rich Nuclei." Plasma Science and Technology 14, no. 7 (July 2012): 610–13. http://dx.doi.org/10.1088/1009-0630/14/7/10.

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7

Kanada-En'yo, Y., Y. Taniguchi, and M. Kimura. "Cluster structure in light neutron-rich nuclei." Journal of Physics: Conference Series 111 (May 1, 2008): 012002. http://dx.doi.org/10.1088/1742-6596/111/1/012002.

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8

Bohlen, H. G., W. von Oertzen, R. Kalpakchieva, T. N. Massey, T. Dorsch, M. Milin, C. Schulz, T. Kokalova, and C. Wheldon. "Band structures in light neutron-rich nuclei." Journal of Physics: Conference Series 111 (May 1, 2008): 012021. http://dx.doi.org/10.1088/1742-6596/111/1/012021.

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9

Hoshino, T., H. Sagawa, and A. Arima. "Giant resonances of light neutron-rich nuclei." Nuclear Physics A 523, no. 2 (February 1991): 228–46. http://dx.doi.org/10.1016/0375-9474(91)90002-n.

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10

Korsheninnikov, A. A., D. V. Aleksandrov, N. Aoi, Y. Doki, N. Inabe, M. Fujimaki, T. Kobayashi, et al. "Experimental studies of light neutron rich nuclei." Nuclear Physics A 588, no. 1 (May 1995): c23—c28. http://dx.doi.org/10.1016/0375-9474(95)00094-h.

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11

Ishihara, M. "Current topics on light neutron-rich nuclei." Nuclear Physics A 588, no. 1 (May 1995): c49—c58. http://dx.doi.org/10.1016/0375-9474(95)00098-l.

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12

Penionzhkevich, Yu E. "Synthesis reactions of neutron-rich isotopes of light elements." Eurasian Journal of Physics and Functional Materials 5, no. 2 (June 22, 2021): 70–87. http://dx.doi.org/10.32523/ejpfm.2021050201.

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One of the most complicated problems of experimental nuclear physics is the synthesis of exotic nuclei near the boundaries of stability. These nuclei, as a rule, are 10 or more neutrons away from stable nuclei, have a short lifetime (less than 1 ms) and low binding energy. All this determines special requirements to the choice of reactions for the synthesis of such nuclei and the method of their transportation and registration. Mainly, for the synthesis of exotic nuclei, reactions of fragmentation of the bombarding heavy ion, direct reactions of the types (p, d) , (d, p) , (d, n) , ( d , 3 He), etc., as well as reactions of fission and deep inelastic transfer are used.

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13

Sagawa, H., and H. Toki. "Hartree-Fock calculations of light neutron-rich nuclei." Journal of Physics G: Nuclear Physics 13, no. 4 (April 1987): 453–61. http://dx.doi.org/10.1088/0305-4616/13/4/008.

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14

Orr, N. A. "Haloes and clustering in light, neutron-rich nuclei." European Physical Journal A 15, no. 1-2 (September 2002): 109–13. http://dx.doi.org/10.1140/epja/i2001-10236-6.

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15

Itagaki, Naoyuki, Shigeto Okabe, and Kiyomi Ikeda. "Molecular-Orbital Structure in Light Neutron-Rich Nuclei." Progress of Theoretical Physics Supplement 142 (2001): 297–323. http://dx.doi.org/10.1143/ptps.142.297.

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16

Cortina-Gil, M. D., P. Roussel-Chomaz, N. Alamanos, J. Barrette, W. Mittig, F. S. Dietrich, F. Auger, et al. "Proton elastic scattering on light neutron-rich nuclei." Physics Letters B 401, no. 1-2 (May 1997): 9–14. http://dx.doi.org/10.1016/s0370-2693(97)00321-3.

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17

Itagaki, N., K. Hagino, T. Otsuka, S. Okabe, and K. Ikeda. "Importance of clustering in light neutron-rich nuclei." Nuclear Physics A 719 (May 2003): C205—C208. http://dx.doi.org/10.1016/s0375-9474(03)00918-7.

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18

Itagaki, N., S. Aoyama, T. Otsuka, T. Yoshida, S. Okabe, and K. Ikeda. "Exotic cluster structure in light neutron-rich nuclei." Nuclear Physics A 738 (June 2004): 17–23. http://dx.doi.org/10.1016/j.nuclphysa.2004.04.006.

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19

Itagaki, N., T. Otsuka, S. Okabe, and al et. "Exotic Cluster Structure in Light Neutron-Rich Nuclei." Acta Physica Hungarica A) Heavy Ion Physics 18, no. 2-4 (November 1, 2003): 173–78. http://dx.doi.org/10.1556/aph.18.2003.2-4.9.

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20

Hoshino, T., H. Sagawa, and A. Arima. "Shell-model study of light neutron-rich nuclei." Nuclear Physics A 506, no. 2 (January 1990): 271–92. http://dx.doi.org/10.1016/0375-9474(90)90387-2.

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21

DLOUHÝ, ZDENĚK. "STRUCTURE OF THE DRIP LINE NUCLEI PROBED BY SEPARATION ENERGIES." International Journal of Modern Physics E 15, no. 07 (October 2006): 1471–75. http://dx.doi.org/10.1142/s0218301306005071.

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The derivation of two-neutron separation energies from the direct mass measurement of the neutron-rich nuclei at GANIL has enabled us to establish new neutron magic numbers N=6 and 16 in neutron-rich region for the first time instead of normal 8 and 20 and to confirm the existence of new doubly magic nuclei 8 He and 24 O . Adjunction of a proton to the new doubly magic nuclei 8 He and 24 O enable to accept two or more neutrons by these nuclei and form, respectively, the neutron halo 11 Li nucleus and create a very neutron-rich set of 27,29,31 F isotopes. The connection between doubly magic nuclei and the neutron halo and/or very neutron-rich odd-Z nuclei is studied by analysis of triton separation energies St of light neutron-rich nuclei.

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22

KOHAMA, AKIHISA, BADAWY ABU-IBRAHIM, WATARU HORIUCHI, SHOHEI IWASAKI, and YASUYUKI SUZUKI. "TOTAL REACTION CROSS SECTIONS OF LIGHT NEUTRON-RICH NUCLEI IN THE GLAUBER APPROXIMATION." Modern Physics Letters A 25, no. 21n23 (July 30, 2010): 1963–66. http://dx.doi.org/10.1142/s0217732310000757.

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We report our recent numerical results of total reaction cross sections of light neutron-rich nuclei, such as carbons and oxygens, in the Glauber approximation to study the exotic structure of neutron-rich unstable nuclei.

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23

Dlouhý, Z., J. C. Angéligue, R. Anne, G. Auger, F. Azaiez, D. Baiborodin, C. Borcea, et al. "Changes in neutron shell closures of light very neutron-rich nuclei." Czechoslovak Journal of Physics 51, S1 (January 2001): A245—A253. http://dx.doi.org/10.1007/s10582-001-0030-8.

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24

Ren, Z., B. Chen, Z. Ma, and W. Mittig. "Relativistic mean-field study of light neutron-rich nuclei." Journal of Physics G: Nuclear and Particle Physics 21, no. 9 (September 1, 1995): 1269–72. http://dx.doi.org/10.1088/0954-3899/21/9/012.

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25

Singh, P., R. Kumar, and R. Kharab. "Coulomb breakup of neutron-rich isotopes of light nuclei." Physics of Atomic Nuclei 71, no. 11 (November 2008): 1932–39. http://dx.doi.org/10.1134/s1063778808110100.

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26

Gornov, M. G., Yu B. Gurov, P. V. Morokhov, S. V. Lapushkin, V. A. Pechkurov, B. A. Chernyshev, V. G. Sandukovsky, and E. A. Pasyuk. "Multilayer semiconductor spectrometer for studying light neutron-rich nuclei." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 446, no. 3 (May 2000): 461–68. http://dx.doi.org/10.1016/s0168-9002(99)00921-3.

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27

Penionzhkevich, Yu E., R. Kalpakchieva, and S. M. Lukyanov. "Particle stability of very neutron-rich very light nuclei." Nuclear Physics A 722 (July 2003): C170—C175. http://dx.doi.org/10.1016/s0375-9474(03)01354-x.

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28

Pramanik, U. Datta, T. Aumann, D. Cortina, H. Emling, H. Geissel, M. Hellström, R. Holzmann, et al. "Structure of light neutron-rich nuclei through coulomb dissociation." Pramana 57, no. 2-3 (August 2001): 535–44. http://dx.doi.org/10.1007/s12043-001-0060-6.

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29

Marqués, F. M. "Probing Few-Body Correlations in Light, Neutron-Rich Nuclei." Few-Body Systems 31, no. 2-4 (May 1, 2002): 145–50. http://dx.doi.org/10.1007/s006010200013.

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30

Horiuchi, H., and Y. Kanada-En'yo. "Light neutron-rich nuclei studied with antisymmetrized molecular dynamics." Nuclear Physics A 588, no. 1 (May 1995): c121—c127. http://dx.doi.org/10.1016/0375-9474(95)00110-m.

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31

Wuosmaa, A. H. "Structure of Light Neutron-rich Nuclei Studied with Transfer Reactions." Acta Physica Polonica B 46, no. 3 (2015): 627. http://dx.doi.org/10.5506/aphyspolb.46.627.

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32

Elekes, Z., Zs Dombrádi, N. Aoi, H. Baba, S. Bishop, K. Demichi, Zs Fülöp, et al. "The study of shell closures in light neutron-rich nuclei." Journal of Physics G: Nuclear and Particle Physics 35, no. 1 (December 13, 2007): 014038. http://dx.doi.org/10.1088/0954-3899/35/1/014038.

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33

Yan-Qing, Guo, and Ren Zhong-Zhou. "Structures of Light Neutron-Rich Nuclei with Orbit–Orbit Coupling." Chinese Physics Letters 24, no. 3 (February 19, 2007): 652–55. http://dx.doi.org/10.1088/0256-307x/24/3/018.

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34

Vieira, D. J., J. M. Wouters, K. Vaziri, R. H. Kraus, H. Wollnik, G. W. Butler, F. K. Wohn, and A. H. Wapstra. "Direct mass measurements of neutron-rich light nuclei nearN=20." Physical Review Letters 57, no. 26 (December 29, 1986): 3253–56. http://dx.doi.org/10.1103/physrevlett.57.3253.

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35

Datta Pramanik, U., T. Aumann, K. Boretzky, D. Cortina, Th W. Elze, H. Emling, H. Geissel, et al. "Studies of light neutron-rich nuclei near the drip line." European Physical Journal A 25, S1 (August 4, 2005): 339–41. http://dx.doi.org/10.1140/epjad/i2005-06-173-2.

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36

Kanada-En'yo, Yoshiko. "Molecular Structure with Exotic Clusters in Light Neutron-Rich Nuclei." Progress of Theoretical Physics Supplement 146 (2002): 190–200. http://dx.doi.org/10.1143/ptps.146.190.

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37

Lu, Z. T., P. Mueller, G. W. F. Drake, W. Nörtershäuser, Steven C. Pieper, and Z. C. Yan. "Colloquium: Laser probing of neutron-rich nuclei in light atoms." Reviews of Modern Physics 85, no. 4 (October 2, 2013): 1383–400. http://dx.doi.org/10.1103/revmodphys.85.1383.

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38

Filippov, G. F., and Yu A. Lashko. "Coexistence of different cluster configurations in light neutron-rich nuclei." Physics of Atomic Nuclei 70, no. 8 (August 2007): 1429–34. http://dx.doi.org/10.1134/s1063778807080170.

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39

Lashko, Yu A., and G. F. Filippov. "Multichannel nuclear reactions involving light neutron-rich nuclei: Microscopic approach." Physics of Atomic Nuclei 70, no. 8 (August 2007): 1440–44. http://dx.doi.org/10.1134/s1063778807080194.

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40

Chulkov, L. V., O. V. Bochkarev, D. Cortina-Gil, H. Geissel, M. Hellström, M. Ivanov, R. Janik, et al. "Total charge-changing cross sections for neutron-rich light nuclei." Nuclear Physics A 674, no. 3-4 (July 2000): 330–42. http://dx.doi.org/10.1016/s0375-9474(00)00168-8.

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41

Ibraeva, E. T., A. V. Dzhazairov-Kahramanov, and O. Imambekov. "Rescattering effects in proton interaction with light neutron rich nuclei." Nuclear Physics A 915 (October 2013): 142–57. http://dx.doi.org/10.1016/j.nuclphysa.2013.07.006.

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42

Bao, Xiaojun. "Production of light neutron-rich nuclei in multinucleon transfer reactions." Nuclear Physics A 986 (June 2019): 60–74. http://dx.doi.org/10.1016/j.nuclphysa.2019.02.009.

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43

Belozyorov, A. V., J. Vincour, Š. Piskoř, R. Kalpakchieva, Yu E. Penionzhkevich, V. S. Salamatin, and V. E. Zhuchko. "A facility for the study of neutron-rich light nuclei." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 411, no. 2-3 (July 1998): 343–50. http://dx.doi.org/10.1016/s0168-9002(98)00357-x.

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44

Oertzen, W. von. "Dimers and polymers in extremely deformed neutron-rich light nuclei." Il Nuovo Cimento A 110, no. 9-10 (September 1997): 895–906. http://dx.doi.org/10.1007/bf03035924.

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45

Kitagawa, H., and H. Sagawa. "Isospin dependence of kinetic energies in light neutron-rich nuclei." Hyperfine Interactions 78, no. 1-4 (1993): 179–83. http://dx.doi.org/10.1007/bf00568136.

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46

Hisashi, Kitagawa, and Sagawa Hiroyuki. "Isospin dependence of kinetic energies in light neutron-rich nuclei." Nuclear Physics A 551, no. 1 (January 1993): 16–34. http://dx.doi.org/10.1016/0375-9474(93)90300-m.

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47

Bohlen, H. G., B. Gebauer, Th Kirchner, M. von Lucke-Petsch, W. von Oertzen, A. N. Ostrowski, Ch Seyfert, et al. "Study of light neutron-rich nuclei with 14C-induced reactions." Nuclear Physics A 583 (February 1995): 775–82. http://dx.doi.org/10.1016/0375-9474(94)00757-e.

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48

Sakai, H., S. Ishida, and H. Okamura. "Spinflip Dipole Giant Resonances in neutron rich light nuclei and neutron halo effects." Nuclear Physics A 569, no. 1-2 (March 1994): 277–85. http://dx.doi.org/10.1016/0375-9474(94)90118-x.

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49

Xu, Yong-Li, Hai-Rui Guo, Yin-Lu Han, and Qing-Biao Shen. "The neutron microscopic optical potential based on skyrme interaction." International Journal of Modern Physics E 25, no. 02 (February 2016): 1650013. http://dx.doi.org/10.1142/s0218301316500130.

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The neutron microscopic optical potential (MOP) based on Skyrme interaction has been achieved by the Green function method in the nuclear matter, and given by the local density approximation (LDA) for finite nuclei. The total cross-sections, nonelastic cross-sections, elastic scattering angular distributions and analyzing powers are predicted for some light nuclei and actinide nuclei below 100[Formula: see text]MeV by the obtained neutron MOP with the Skyrme interaction SkC. These data are also predicted for targets in the mass range of [Formula: see text] which are too deformed and have rich nuclear structure properties. All of the theoretical results give reasonable agreements with the corresponding experimental data.

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50

PÉREZ-GARCÍA, M. ÁNGELES. "CHARGE DISTRIBUTION AND RADII IN CLUSTERS FROM NUCLEAR PASTA MODELS." International Journal of Modern Physics E 19, no. 07 (July 2010): 1477–89. http://dx.doi.org/10.1142/s0218301310015886.

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We study the consistency of the description of charge distributions and radii of nuclear clusters obtained with semiclassical nuclear pasta models. These nuclei are expected to exist in the low density outer crust of neutron stars. Properties of the arising clusterized nucleon matter can be compared to realistic nuclear properties as experimentally extracted on earth. We focus on non iso-symmetric light clusters with nucleon number 8 ≤ A ≤ 30 and use Monte Carlo many-body techniques. We simulate isotopic chains for a set of selected nuclei using a model Hamiltonian consisting of the usual kinetic term, hadronic nucleon nucleon (NN), Coulomb and an effective density dependent Pauli potential. It is shown that for neutron rich (deficient) clusters neutron (proton) skins develop. Different (matter, neutron, proton, electric charge) radii are computed for this set of non iso-symmetric nuclei. Nuclear binding energies are also analyzed in the isotopic chains.

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