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Journal articles on the topic 'Neutron rich'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

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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2

Harada, Toru. "Neutron-rich Hypernuclei." Nuclear Physics A 835, no. 1-4 (April 2010): 136–43. http://dx.doi.org/10.1016/j.nuclphysa.2010.01.186.

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3

Bressani, Tullio, Elena Botta, and Stefania Bufalino. "Neutron-Rich Hypernuclei." Nuclear Physics News 22, no. 3 (July 2012): 13–18. http://dx.doi.org/10.1080/10619127.2012.683718.

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4

Alcain, P. N., and C. O. Dorso. "The neutrino opacity of neutron rich matter." Nuclear Physics A 961 (May 2017): 183–99. http://dx.doi.org/10.1016/j.nuclphysa.2017.02.011.

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5

HOROWITZ, C. J. "MULTI-MESSENGER OBSERVATIONS OF NEUTRON-RICH MATTER." International Journal of Modern Physics E 20, no. 10 (October 2011): 2077–100. http://dx.doi.org/10.1142/s0218301311020332.

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At very high densities, electrons react with protons to form neutron-rich matter. This material is central to many fundamental questions in nuclear physics and astrophysics. Moreover, neutron-rich matter is being studied with an extraordinary variety of new tools such as Facility for Rare Isotope Beams (FRIB) and the Laser Interferometer Gravitational Wave Observatory (LIGO). We describe the Lead Radius Experiment (PREX) that uses parity violating electron scattering to measure the neutron radius in 208Pb. This has important implications for neutron stars and their crusts. We discuss X-ray observations of neutron star radii. These also have important implications for neutron-rich matter. Gravitational waves (GW) open a new window on neutron-rich matter. They come from sources such as neutron star mergers, rotating neutron star mountains, and collective r-mode oscillations. Using large scale molecular dynamics simulations, we find neutron star crust to be very strong. It can support mountains on rotating neutron stars large enough to generate detectable gravitational waves. Finally, neutrinos from core collapse supernovae (SN) provide another, qualitatively different probe of neutron-rich matter. Neutrinos escape from the surface of last scattering known as the neutrino-sphere. This is a low density warm gas of neutron-rich matter. Neutrino-sphere conditions can be simulated in the laboratory with heavy ion collisions. Observations of neutrinos can probe nucleosyntheses in SN. Simulations of SN depend on the equation of state (EOS) of neutron-rich matter. We discuss a new EOS based on virial and relativistic mean field calculations. We believe that combing astronomical observations using photons, GW, and neutrinos, with laboratory experiments on nuclei, heavy ion collisions, and radioactive beams will fundamentally advance our knowledge of compact objects in the heavens, the dense phases of QCD, the origin of the elements, and of neutron-rich matter.

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6

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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7

Krasznahorkay, A., H. Akimune, A. M. van den Berg, N. Blasi, S. Brandenburg, M. Csatlo´s, M. Fujiwara, et al. "Neutron-skin thickness in neutron-rich isotopes." Nuclear Physics A 731 (February 2004): 224–34. http://dx.doi.org/10.1016/j.nuclphysa.2003.11.034.

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8

Gal, A., and D. J. Millener. "Neutron-rich hypernuclei:HΛ6and beyond." Physics Letters B 725, no. 4-5 (October 2013): 445–50. http://dx.doi.org/10.1016/j.physletb.2013.07.027.

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9

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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10

Dörfler, T., W. D. Schmidt-Ott, T. Hild, T. Mehren, W. Böhmer, P. Möller, B. Pfeiffer, et al. "Neutron-rich isotopesTi54−57." Physical Review C 54, no. 6 (December 1, 1996): 2894–903. http://dx.doi.org/10.1103/physrevc.54.2894.

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11

Shuanggui, Yuan, Zhang Tianmei, Pan qiangyan, Zhang Xueqian, and Xu Shuwei. "New neutron-rich nuclide185Hf." Zeitschrift f�r Physik A Hadrons and Nuclei 344, no. 3 (September 1992): 355–56. http://dx.doi.org/10.1007/bf01303034.

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12

GRIDNEV, K. A., V. N. TARASOV, D. V. TARASOV, D. K. GRIDNEV, V. V. PILIPENKO, and W. GREINER. "THEORETICAL PREDICTION OF EXTREMELY NEUTRON RICH Zr AND Pb." International Journal of Modern Physics E 19, no. 03 (March 2010): 449–57. http://dx.doi.org/10.1142/s0218301310014868.

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The properties of even–even Zr and Pb isotopes in the ground state are studied up to the neutron drip-lines on the basis of the Hartree–Fock method with Skyrme forces allowing for deformation (DHF). The DHF calculations with Ska forces predict the existence of stability peninsula (or island) around 152 Zr . On the example of Zr isotopes it is shown that adding neutrons to an already unstable nucleus with neutron excess can restore the stability. It is demonstrated that extremely neutron-rich Pb isotopes for 222≤A≤230 have abnormally large deformation parameters of proton and neutron density distributions. The existence of 266–288 Pb stable against one-neutron emission is also predicted.

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13

Simpson, Gary. "Investigating the Structure of Neutron-Rich Nuclei with Neutrons." Nuclear Physics News 24, no. 1 (January 2, 2014): 26–27. http://dx.doi.org/10.1080/10619127.2013.855570.

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14

Hebeler, K., J. D. Holt, J. Menéndez, and A. Schwenk. "Nuclear Forces and Their Impact on Neutron-Rich Nuclei and Neutron-Rich Matter." Annual Review of Nuclear and Particle Science 65, no. 1 (October 19, 2015): 457–84. http://dx.doi.org/10.1146/annurev-nucl-102313-025446.

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15

Frank, N., T. Baumann, D. Bazin, B. A. Brown, J. Brown, P. A. DeYoung, J. E. Finck, et al. "Neutron decay spectroscopy of neutron-rich oxygen isotopes." Nuclear Physics A 813, no. 3-4 (December 2008): 199–211. http://dx.doi.org/10.1016/j.nuclphysa.2008.09.009.

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16

Horowitz, C. J. "Neutron rich matter, neutron stars, and their crusts." Journal of Physics: Conference Series 312, no. 4 (September 23, 2011): 042003. http://dx.doi.org/10.1088/1742-6596/312/4/042003.

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17

Hansen, P. G., and B. Jonson. "The Neutron Halo of Extremely Neutron-Rich Nuclei." Europhysics Letters (EPL) 4, no. 4 (August 15, 1987): 409–14. http://dx.doi.org/10.1209/0295-5075/4/4/005.

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18

Leist, B., W. Ziegert, M. Wiescher, K. L. Kratz, and F. K. Thielemann. "Neutron capture cross sections for neutron-rich isotopes." Zeitschrift f�r Physik A Atoms and Nuclei 322, no. 3 (September 1985): 531–32. http://dx.doi.org/10.1007/bf01412093.

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19

Abdullah, Ahmed N. "Nuclear structure investigation of some neutron-rich halo nuclei." International Journal of Modern Physics E 26, no. 07 (July 2017): 1750048. http://dx.doi.org/10.1142/s0218301317500483.

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The ground state proton, neutron and matter densities, the corresponding rms radii and charge form factors of a dripline nuclei 6He, [Formula: see text]Li, [Formula: see text]Be and [Formula: see text]Be have been studied via a three–body model of [Formula: see text]. The core–neutron interaction takes the form of Woods-Saxon (WS) potential. The two valence neutrons of 6He, [Formula: see text]Li and [Formula: see text]Be interact by the realistic interaction of ZBMII while those of [Formula: see text]Be interact via the realistic interaction of VPNP. The core and valence (halo) density distributions are described by the single-particle wave functions of the WS potential. The calculated results are discussed and compared with the experimental data. The long tail performance is clearly noticed in the calculated neutron and matter density distributions of these nuclei. The structure of the two valence neutrons in 6He, [Formula: see text]Li and [Formula: see text]Be is found to be mixed configurations with dominant [Formula: see text] while that for [Formula: see text]Be is mixed configurations with dominant ([Formula: see text]. The analysis of the present study supports the halo structure of these nuclei.

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20

KEMSLEY, JYLLIAN. "NEW NEUTRON-RICH ISOTOPES DISCOVERED." Chemical & Engineering News 85, no. 45 (November 5, 2007): 37. http://dx.doi.org/10.1021/cen-v085n045.p037.

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21

Horiuchi, H., Y. Kanada-En'yo, and M. Kimura. "Clustering in Neutron-Rich Nuclei." Acta Physica Hungarica A) Heavy Ion Physics 18, no. 2-4 (November 1, 2003): 209–13. http://dx.doi.org/10.1556/aph.18.2003.2-4.14.

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22

Ikeda, Kiyomi. "Structure of neutron rich nuclei." Nuclear Physics A 538 (March 1992): 355–65. http://dx.doi.org/10.1016/0375-9474(92)90785-i.

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23

Pougheon, F. "Very neutron-rich exotic nuclei." Zeitschrift f�r Physik A: Hadrons and Nuclei 349, no. 3-4 (September 1994): 273–78. http://dx.doi.org/10.1007/bf01288974.

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24

Borge, M. J. G., D. G. Burke, H. Gabelmann, P. Hill, O. C. Jonsson, N. Kaffrell, W. Kurcewicz, et al. "The new neutron-rich isotope228Rn." Zeitschrift f�r Physik A Atomic Nuclei 333, no. 1 (March 1989): 109–10. http://dx.doi.org/10.1007/bf01290116.

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25

Souliotis, G. A. "Approaching neutron-rich nuclei towards the r-process path in 86Kr-induced collisions at 15 MeV/nucleon." HNPS Proceedings 19 (January 1, 2020): 72. http://dx.doi.org/10.12681/hnps.2519.

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The production cross sections of projectile-like fragments from collisions of 15 MeV/nucleon 86Kr with 64,58Ni and 124,112Sn have been measured using a magnetic separator with emphasis on the neutron-rich isotopes. Neutron pick-up isotopes (with up to 6-8 neutrons picked-up from the target) were observed with large cross sections. The present results were also compared with our previous data of the same reactions at 25 MeV/nucleon. The data at 15 MeV/nucleon show enhanced production of neutron-rich isotopes very close to the projectile, relative to the corresponding data at 25 MeV/nucleon. The large cross sections of such reactions involving peripheral nucleon exchange, indicate that these reactions offer a novel route to access extremely neutron-rich rare isotopes towards the the astrophysical r-process path and the neutron-drip line.

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26

So, Woonyoung. "Effect of Valence Neutron(s) in Neutron-rich Nuclei." Journal of the Korean Physical Society 59, no. 4 (October 14, 2011): 2869–72. http://dx.doi.org/10.3938/jkps.59.2869.

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27

Cizewski, J. A., K. L. Jones, S. D. Pain, J. S. Thomas, C. Baktash, D. W. Bardayan, J. C. Blackmon, et al. "Neutron transfer reactions with neutron-rich radioactive ion beams." Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms 241, no. 1-4 (December 2005): 200–203. http://dx.doi.org/10.1016/j.nimb.2005.07.025.

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28

Matsuo, M., Y. Serizawa, and K. Mizuyama. "Di-neutron dynamics in medium-mass neutron-rich nuclei." Journal of Physics: Conference Series 20 (January 1, 2005): 113–18. http://dx.doi.org/10.1088/1742-6596/20/1/019.

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29

Thomas, J. S., D. W. Bardayan, J. C. Blackmon, J. A. Cizewski, R. P. Fitzgerald, U. Greife, C. J. Gross, et al. "Single-neutron excitations in neutron-rich N = 51 nuclei." European Physical Journal A 25, S1 (August 10, 2005): 371–74. http://dx.doi.org/10.1140/epjad/i2005-06-127-8.

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30

Manisa, Kaan. "EOS of neutron-rich matter and pure neutron matter." Science China Physics, Mechanics and Astronomy 55, no. 3 (February 13, 2012): 443–49. http://dx.doi.org/10.1007/s11433-012-4652-6.

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31

Riisager, K., R. Anne, S. E. Arnell, R. Bimbot, H. Emling, D. Guillemaud-Mueller, P. G. Hansen, et al. "Two-neutron removal reactions for very neutron-rich nuclei." Nuclear Physics A 540, no. 1-2 (April 1992): 365–82. http://dx.doi.org/10.1016/0375-9474(92)90210-b.

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32

Reffo, Gianni, M. Blann, T. Komoto, and R. J. Howerton. "Low energy neutron capture of neutron-rich target nuclides." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 267, no. 2-3 (May 1988): 408–24. http://dx.doi.org/10.1016/0168-9002(88)90483-4.

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33

AOYAMA, S., and N. ITAGAKI. "DI-NEUTRON CORRELATIONS IN THE SUPER NEUTRON-RICH NUCLEUS; 7H." Modern Physics Letters A 25, no. 21n23 (July 30, 2010): 1828–32. http://dx.doi.org/10.1142/s0217732310000423.

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We study the di-neutron correlations in the super neutron-rich nucleus 7 H with the AMD triple-S (AMD superposition of selected snapshots). 7 H is the most neutron-rich nucleus in the neutron ratio to the proton ( N / Z = 6). And the strong di-neutron correlations are expected due to the weak binding properties. In this paper, the mixing of di-neutron cluster components is estimated by calculating the squared overlap with the di-neutron condensate type wave function. The calculated results show significant mixing of di-neutron (t + 2n + 2n) components (70 ~ 80%).

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34

Torilov, S. Yu, K. A. Gridnev, and T. V. Korovitskaya. "Cluster states in neutron-rich nuclei." Bulletin of the Russian Academy of Sciences: Physics 77, no. 7 (July 2013): 849–51. http://dx.doi.org/10.3103/s1062873813070253.

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35

Shubhchintak, C. A. Bertulani, and T. Aumann. "Maris polarization in neutron-rich nuclei." Physics Letters B 778 (March 2018): 30–34. http://dx.doi.org/10.1016/j.physletb.2017.12.067.

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36

Podolyák, Zs, P. H. Regan, M. Pfützner, J. Gerl, M. Hellström, M. Caamaño, P. Mayet, et al. "Isomer spectroscopy of neutron rich 190W116." Physics Letters B 491, no. 3-4 (October 2000): 225–31. http://dx.doi.org/10.1016/s0370-2693(00)01051-0.

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37

Escrig, D., A. Jungclaus, B. Binder, A. Dietrich, T. Härtlein, H. Bauer, Ch Gund, et al. "Rotational bands in neutron-rich 160,161,162Ho." European Physical Journal A 21, no. 1 (July 2004): 67–74. http://dx.doi.org/10.1140/epja/i2003-10195-x.

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38

Gade, A., and S. N. Liddick. "Shape coexistence in neutron-rich nuclei." Journal of Physics G: Nuclear and Particle Physics 43, no. 2 (January 13, 2016): 024001. http://dx.doi.org/10.1088/0954-3899/43/2/024001.

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39

Prakash, M., and K. S. Bedell. "Incompressibility of neutron-rich nuclear matter." Physical Review C 32, no. 3 (September 1, 1985): 1118–21. http://dx.doi.org/10.1103/physrevc.32.1118.

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40

Uzu, E., M. Yamaguchi, H. Kamada, and Y. Koike. "Faddeev calculation for neutron-rich nuclei." Nuclear Physics A 790, no. 1-4 (June 2007): 286c—289c. http://dx.doi.org/10.1016/j.nuclphysa.2007.03.046.

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41

Gurgi, L. A., P. H. Regan, P. A. Söderström, H. Watanabe, P. M. Walker, Zs Podolyák, S. Nishimura, et al. "Isomer spectroscopy of neutron-rich 168Tb103." Radiation Physics and Chemistry 140 (November 2017): 493–96. http://dx.doi.org/10.1016/j.radphyschem.2016.12.011.

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42

Kameda, D., H. Ueno, K. Asahi, M. Takemura, A. Yoshimi, T. Haseyama, M. Uchida, et al. "Nuclear moments of neutron-rich 32Al." Journal of Physics: Conference Series 49 (October 10, 2006): 138–39. http://dx.doi.org/10.1088/1742-6596/49/1/030.

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43

Otsuka, Takaharu, Nobuhisa Fukunishi, and Hiroyuki Sagawa. "Structure of exotic neutron-rich nuclei." Physical Review Letters 70, no. 10 (March 8, 1993): 1385–88. http://dx.doi.org/10.1103/physrevlett.70.1385.

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44

Friedman, W. A., D. Bazin, W. G. Lynch, G. Renault, and M. B. Tsang. "Production of Rare Neutron-Rich Isotopes." Progress of Theoretical Physics Supplement 146 (2002): 549–50. http://dx.doi.org/10.1143/ptps.146.549.

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45

Schaffner, Jürgen, and Igor N. Mishustin. "Hyperon-rich matter in neutron stars." Physical Review C 53, no. 3 (March 1, 1996): 1416–29. http://dx.doi.org/10.1103/physrevc.53.1416.

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46

BRINE, M. P., P. D. STEVENSON, J. A. MARUHN, and P. G. REINHARD. "DIPOLE RESPONSE IN NEUTRON-RICH MAGNESIUM." International Journal of Modern Physics E 15, no. 07 (October 2006): 1417–23. http://dx.doi.org/10.1142/s0218301306005009.

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The time-dependent Hartree-Fock method, using the Skyrme interaction, is used to study the isovector giant dipole response of neutron-rich 34 Mg . The response is separately examined along the major and minor axes of this prolate nucleus, with a pygmy-like peak in the direction of the major axis at around 10 MeV. Time-dependent density plots show a superimposed surface mode not fully coupled to the bulk motion.

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47

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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48

Middleton, Christine. "Neutron-rich magnesium undergoes unexpected transitions." Physics Today 72, no. 4 (April 2019): 14–16. http://dx.doi.org/10.1063/pt.3.4177.

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49

Wolski, R., P. Roussel-Chomaz, S. I. Sidorchuk, and G. M. Ter-Akopian. "Search for extremely neutron rich systems." Nuclear Physics A 738 (June 2004): 431–35. http://dx.doi.org/10.1016/j.nuclphysa.2004.04.080.

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50

Hartmann, D., S. E. Woosley, and M. F. El Eid. "Nucleosynthesis in neutron-rich supernova ejecta." Astrophysical Journal 297 (October 1985): 837. http://dx.doi.org/10.1086/163580.

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