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Journal articles on the topic 'Halo nuclei'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Austin, Sam M., and George F. Bertsch. "Halo Nuclei." Scientific American 272, no. 6 (1995): 90–95. http://dx.doi.org/10.1038/scientificamerican0695-90.

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2

Jonson, B. "Halo nuclei." Nuclear Physics A 574, no. 1-2 (1994): 151–66. http://dx.doi.org/10.1016/0375-9474(94)90043-4.

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3

Tanihata, Isao. "Neutron halo nuclei." Journal of Physics G: Nuclear and Particle Physics 22, no. 2 (1996): 157–98. http://dx.doi.org/10.1088/0954-3899/22/2/004.

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4

Vaagen, J. S., D. K. Gridnev, H. Heiberg-Andersen, et al. "Borromean Halo Nuclei." Physica Scripta T88, no. 1 (2000): 209. http://dx.doi.org/10.1238/physica.topical.088a00209.

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5

R.K. Biju, K. Prathapan, and K.P. Anjali. "Theoretical Study on the Formation of 1-neutron and 2-neutron Halo Nuclei via Decay of Elements in Super-Heavy Region." Journal of Nuclear Physics, Material Sciences, Radiation and Applications 8, no. 1 (2020): 11–24. http://dx.doi.org/10.15415/jnp.2020.81003.

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The possibility for the existence of 1-neutron and 2-neutron halo nuclei through the decay of even-even nuclei 270-316116, 272-318118 and 278-320120 in the super-heavy region is studied within the frame work of the Coulomb and Proximity Potential Model (CPPM). Halo structure in neutron rich nuclei with Z<=20 is identified by calculating the neutron separation energies and on the basis of potential energy considerations. The 1n + core configuration of proposed 1-neutron halo nuclei between z=10 and Z=20 is found shifted to 2n + core configuration in higher angular momentum states. The calcul

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6

Izosimov, I. N. "Isospin in halo nuclei: Borromean halo, tango halo, and halo isomers." Physics of Atomic Nuclei 80, no. 5 (2017): 867–76. http://dx.doi.org/10.1134/s1063778817050118.

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7

Prathapan, K., M. K. Preethi Rajan, and R. K. Biju. "Study on the decay of Z = 127 – 132 superheavy nuclei via emission of 1-n and 2-n halo nuclei." Nuclear Physics and Atomic Energy 24, no. 4 (2023): 324–35. http://dx.doi.org/10.15407/jnpae2023.04.324.

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The barrier penetrability, decay constant and decay half-life of 1-n halo nuclei 11Be, 15,17,19C, 22N, 23O, 24,26F, 29,31Ne, 34,37Na, 35,37Mg, and 55Ca; and 2-n halo nuclei 22C, 27,29F, 34Ne, 36Na, and 46P from Z = 127 – 132 parents were calculated within the framework of the Coulomb and proximity potential model by calculating the Q-values using the finite-range droplet model. A comparison between the decay half-lives is made by considering the halo candidates as a normal cluster and as a deformed structure with a rms radius. Neutron shell closure at 190, 196, 198, 200, 204, and 208 are ident

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8

Chulkov, L. V. "Fragmentation of halo nuclei." Il Nuovo Cimento A 111, no. 6-7 (1998): 791–802. http://dx.doi.org/10.1007/bf03185350.

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9

Lombard, R. J. "Remarks on halo nuclei." Physics of Atomic Nuclei 64, no. 7 (2001): 1240–43. http://dx.doi.org/10.1134/1.1389549.

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10

ZhengDa, Wang, Wang XiaoBin, Wang XiaoChun, and Zhang XiaoDong. "Spectra of Halo Nuclei." Communications in Theoretical Physics 33, no. 1 (2000): 81–86. http://dx.doi.org/10.1088/0253-6102/33/1/81.

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11

Jonson, B. "Halo states in nuclei." Nuclear Physics A 631 (March 1998): 376–84. http://dx.doi.org/10.1016/s0375-9474(98)00035-9.

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12

Tanihata, Isao, and Rituparna Kanungo. "Halo and skin nuclei." Comptes Rendus Physique 4, no. 4-5 (2003): 437–49. http://dx.doi.org/10.1016/s1631-0705(03)00065-3.

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13

Tomio, L. "Universality and Halo Nuclei." EPJ Web of Conferences 3 (2010): 01013. http://dx.doi.org/10.1051/epjconf/20100301013.

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14

Hussein, M. S., C. A. Bertulani, L. F. Canto, R. Donangelo, M. P. Pato, and A. F. R. de Toledo Piza. "Fusion of halo nuclei." Nuclear Physics A 588, no. 1 (1995): c85—c89. http://dx.doi.org/10.1016/0375-9474(95)00104-9.

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15

Akkoyun, Serkan. "Machine Learning Based Classification of the Halos in Light Nuclei Region." Cumhuriyet Science Journal 45, no. 1 (2024): 160–63. http://dx.doi.org/10.17776/csj.1416907.

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Experimental and theoretical studies on halo nuclei, whose nucleon binding energies are extremely weak, are among the most interesting topics of nuclear physics studies. By better defining and understanding this unusual behavior of these nuclei, our understanding of nuclear structure can be further improved. Although there are already a few experimentally proven halo nuclei in the literature, many others have found their place in the literature as candidate halo nuclei. In this study, the classification of halo nuclei was carried out using an artificial neural network approach. In the light nu

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16

Izosimov, Igor. "Borromean halo, Tango halo, and halo isomers in atomic nuclei." EPJ Web of Conferences 107 (2016): 09003. http://dx.doi.org/10.1051/epjconf/201610709003.

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17

Nakatsukasa, Takashi, Kazuhiro Yabana, Makoto Ito, Minoru Kobayashi, and Manabu Ueda. "Fusion Reaction of Halo Nuclei: Proton Halo versus Neutron Halo." Progress of Theoretical Physics Supplement 154 (2004): 85–91. http://dx.doi.org/10.1143/ptps.154.85.

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18

N. ABDULLAH, Ahmed. "NUCLEAR STRUCTURE STUDY OF THE HALO NUCLEI." MINAR International Journal of Applied Sciences and Technology 05, no. 04 (2023): 246–61. http://dx.doi.org/10.47832/2717-8234.17.18.

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The existence of halo nuclei is one of the major important discoveries in the field of nuclear physics. These nuclei are treated as loosely bound system in which a core of normal nuclear density is surrounded by so-called neutron (or proton) halo of diluted nuclear matter. Many theoretical investigations have attempted to understand these nuclei, which exist at light to heavy masses. The phenomenon of nuclear halo is a quantum effect that occurs in nuclei due to the presence of valence nucleons with low separation energy and I = 0, 1 (low angular momentum), and is manifested by the extraordina

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19

YAMASHITA, M. T., T. FREDERICO, and M. H. HUSSEIN. "A DOORWAY TO BORROMEAN HALO NUCLEI: THE SAMBA CONFIGURATION." Modern Physics Letters A 21, no. 22 (2006): 1749–55. http://dx.doi.org/10.1142/s0217732306020056.

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We exploit the possibility of new configurations in three-body halo nuclei, Samba type (the neutron-core form a bound system) as a doorway to Borromean systems. The nuclei 12 Be , 15 B , 23 N and 27 F are of such nature, in particular 23 N with a half-life of 37.7 s and a halo radius of 6.07 fm is an excellent example of Samba-halo configuration. The fusion below the barrier of the Samba halo nuclei with heavy targets could reveal the so far elusive enhancement and a dominance of one-neutron over two-neutron transfers, in contrast to what was found recently for the Borromean halo nucleus 6 He

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20

LIANG, YU-JIE, ZU-HUA LIU, and HONG-YU ZHOU. "INVESTIGATIONS ON THE NUCLEAR HALO STRUCTURES." International Journal of Modern Physics E 17, no. 09 (2008): 1729–38. http://dx.doi.org/10.1142/s0218301308010738.

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The halo structures in some light nuclei are investigated systemically with the nuclear asymptotic normalization coefficient (ANC) method and the relativistic mean-field (RMF) theory. Some important results about the halo structures in mirror nuclei are obtained, and some qualitative analyses are made to explore the role of Coulomb effects on the formation of proton halo nuclei.

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21

VAAGEN, J. S., B. V. DANILIN, and S. N. ERSHOV. "CONTINUUM SPECTROSCOPY OF HALO NUCLEI." International Journal of Modern Physics E 16, no. 04 (2007): 1033–45. http://dx.doi.org/10.1142/s0218301307006484.

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Halo nuclei represent a new type of structure found in extremely neutron rich light nuclei, at the limits of nuclear existence. Of particular interest are Borromean nuclei, where none of the binary substructures can bind. Similar structures, Efimov states, have now also been produced in traps in molecular physics. Nuclear physics has in recent years taken further steps to also explore the nature of the halo continuum, in fact the major part of the spectrum since halo nuclei support only one or a few bound states. Since 3 → 3 scattering is prohibitively difficult to perform, the halo continuum

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22

Baran, Andrzej. "Neutron halo in heavy nuclei." Journal of Physics G: Nuclear and Particle Physics 31, no. 10 (2005): S1823—S1826. http://dx.doi.org/10.1088/0954-3899/31/10/080.

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23

Nakamura, T., and N. Fukuda. "Breakup reactions of halo nuclei." European Physical Journal A 25, S1 (2005): 325–26. http://dx.doi.org/10.1140/epjad/i2005-06-139-4.

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24

Fukuda, Naoki, Takashi Nakamura, Toshio Kobayashi, et al. "Coulomb Dissociation of Halo Nuclei." Progress of Theoretical Physics Supplement 146 (2002): 462–66. http://dx.doi.org/10.1143/ptps.146.462.

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25

Pal, M. K. "Antisymmetrized treatment of halo nuclei." Journal of Physics G: Nuclear and Particle Physics 24, no. 8 (1998): 1513–17. http://dx.doi.org/10.1088/0954-3899/24/8/027.

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26

Furutachi, N., M. Kimura, A. Dote, and Y. Kanada-En'yo. "Structures of Light Halo Nuclei." Progress of Theoretical Physics 122, no. 4 (2009): 865–80. http://dx.doi.org/10.1143/ptp.122.865.

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27

Bai, Xinhua, and Jimin Hu. "Neutron halo in light nuclei." Physics Letters B 395, no. 3-4 (1997): 151–56. http://dx.doi.org/10.1016/s0370-2693(97)00070-1.

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28

Nakamura, T., N. Fukuda, N. Aoi, et al. "Coulomb dissociation of halo nuclei." Nuclear Physics A 722 (July 2003): C301—C307. http://dx.doi.org/10.1016/s0375-9474(03)01381-2.

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29

Barranco, F., E. Vigezzi, and R. A. Broglia. "Momentum distributions in halo nuclei." Zeitschrift für Physik A: Hadrons and Nuclei 356, no. 1 (1996): 45–48. http://dx.doi.org/10.1007/s002180050146.

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30

Bertulani, C. A. "Electron scattering on halo nuclei." Physics Letters B 624, no. 3-4 (2005): 203–9. http://dx.doi.org/10.1016/j.physletb.2005.08.030.

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31

Ershov, S. N. "Breakup reactions of halo nuclei." Physics of Atomic Nuclei 67, no. 10 (2004): 1851–59. http://dx.doi.org/10.1134/1.1811190.

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32

Fedorov, D. V., A. S. Jensen, and K. Riisager. "Efimov States in Halo Nuclei." Physical Review Letters 73, no. 21 (1994): 2817–20. http://dx.doi.org/10.1103/physrevlett.73.2817.

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33

Johnson, R. C., J. S. Al-Khalili, and J. A. Tostevin. "Elastic Scattering of Halo Nuclei." Physical Review Letters 79, no. 15 (1997): 2771–74. http://dx.doi.org/10.1103/physrevlett.79.2771.

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34

Sagawa, H. "Multipole resonances in halo nuclei." Nuclear Physics A 538 (March 1992): 619–25. http://dx.doi.org/10.1016/0375-9474(92)90810-7.

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35

Jonson, B. "Halo nuclei and other exotics." Nuclear Physics A 583 (February 1995): 733–46. http://dx.doi.org/10.1016/0375-9474(94)00752-9.

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36

Sagawa, H. "Density distributions of halo nuclei." Physics Letters B 286, no. 1-2 (1992): 7–12. http://dx.doi.org/10.1016/0370-2693(92)90150-3.

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37

Xiang, Yifeng, Qingjin Luo, Siqi Yang, and Kaiyuan Zhang. "Spherical, Axial, and Triaxial Symmetries in the Study of Halo Nuclei with Covariant Density Functional Theory." Symmetry 15, no. 7 (2023): 1420. http://dx.doi.org/10.3390/sym15071420.

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The halo phenomenon in exotic nuclei has long been an important frontier in nuclear physics research since its discovery in 1985. In parallel with the experimental progress in exploring halo nuclei, the covariant density functional theory has become one of the most successful tools for the microscopic study of halo nuclei. Based on spherical symmetry, the relativistic continuum Hartree–Bogoliubov theory describes the first halo nucleus 11Li self-consistently and predicts the giant halo phenomenon. Based on axial symmetry, the deformed relativistic Hartree–Bogoliubov theory in continuum has pre

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38

Abbas, Syed Afsar. "Fusion of halo nucleus 6He on 238U : Evidence for tennis-ball (bubble) structure of the core of the halo (even the giant-halo) nucleus." Modern Physics Letters A 34, no. 27 (2019): 1950221. http://dx.doi.org/10.1142/s0217732319502213.

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In a decade-and-a-half old experiment, Raabe et al. [Nature 431, 823 (2004)], had studied fusion of an incoming beam of halo nucleus 6He with the target nucleus [Formula: see text]. We extract a new interpretation of the experiment, different from the one that has been inferred so far. We show that their experiment is actually able to discriminate between the structures of the target nucleus (behaving as standard nucleus with density distribution described with canonical RMS radius [Formula: see text] with [Formula: see text] fm), and the “core” of the halo nucleus, which surprisingly, does no

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39

Ismail, Atef, Yen Cheong Lee, and Z. M. M. Mahmoud. "Puzzle of the folding potential on the nuclear halo reactions." International Journal of Modern Physics E 24, no. 04 (2015): 1550029. http://dx.doi.org/10.1142/s0218301315500299.

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Folding potentials of the elastic scattering drip-line nuclei at various incident energies is one method to study nuclear matter density distributions and nuclear radii. The nuclei with density distributions consisting of a bulk (core) and an outer layer (halo), dilute and spatially extended are called the halo nuclei caused for the weak particle binding. Several halo nuclei are studied and many potential candidates are identified. All the cross-sections of the elastic scattering for the drip-line nuclei 11 Be and 6 He , are calculated to understand the exotic properties of these nuclei starti

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40

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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41

Dariush, Amirhashemi, Tanir A.Güneş, and Koç Kemal. "The Examination of the Halo Nucleus Properties of 6-11Li Isotopes According to the Shell Model." International Journal of Engineering and Technical Research (IJETR) Volume-8, Issue-3, March 2018, Volume-8, Issue-3, March 2018 (2018): 36–39. https://doi.org/10.5281/zenodo.1211597.

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Halo nuclei are separated into two as two or one neutron halo nuclei depending on the nucleon number taking place in their final orbits. These cores have three mass configurations as neutron-neutron-core (n+n+c). One neutron halo nuclei have two-mass configuration (n+c). Two mass system could be reduced to one mass system by accepting the last two neutrons of two halo nuclei called as dineutron as a single particle also by taking the phenomenon of pairing between the nucleons into consideration. In this way, it becomes easier to solve the cores transforming into one neutron halo state. The fir

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42

REN, ZHONGZHOU, NING LI, H. Y. ZHANG, and W. Q. SHEN. "A THREE-BODY MODEL ON NEUTRON HALO IN EXOTIC LIGHT NUCLEI." Modern Physics Letters A 18, no. 02n06 (2003): 174–77. http://dx.doi.org/10.1142/s0217732303010193.

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The three-body calculations on halo nuclei are reviewed and discussed. It is concluded that the ground state properties of halo nuclei 11 Li , 14 Be and 17 B are independent of the shape of two-body potentials and an explanation on it is given. It is also shown that an introduction of a three-body interaction may be useful for a good explanation of the properties of halo nuclei.

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43

Zhukov, M. V., Yu L. Parfenova, and J. S. Vaagen. "Reaction mechanisms for light halo nuclei." Physics of Atomic Nuclei 65, no. 4 (2002): 746–51. http://dx.doi.org/10.1134/1.1471285.

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44

ORR, NIGEL. "NEUTRON-NEUTRON CORRELATIONS IN HALO NUCLEI." Modern Physics Letters A 21, no. 31n33 (2006): 2503–11. http://dx.doi.org/10.1142/s0217732306022171.

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Work aimed at probing the spatial configuration of the valence neutrons in two-neutron halo nuclei using the technique of intensity interferometry is described. Following a brief review of the method and its application to our first measurements of the breakup of 6 He , 11 Li and 14 Be , the results of the analysis of a high statistics data set for 6 He are presented.

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45

Di Pietro, A., P. Figuera, M. Fisichella, M. Lattuada, and M. Zadro. "Elastic scattering induced by halo nuclei." Journal of Physics: Conference Series 492 (March 18, 2014): 012001. http://dx.doi.org/10.1088/1742-6596/492/1/012001.

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46

Hammer, H. W. "Few-Body Universality in Halo Nuclei." EPJ Web of Conferences 113 (2016): 01004. http://dx.doi.org/10.1051/epjconf/201611301004.

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47

Johnson, Ronald. "Scattering and Reactions of Halo Nuclei." Progress of Theoretical Physics Supplement 140 (2000): 33–50. http://dx.doi.org/10.1143/ptps.140.33.

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48

Sherr, Rubby. "Simple model of neutron ‘‘halo nuclei’’." Physical Review C 54, no. 3 (1996): 1177–81. http://dx.doi.org/10.1103/physrevc.54.1177.

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49

Esbensen, H., and G. F. Bertsch. "Nuclear induced breakup of halo nuclei." Physical Review C 59, no. 6 (1999): 3240–45. http://dx.doi.org/10.1103/physrevc.59.3240.

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50

Filippov, G. F. "Nature of halo in light nuclei." Physics of Atomic Nuclei 64, no. 7 (2001): 1236–39. http://dx.doi.org/10.1134/1.1389548.

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