Relevant bibliographies by topics / Neutron rich

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Neutron rich'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Neutron rich"

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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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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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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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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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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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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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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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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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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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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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Dissertations / Theses on the topic "Neutron rich"

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Brown, Simon Mark. "Neutron shell breaking in neutron-rich neon isotopes." Thesis, University of Surrey, 2010. http://epubs.surrey.ac.uk/2829/.

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The breaking of the N=20 shell gap in neutron-rich nuclei is investigated by studying the single-particle structure of 27Ne via neutron transfer onto a 26Ne beam. The observation of low-lying negative parity states in 27Ne above the 3/2+ ground state is further evidence of the raising of the νd3/2 orbital that is seen in other neutron-rich nuclei in the N=20 region. The previously unseen 7/2− state has been identified as unbound by 331 keV and lies above the already known 3/2− level. The measurements of the present work contradict SDPF-M Monte-Carlo Shell Model predictions, but are in good agreement with WBP shell model calculations in which the single-particle energies of the pf shell are artificially lowered by 1 MeV. This modification was made to mimic the closing of the N = 20 shell gap in neutron-rich nuclei. The predictions of the modifiedWBP calculations are also in agreement with experimental measurements in the adjacent nuclei of 25Ne and 29Mg. The calculations show that core-excited configurations play a significant role in both the 3/2+ ground state and the 7/2− intruder state in 27Ne.
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González, Boquera Claudia. "Neutron-rich matter in atomic nuclei and neutron stars." Doctoral thesis, Universitat de Barcelona, 2020. http://hdl.handle.net/10803/668774.

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The proper understanding of the equation of state (EoS) of highly asymmetric nuclear matter is essential when studying systems such as neutron stars (NSs). Using zero-range Skyrme interactions and finite-range interactions such as Gogny forces, momentum-dependent interactions (MDI) and simple effective interactions (SEI), we analyze the properties of the EoS and the influence they may have on the calculations for NSs. We start by studying the convergence properties of the Taylor series expansion of EoS in powers of the isospin asymmetry. Next, we analyze the accuracy of the results for β-stable nuclear matter, which is found in the interior of NSs, when it is computed using the Taylor expansion of the EoS. The agreement with the results obtained using the full expression of the EoS is better for interactions with small-to-moderate values of the slope of the symmetry energy L. The mass and radius relation for a NS is obtained by integrating the so-called Tolman-Oppenheimer-Volkoff (TOV) equations, where the input is the EoS of the system. We have studied the mass-radius relation for Skyrme and Gogny interactions, and we see that that very soft forces are not able to give stable solutions of the TOV equations and only the stiff enough parametrizations can provide 2M0 NSs. We also notice that none of the existing parametrizations of the standard Gogny D1 interaction is able to provide a NS inside the observational constraints. Because of that, we propose a new parametrization, which we name D1M∗, that is able to provide NSs of 2M0 while still providing the same good description of finite nuclei as D1M. A parametrization D1M∗∗ is also presented, which is fitted in the same way as D1M∗ and provides NSs up to 1.91M0. Moreover, we estimate the core-crust transition in NSs by finding where the nuclear matter in the core is unstable against fluctuations of the density. To do that, we employ two methods, the thermodynamical method and the dynamical method. In the case of finite-range interactions, such as the Gogny ones, to use the dynamical method we have had to derive the explicit expression of the energy curvature matrix in momentum space for this type of interactions. We observe a decreasing trend of the transition density with the slope L of the symmetry energy, while the correlation between the transition pressure and L is much lower. Finally different NS properties are studied. The crustal properties, such as the crustal mass, crustal thickness and crustal fraction of the moment of inertial have lower values if one computes them using the core-crust transition density obtained with the dynamical method instead of the one obtained with the thermodynamical method, pointing out the importance of the accurate evaluation of the transition density when studying observational phenomena. We have also studied the moment of inertia of NSs, which is compared to constraints proposed in the literature. Finally, the tidal deformability for NSs is also calculated and compared with the constraints coming from the GW170817 event detected by the LIGO and Virgo observatories and which accounts for the merger of two NSs in a binary system.
El coneixement de l’equació d’estat (EoS) de matèria altament densa i assimètrica és essencial per tal d’estudiar les estrelles de neutrons (NSs). En aquesta tesi s’analitzen, utilitzant interaccions de camp mig no relativistes, les propietats de l’EoS i la seva influència en càlculs de NSs. Primerament, s’estudia la convergència del desenvolupament en sèrie de Taylor de l’EoS en potències de l'assimetria d’isospí. Seguidament, s’analitza l’exactitud dels resultats per matèria β-estable, la qual es troba a l’interior de les NSs, quan es calcula utilitzant el desenvolupament de Taylor de l’EoS. La relació entre la massa i el radi obtinguda integrant les equacions Tolman-Oppenheimer-Volkoff (TOV) també és estudiada. A causa de que les interaccions de Gogny de la família D1 no aconsegueixen donar NSs compatibles amb observacions astrofísiques, en aquesta tesi proposem dues noves forces de Gogny, anomenades D1M∗ i D1M∗∗, les quals poden donar, respectivament, NSs de 2 i 1.91 masses solars. Una altra part de la tesi es dedica a l’estudi de la transició entre l’escorça i el nucli, buscant la densitat a la qual la matèria uniforme al nucli és inestable contra fluctuacions de densitat. Ho estudiem amb dos mètodes, el mètode termodinàmic i el mètode dinàmic. Finalment, s’analitzen diverses propietats de les NSs, com són la relació entre la massa i el radi de l’estrella, les propietats de l’escorça, el moment d’inèrcia, així com la deformació deguda als corrents de marea (tidal deformability) que està relacionada amb l’emissió d’ones gravitacionals en sistemes binaris d’estrelles de neutrons.
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Reed, Alan Thomas. "Decay studies of neutron-rich nuclei." Thesis, University of Liverpool, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.367175.

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Gengelbach, Aila. "Collectivity in Neutron-Rich Erbium Isotopes." Licentiate thesis, Uppsala universitet, Kärnfysik, 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-442208.

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Neutron-rich rare-earth nuclei around the maximum of collectivity are predicted to exist with an extremely stable intrinsic configuration in their ground-state structure. Due to the high degree of axial symmetry and large deformation, these nuclei are also excellent candidates for having long-lived high-K isomers. The present work concerns a study of the structure of the yrast bands and a search for isomers in the neutron-rich 68Er isotopes. Excited states of 68Er isotopes were populated via multi-nucleon transfer reactions. A 859 MeV 136Xe-beam was used to bombard a 170Er-target. The experimental setup consisted of the high-resolution γ-ray spectrometer AGATA coupled to the heavy-ion magnetic spectrometer PRISMA. The experiment collected 2 TB of useful data corresponding to 3 days of effective beam time. Beam-like fragments were identified by the PRISMA specrometer placed at the grazing angle of 44 degrees. PRISMA allows for Z, A and q identification as well as TOF and velocity vector determination. This is required for the Doppler correction of the emitted γ rays detected in time coincidence with AGATA. A good Z and very clean A separation has been achieved in PRISMA. Making use of two-body kinematics, Doppler corrected γ-ray spectra for target-like fragments were obtained as well. Due to the novel techniques of PSA and γ-ray tracking, AGATA provided high-quality γ-ray spectra for both beam-like xenon and target-like erbium isotopes. Known yrast bands and isomeric states in neutron-rich erbium isotopes were observed. A candidate for the decay of an isomeric state with Eγ=184 keV  in 173Er, which has no previously known excited states, was identified.
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Woods, P. J. "Mass measurements of light neutron rich nuclei." Thesis, University of Manchester, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.374579.

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Rueffer, Mareike. "Collinear laser spectroscopy of neutron-rich niobium." Thesis, University of Birmingham, 2010. http://etheses.bham.ac.uk//id/eprint/802/.

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Hyperfine structure spectra and isotope shifts of the neutron-rich nuclei \(^{99}\)Nb, \(^{101}\)Nb, \(^{102}\)Nb and \(^{103}\)Nb were obtained at the IGISOL (Ion Guide Isotope Separator On-Line) facility at the accelerator laboratory of the University of Jyväskylä. The data were taken using collinear laser spectroscopy of bunched beams. Optical pumping from the ground state to populate metastable atomic states in the ion beam cooler allowed efficient spectroscopy of the ionic system that would otherwise be inaccessible due to a lack of suitable ground state resonance lines. The measurements of the hyperfine structure and the isotope shifts contribute valuable nuclear information to the understanding of the \(A\) ~ 100 region which displays a sudden onset of deformation that cannot be explained by the single particle shell model. It was possible to confirm the spin assignments for \(^{99}\)Nb, \(^{101}\)Nb and \(^{103}\)Nb as \(I\) = 9/2, \(I\) = 5/2 and \(I\) = 5/2 respectively. The extracted information on the mean square charge radii, \(\delta\big\), the magnetic dipole moments, \(\mu\), and the electric quadrupole moments, \(Q\), confirm a shape change of nuclei at \(N\) = 60 from soft and oblate (for \(N\)< 60) to more rigid and strongly prolate shapes (for \(N\geq\)60).
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Patel, Dinesh. "Magnetic properties of neutron-rich fission fragments." Thesis, University of Manchester, 2003. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.756107.

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Pietras, Ben. "Spectroscopy of neutron-rich oxygen and fluorine nuclei via single-neutron knockout reactions." Thesis, University of Liverpool, 2009. http://livrepository.liverpool.ac.uk/3713/.

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At the limits of nuclear stability, increasing proton-neutron asymmetry leads to a shifting of orbitals from nuclear shell model predictions. In turn this leads to a weakening of shell gaps such as at N = 20, and the emergence of new gaps at N = 14 and 16. To observe this evolution of the structure as the neutron dripline is approached, single-nucleon removal reactions have been employed for oxygen and fluorine isotopes. These reactions are an excellent way of probing the nuclear wavefunction to reveal information on the single-particle content in the wavefunction. Cross sections have been measured, both inclusive and exclusive, and partial production cross sections calculated. This has allowed spectroscopic factors to be extracted and compared to theoretical predictions from shell model calculations. Longitudinal momentum distributions, both inclusive and exclusive, have also been measured. The orbital angular momentum of the removed nucleon has a pronounced effect on the momentum distribution of the surviving core, which can be compared to theoretical predictions based on eikonal theory. This gives a valuable insight into the configuration mixing for the ground and excited states of the nuclei of interest.
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O'Donnell, David. "γ-Ray spectroscopy of neutron-rich chlorine nuclei." Thesis, University of the West of Scotland, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.556205.

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A beam of 36/16S20 at 215 MeV was used to bombard a 300 ugcm-2 thick target of 208/82Pb126 in order to initiate deep-inelastic and multi-nucleon transfer reactions. The I-ray decay of the reaction products was studied using the CLARA array of escape suppressed germanium detectors which was coupled to the large-angular-acceptance magnetic spectrometer PRISMA, in which the velocity, mass, atomic number and kinetic energy of the reaction products was measured. Determination of the velocity and mass has allowed Doppler corrected γ-ray spectra to be obtained for each individual projectile-like nuclide to be produced. Seven neutron-rich isotopes of Cl have been populated and their decay by γ-ray emission has been studied. Decay schemes have been constructed and compared to the results of shell-model calculations. Previously unreported transitions have been observed in 38Cl, 40Cl, 41Cl and 42Cl. ___.
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Valiente-Dobon, Jose Javier. "Studies of neutron-rich nuclei using deep inelastic collisions." Thesis, University of Surrey, 2003. http://epubs.surrey.ac.uk/843390/.

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A deep inelastic reaction between a thin self-supporting 19878Pt target and an 850MeV 13654Xe beam has been used to populate and study both neutron-rich nuclei around the beam and target masses and the reaction mechanism. An Ipi= 10+ isomeric state has been found in the N = 80 isotone 13656Ba with a measured half-life of 91 +/- 2ns. The structure of the predominantly (h11/2)-210+ isomer is discussed in terms of shell model and pair-truncated shell model calculations and compared to the even-Z, N = 80 isotones ranging from 13050Sn to 14868Er. A qualitative explanation of the observed dramatic decrease in the B(E2 : 10+ → 8+) value for the N = 80 isotones at 136Ba is given in terms of the increasing single-particle energy of the h11/2 neutron configuration as the proton sub-shell is filled. A 4-quasiparticle isomer has been observed in with a half-life of 188 +/- 38ns. The results are compared with blocked BCS Nilsson calculations which favour the Kpi= 15- interpretation. This isomer completes the even-A tungsten, 4-quasiparticle isomer systematics from A = 176 to 186. A high spin isomeric state has been found in the near spherical nucleus 19874W with a half-life of 36 +/- 2ns. The nature of this isomer has been interpreted from an examination of the systematics of platinum isotopes and neighbouring nuclei as a tentative Ipi= 12+ state from rotation-aligned, two neutron (i13/2)2configuration. Using prompt-delayed gamma-ray correlations, the complementary fragments of the reaction have been studied and used to identify new states in 19476Os. The angular momentum transfer to the binary fragments in the reaction has been investigated in terms of the average total gamma-ray fold versus the scattering angle of the recoils.
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Books on the topic "Neutron rich"

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Vernon, Adam Robert. Collinear Resonance Ionization Spectroscopy of Neutron-Rich Indium Isotopes. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-54189-7.

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Schopper, H., ed. Tables of Excitations of Proton- and Neutron-Rich Unstable Nuclei. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-75278-3.

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M, Ishihara, Takigawa N. 1943-, and Yamaji S, eds. RIKEN International Workshop on Heavy-Ion Reactions with Neutron-Rich Beams, Wako, Japan, 18-20 February 1993. Singapore: World Scientific, 1993.

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International Conference on Fission and Properties of Neutron-Rich Nuclei (4th 2007 Sanibel Island, Fla.). Fission and properties of neutron-rich nuclei: Proceedings of the fourth International Conference, Sanibel Island, USA, 11-17 November 2007. Edited by Hamilton Joseph H, Ramayya A. V, and Carter H. K. Singapore: World Scientific, 2008.

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H, Hamilton Joseph, Ramayya A. V, and Carter H. K, eds. Fission and properties of neutron-rich nuclei: Proceedings of the fourth International Conference, Sanibel Island, USA, 11-17 November 2007. Singapore: World Scientific, 2008.

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Zyromski, Kristiana Elizabeth. Fusion enhancement with neutron-rich radioactive beams. 1999.

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Ishihara, M. Heavy-Ion Reactions With Neutron-Rich Beam: Proceedings of the Riken International Workshop. World Scientific Publishing Company, 1993.

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Fission and Properties of Neutron-Rich Nuclei: Proceedings of the 2nd International Conference. World Scientific Publishing Company, 2000.

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Hamilton, J. H., A. V. Ramayya, Joseph H. Hamilton, and Akunuri V. Ramayya. Fission and Properties of Neutron-Rich Nuclei - Proceedings of the Fifth International Conference on Icfn5. World Scientific Publishing Co Pte Ltd, 2013.

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Pillai, Chandrasekhara. Direct mass measurements of light neutron-rich nuclei using a combined energy and time-of-flight technique. 1985.

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Book chapters on the topic "Neutron rich"

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Myint, Khin Swe, T. Harada, S. Shinmura, and Y. Akaishi. "Neutron Rich Lambda Hypernuclei." In Few-Body Problems in Physics ’99, 383–86. Vienna: Springer Vienna, 2000. http://dx.doi.org/10.1007/978-3-7091-6287-3_67.

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Pougheon, F. "Very neutron-rich exotic nuclei." In Atomic and Nuclear Clusters, 130–35. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79696-8_30.

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Ogloblin, Alexei A., and Yuri E. Penionzhkevich. "Very Neutron-Rich Very Light Nuclei." In Treatise on Heavy Ion Science, 261–360. Boston, MA: Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-0713-6_4.

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Trautvetter, H. P. "26Al-destruction in neutron rich environments." In Nucleosynthesis and Its Implications on Nuclear and Particle Physics, 347–54. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4578-4_39.

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Horiuchi, H., Y. Kanada-En’yo, and A. Ono. "Neutron-rich nuclei studied with AMD." In Atomic and Nuclear Clusters, 142–46. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79696-8_32.

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Day Goodacre, Thomas. "Charge Radii of Neutron Rich Mercury." In Applied Laser Spectroscopy for Nuclear Physics, 117–25. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-73889-1_10.

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Roeckl, Ernst. "Proton-Rich and Neutron-Rich Nuclei Produced by Heavy Ions." In ACS Symposium Series, 439–45. Washington, DC: American Chemical Society, 1986. http://dx.doi.org/10.1021/bk-1986-0324.ch066.

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Kane, Robert R., Karin Drechsel, Young Soo Kim, Cynthia L. Beno, Christine S. Lee, Gabriel Mendez, Solomon Romano, and M. Frederick Hawthorne. "Boron-Rich Oligophosphates — Novel Molecules for Use in BNCT." In Cancer Neutron Capture Therapy, 57–65. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4757-9567-7_6.

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Dlouhý, Z., D. Baiborodin, and J. Mrázek. "New neutron magic number N = 16 for neutron-rich nuclei." In Exotic Nuclei and Atomic Masses, 44. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/978-3-642-55560-2_11.

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Pfeiffer, B., and K.-L. Kratz. "The Proton-Neutron Interaction in Neutron-Rich A ≃ 100 Nuclei." In Nuclear Structure of the Zirconium Region, 368–75. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73958-3_48.

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Conference papers on the topic "Neutron rich"

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HOROWITZ, C. J. "NEUTRON RICH NUCLEI AND NEUTRON STARS." In Proceedings of the Fifth International Conference on ICFN5. WORLD SCIENTIFIC, 2013. http://dx.doi.org/10.1142/9789814525435_0065.

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Delaplane, R. G., T. Lundström, U. Dahlborg, and W. S. Howells. "A neutron diffraction study of amorphous boron." In Boron-rich solids. AIP, 1991. http://dx.doi.org/10.1063/1.40877.

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Sakaguchi, Atsushi. "Neutron-Rich Λ Hypernuclei." In Proceedings of the 12th International Conference on Hypernuclear and Strange Particle Physics (HYP2015). Journal of the Physical Society of Japan, 2017. http://dx.doi.org/10.7566/jpscp.17.011007.

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Sakurai, H., S. M. Lukyanov, M. Notani, N. Aoi, D. Beaumel, N. Fukuda, M. Hirai, et al. "New neutron-rich isotope." In EXOTIC NUCLEI AND ATOMIC MASSES. ASCE, 1998. http://dx.doi.org/10.1063/1.57323.

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Marketin, Tomislav, André Sieverding, Meng-Ru Wu, Nils Paar, and Gabriel Martínez-Pinedo. "Beta-Delayed Neutron Emission in Neutron-Rich Nuclei." In Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016). Journal of the Physical Society of Japan, 2017. http://dx.doi.org/10.7566/jpscp.14.020605.

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Severyukhin, A. P., N. N. Arsenyev, E. O. Sushenok, I. N. Borzov, Yu E. Penionzhkevich, and D. Verney. "MULTI-NEUTRON EMISSION OF NEUTRON-RICH Ca ISOTOPES." In International Symposium on Exotic Nuclei EXON-2016. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226548_0016.

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Adenwalla, Shireen, Ravi Billa, Jennifer I. Brand, Ellen Day, Manuel J. Diaz, Andrew Harken, Angel McMullen-Gunn, Rekha Padmanabhan, and Brian W. Robertson. "Semiconducting boron-rich neutron detectors." In Optical Science and Technology, SPIE's 48th Annual Meeting, edited by F. Patrick Doty, H. Bradford Barber, and Hans Roehrig. SPIE, 2004. http://dx.doi.org/10.1117/12.506646.

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NAZAREWICZ, W., and M. PlOSZAJCZAK. "STRUCTURE OF NEUTRON-RICH NUCLEI." In Proceedings of the Third International Conference. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812705211_0001.

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WIESCHER, M. "ASTROPHYSICS OF NEUTRON RICH NUCLEI." In Proceedings of the Third International Conference. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812705211_0049.

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HORIUCHI, HISASHI. "CLUSTERING IN NEUTRON-RICH NUCLEI." In Proceedings of the Third ANL/MSU/JINA/INT RIA Workshop. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812708250_0011.

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Reports on the topic "Neutron rich"

1

Esbensen, H. Pair correlations in neutron-rich nuclei. Office of Scientific and Technical Information (OSTI), August 1995. http://dx.doi.org/10.2172/166475.

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Ahmad, I., C. J. Lister, and L. R. Morss. Level structures of neutron-rich Xe isotopes. Office of Scientific and Technical Information (OSTI), August 1995. http://dx.doi.org/10.2172/166328.

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Wiedeking, M., P. Fallon, L. Bernstein, A. Macchiavelli, L. Phair, J. Burke, D. Bleuel, et al. Studying neutron-rich 18 N in fusion-evaporation reactions. Office of Scientific and Technical Information (OSTI), July 2006. http://dx.doi.org/10.2172/895994.

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Chasteler, R. M. Nuclear-decay studies of neutron-rich rare-earth nuclides. Office of Scientific and Technical Information (OSTI), April 1990. http://dx.doi.org/10.2172/6738019.

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Reeder, P. L., Y. Kim, W. K. Hensley, H. S. Miley, R. A. Warner, D. J. Vieira, J. M. Wouters, Z. Y. Zhou, and H. L. Seifert. Beta decay data for neutron-rich Li-Cl nuclides. Office of Scientific and Technical Information (OSTI), May 1994. http://dx.doi.org/10.2172/10162840.

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Urban, W., M. A. Jones, and J. L. Durell. Crossings in alternating-parity bands of neutron-rich Ba nuclei. Office of Scientific and Technical Information (OSTI), July 1995. http://dx.doi.org/10.2172/510564.

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Ahmad, I., C. J. Lister, and L. R. Morss. Lifetimes in neutron-rich Nd isotopes measured by Doppler profile method. Office of Scientific and Technical Information (OSTI), August 1995. http://dx.doi.org/10.2172/166329.

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Carpenter, M. P., R. V. F. Janssens, and I. Ahmad. Gamma-ray spectroscopy of neutron-rich products of heavy-ion collisions. Office of Scientific and Technical Information (OSTI), August 1995. http://dx.doi.org/10.2172/166333.

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Wu, Ching-Yen. Shape evolution in neutron-rich nuclei near the r-process path. Office of Scientific and Technical Information (OSTI), October 2015. http://dx.doi.org/10.2172/1226934.

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Ahmad, I., C. J. Lister, and L. R. Morss. Triaxial shapes in the ground states of even-even neutron-rich Ru isotopes. Office of Scientific and Technical Information (OSTI), August 1995. http://dx.doi.org/10.2172/166327.

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