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Artigos de revistas sobre o tema "Nuclear properties"

Autor: Grafiati

Publicado: 15 de fevereiro de 2025

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1

Chung, K. C., C. S. Wang e A. J. Santiago. "Nuclear matter properties from nuclear masses". Europhysics Letters (EPL) 47, n.º 6 (15 de setembro de 1999): 663–67. http://dx.doi.org/10.1209/epl/i1999-00440-4.

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2

Poenaru, D. N., W. Greiner e E. Hourani. "C12emission fromBa114and nuclear properties". Physical Review C 51, n.º 2 (1 de fevereiro de 1995): 594–600. http://dx.doi.org/10.1103/physrevc.51.594.

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3

PASSAMANI, TOMAZ, e MARIA LUIZA CESCATO. "HOT NUCLEAR MATTER PROPERTIES". International Journal of Modern Physics E 16, n.º 09 (outubro de 2007): 3041–44. http://dx.doi.org/10.1142/s0218301307009002.

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The nuclear matter at finite temperature is described in the relativistic mean field theory using linear and nonlinear interactions. The behavior of effective nucleon mass with temperature was numerically calculated. For the nonlinear NL3 interaction we also observed the striking decrease at temperatures well below the nucleon mass. The calculation of NL3 nuclear matter equation of state at finite temperature is still on progress.

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4

Choi, Woong-Ki, Byung-Joo Kim, Eung-Seon Kim, Se-Hwan Chi e Soo-Jin Park. "Nuclear Graphites (II) : Mechanical Properties". Carbon letters 11, n.º 1 (30 de março de 2010): 41–47. http://dx.doi.org/10.5714/cl.2010.11.1.041.

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5

Böker, Torsten. "Properties of nuclear star clusters". Journal of Physics: Conference Series 131 (1 de outubro de 2008): 012043. http://dx.doi.org/10.1088/1742-6596/131/1/012043.

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6

Ehehalt, W., W. Cassing, A. Engel, U. Mosel e Gy Wolf. "Resonance properties in nuclear matter". Physical Review C 47, n.º 6 (1 de junho de 1993): R2467—R2469. http://dx.doi.org/10.1103/physrevc.47.r2467.

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7

Akaishi, Yoshinori, Akinobu Doté e Toshimitsu Yamazaki. "Properties of Nuclear-KBound States". Progress of Theoretical Physics Supplement 149 (2003): 221–32. http://dx.doi.org/10.1143/ptps.149.221.

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8

Cabrera, Daniel. "Meson Properties in Nuclear Medium". Progress of Theoretical Physics Supplement 149 (2003): 67–78. http://dx.doi.org/10.1143/ptps.149.67.

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9

Bozek, P. "Spectral properties of nuclear matter". Journal of Physics: Conference Series 35 (1 de abril de 2006): 373–83. http://dx.doi.org/10.1088/1742-6596/35/1/034.

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10

Smolyanskii, A. S., Yu A. Smirnova, V. G. Vasilenko, S. B. Burukhin, B. A. Briskman e V. K. Milinchuk. "Refractive properties of nuclear microfilters". Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms 155, n.º 3 (agosto de 1999): 331–34. http://dx.doi.org/10.1016/s0168-583x(99)00252-9.

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11

Wang, M., G. Audi, F. G. Kondev, B. Pfeiffer, J. Blachot, X. Sun e M. MacCormick. "NUBASE2012 Evaluation of Nuclear Properties". Nuclear Data Sheets 120 (junho de 2014): 6–7. http://dx.doi.org/10.1016/j.nds.2014.06.127.

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12

Baldo, M., e G. F. Burgio. "Properties of the nuclear medium". Reports on Progress in Physics 75, n.º 2 (9 de janeiro de 2012): 026301. http://dx.doi.org/10.1088/0034-4885/75/2/026301.

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13

Hassaneen. "THE PROPERTIES OF NUCLEAR MATTER". Physics International 4, n.º 1 (1 de janeiro de 2013): 37–59. http://dx.doi.org/10.3844/pisp.2013.37.59.

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14

LEJEUNE, A., J. CUGNON e P. GRANGE. "PROPERTIES OF HOT NUCLEAR MATTER". Le Journal de Physique Colloques 47, n.º C4 (agosto de 1986): C4–373—C4–376. http://dx.doi.org/10.1051/jphyscol:1986442.

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15

Wendler, W., P. Smeibidl e F. Pobell. "Nuclear magnetic properties of aluminium". Journal of Low Temperature Physics 108, n.º 3-4 (agosto de 1997): 291–304. http://dx.doi.org/10.1007/bf02398716.

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16

Close, F. E., R. G. Roberts e G. G. Ross. "Nuclear properties from perturbative QCD". Physics Letters B 168, n.º 4 (março de 1986): 400–404. http://dx.doi.org/10.1016/0370-2693(86)91652-7.

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17

Benhar, Omar, Alessandro Lovato e Lucas Tonetto. "Properties of Hot Nuclear Matter". Universe 9, n.º 8 (25 de julho de 2023): 345. http://dx.doi.org/10.3390/universe9080345.

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A fully quantitative description of the equilibrium and dynamical properties of hot nuclear matter will be needed for the interpretation of the available and forthcoming astrophysical data, providing information on the post-merger phase of a neutron star coalescence. We discuss the results of a recently developed theoretical model, based on a phenomenological nuclear Hamiltonian including two- and three-nucleon potentials, to study the temperature dependence of average and single-particle properties of nuclear matter relevant to astrophysical applications. The potential of the proposed approach for describing dissipative processes leading to the appearance of bulk viscosity in neutron star matter is also outlined.

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18

Ishkhanov, B. S., M. E. Stepanov e T. Yu Tretyakova. "Nuclear shell structure in the systematics of nuclear properties". Bulletin of the Russian Academy of Sciences: Physics 78, n.º 5 (maio de 2014): 405–11. http://dx.doi.org/10.3103/s1062873814050086.

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19

Orlov, S. "Gravitational Properties of Atom". Journal of Advance Research in Applied Science (ISSN: 2208-2352) 3, n.º 2 (29 de fevereiro de 2016): 19–26. http://dx.doi.org/10.53555/nnas.v3i2.660.

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The evidence that the strength of any body provide nuclear forces of gravity. The nuclear force of gravity generated by the essential micro vortices. The vortex creates a pressure gradient in the ether. The pressure gradient is the source of nuclear energy. The nuclear force of gravity on the surface of the cores is equal for all elementary particles.

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20

Orlov, Sergey. "Gravitational Properties of Atom". International Letters of Chemistry, Physics and Astronomy 54 (julho de 2015): 184–88. http://dx.doi.org/10.18052/www.scipress.com/ilcpa.54.184.

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The evidence that the strength of any body provide nuclear forces of gravity. The nuclear force of gravity generated by the essential micro vortices. The vortex creates a pressure gradient in the ether. The pressure gradient is the source of nuclear energy. The nuclear force of gravity on the surface of the cores is equal for all elementary particles.

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21

Orlov, Sergey. "Gravitational Properties of Atom". International Letters of Chemistry, Physics and Astronomy 54 (3 de julho de 2015): 184–88. http://dx.doi.org/10.56431/p-e3vh67.

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The evidence that the strength of any body provide nuclear forces of gravity. The nuclear force of gravity generated by the essential micro vortices. The vortex creates a pressure gradient in the ether. The pressure gradient is the source of nuclear energy. The nuclear force of gravity on the surface of the cores is equal for all elementary particles.

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22

Akito, Arima. "Nuclear structure, especially nuclear magnetic properties, studied by electron scattering". Nuclear Physics A 446, n.º 1-2 (dezembro de 1985): 45–64. http://dx.doi.org/10.1016/0375-9474(85)90579-2.

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23

Roca-Maza, X. "Nuclear Equation of State from Nuclear Collective Excited State Properties". Acta Physica Polonica B Proceedings Supplement 16, n.º 4 (2023): 1. http://dx.doi.org/10.5506/aphyspolbsupp.16.4-a1.

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24

Bolonkin, A. A. "Femtotechnology: Nuclear Matter with Fantastic Properties". American Journal of Engineering and Applied Sciences 2, n.º 2 (1 de fevereiro de 2009): 501–14. http://dx.doi.org/10.3844/ajeassp.2009.501.514.

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25

Kozlov, V. A., G. V. Seledtsova, A. B. Dorzhieva, I. P. Ivanova e V. I. Seledtsov. "Antitumor properties of nuclear erythroid cells". Siberian journal of oncology 21, n.º 3 (29 de junho de 2022): 42–49. http://dx.doi.org/10.21294/1814-4861-2022-21-3-42-49.

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Purpose. To study suppressor and/or cytotoxic activity of the nuclear erythroid cells (NEC) against tumor cells of various origins. Material and Methods. C57Bl/6 mice and P815, L1210, B16 and L929 tumor cells were used. “Phenylhydrazine” NECs were obtained from mice with induced hemolytic anemia. “Erythropoietin” NECs were isolated from the “phenylhydrazine spleen” and further cultured in the presence of erythropoietin. Another source of NEC was neonatal mouse spleen, human and mouse fetal liver cells, and mouse bone marrow cells cultured with erythropoietin. The cytostatic effect of NEC or their supernatants was recorded by reducing proliferation of P815, L1210, B16, LLC, L929 lines. Results. The presence of pronounced direct antitumor activity was found in both NEC and their culturing products in relation to cells of various tumor lines. The suppressor effect was not specifc. Conclusion. We know about the signifcant numerical predominance of NEC during the embryo development over all other hematopoietic cells and their high suppressive potential. Therefore, it can be assumed that erythroblasts are involved in process of creating antitumor protection of a fetus during this period of life.

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26

Kheswa, B. V., M. Wiedeking, F. Giacoppo, S. Goriely, M. Guttormsen, A. C. Larsen, F. L. Bello Garrote et al. "Statistical nuclear properties and synthesis of138La". EPJ Web of Conferences 93 (2015): 04005. http://dx.doi.org/10.1051/epjconf/20159304005.

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27

Ono, Akira. "Nuclear matter properties in fragmentation reactions". Journal of Physics: Conference Series 436 (17 de abril de 2013): 012068. http://dx.doi.org/10.1088/1742-6596/436/1/012068.

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28

Artun, Ozan. "Nuclear structure properties in neutron stars". International Journal of Modern Physics E 29, n.º 09 (setembro de 2020): 2050079. http://dx.doi.org/10.1142/s0218301320500792.

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The charge, proton and neutron density distributions along with nuclear properties were calculated by Hartree–Fock approach with Skyrme force interaction for isotopic Pb chain ([Formula: see text]). The effects of correlation on neutron skin thicknesses by obtaining bulk and surface contributions were analyzed by three different approaches. The occurrence of the nuclei with bubble structure due to central depletion in nucleonic was investigated for Pb isotopes as a function of relative neutron excess [Formula: see text]. The important role of the bubble effect in heavy region was explained by the relation between Coulomb and nn-interaction. The single particle energy levels were determined by each [Formula: see text] state of stable Pb isotopes, as well as charge form factors [Formula: see text]. Besides, the average neutron–proton [Formula: see text] and residual neutron–proton [Formula: see text] interactions of the Pb isotopes were calculated by the theoretical binding energies. The fluctuations in the obtained results were considered in detail because its variation may give a good criterion for the mass model approaches.

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29

Nishizaki, S., T. Takatsuka e J. Hiura. "Properties of Hot Asymmetric Nuclear Matter". Progress of Theoretical Physics 92, n.º 1 (1 de julho de 1994): 93–109. http://dx.doi.org/10.1143/ptp/92.1.93.

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30

Eichholz, Geoffrey G. "Thorium Dioxide: Properties and Nuclear Applications". Nuclear Technology 76, n.º 2 (fevereiro de 1987): 309. http://dx.doi.org/10.13182/nt87-a33886.

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31

Carbone, Arianna, e Omar Benhar. "Transport properties ofβ-stable nuclear matter". Journal of Physics: Conference Series 336 (28 de dezembro de 2011): 012015. http://dx.doi.org/10.1088/1742-6596/336/1/012015.

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32

Hayano, Ryugo S., e Tetsuo Hatsuda. "Hadron properties in the nuclear medium". Reviews of Modern Physics 82, n.º 4 (27 de outubro de 2010): 2949–90. http://dx.doi.org/10.1103/revmodphys.82.2949.

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33

Von-Eiff, D., W. Stocker e M. K. Weigel. "Relativistic investigation of nuclear surface properties". Physical Review C 50, n.º 3 (1 de setembro de 1994): 1436–44. http://dx.doi.org/10.1103/physrevc.50.1436.

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34

Dickhoff, W. H., e H. Muther. "Nucleon properties in the nuclear medium". Reports on Progress in Physics 55, n.º 11 (1 de novembro de 1992): 1947–2023. http://dx.doi.org/10.1088/0034-4885/55/11/002.

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35

Starosta, K., I. Hamamoto, T. Koike e C. Vaman. "Electromagnetic properties of nuclear chiral partners". Physica Scripta T125 (28 de junho de 2006): 18–20. http://dx.doi.org/10.1088/0031-8949/2006/t125/004.

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36

Audi, G., F. G. Kondev, M. Wang, B. Pfeiffer, X. Sun, J. Blachot e M. MacCormick. "The Nubase2012 evaluation of nuclear properties". Chinese Physics C 36, n.º 12 (dezembro de 2012): 1157–286. http://dx.doi.org/10.1088/1674-1137/36/12/001.

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37

Rapp, R. E., e H. Godfrin. "Nuclear magnetic properties ofHe3adsorbed on graphite". Physical Review B 47, n.º 18 (1 de maio de 1993): 12004–17. http://dx.doi.org/10.1103/physrevb.47.12004.

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38

DUTRA, M., O. LOURENÇO, A. DELFINO e J. S. SÁ MARTINS. "SKYRME MODELS AND NUCLEAR MATTER PROPERTIES". International Journal of Modern Physics D 19, n.º 08n10 (agosto de 2010): 1583–86. http://dx.doi.org/10.1142/s0218271810017937.

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In this preliminary study we select a set of six Skyrme models which present reasonable symmetry energies lying in the range of 28–35 MeV to analyze the behavior of several other bulk properties at zero temperature, as well as the critical temperature parameters. The models are also investigated to see whether they satisfy a stringent constraint recently proposed from heavy-ion experiments.

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39

Carollo, C. Marcella, I. John Danziger, R. Michael Rich e Xinzhong Chen. "Nuclear Properties of Kinematically Distinct Cores". Astrophysical Journal 491, n.º 2 (20 de dezembro de 1997): 545–60. http://dx.doi.org/10.1086/304979.

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40

Chiotti, Premo. "Thorium dioxide: Properties and nuclear applications". Journal of Nuclear Materials 136, n.º 2-3 (novembro de 1985): 290. http://dx.doi.org/10.1016/0022-3115(85)90019-4.

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41

Audi, G., F. G. Kondev, Meng Wang, W. J. Huang e S. Naimi. "The NUBASE2016 evaluation of nuclear properties". Chinese Physics C 41, n.º 3 (março de 2017): 030001. http://dx.doi.org/10.1088/1674-1137/41/3/030001.

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42

Connelly, A. J., R. J. Hand, P. A. Bingham e N. C. Hyatt. "Mechanical properties of nuclear waste glasses". Journal of Nuclear Materials 408, n.º 2 (janeiro de 2011): 188–93. http://dx.doi.org/10.1016/j.jnucmat.2010.11.034.

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43

Abd-Alla, M., S. Ramadan e M. Y. M. Hassan. "Thermostatic properties of polarized nuclear matter". Physical Review C 36, n.º 4 (1 de outubro de 1987): 1565–72. http://dx.doi.org/10.1103/physrevc.36.1565.

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44

Schmidt, E. O., D. Ferreiro, L. Vega Neme e G. A. Oio. "Spectral nuclear properties of NLS1 galaxies". Astronomy & Astrophysics 596 (dezembro de 2016): A95. http://dx.doi.org/10.1051/0004-6361/201629343.

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45

Jiang, M. F., e T. T. S. Kuo. "Thermodynamic properties of superconducting nuclear matter". Nuclear Physics A 481, n.º 2 (maio de 1988): 294–312. http://dx.doi.org/10.1016/0375-9474(88)90498-8.

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46

Kiderlen, D., H. Hofmann e F. A. Ivanyuk. "Dynamical aspects of thermal nuclear properties". Nuclear Physics A 550, n.º 3 (dezembro de 1992): 473–506. http://dx.doi.org/10.1016/0375-9474(92)90019-g.

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47

Hassan, Israa M., e Freed M. Mohammed. "Employing Some of Nuclear Models to Study the Energy Levels of Odd Atomic Mass Nuclei". NeuroQuantology 20, n.º 3 (26 de março de 2022): 182–86. http://dx.doi.org/10.14704/nq.2022.20.3.nq22058.

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The energy levels and their Gamma Transitions for the nuclei are important characteristics for identify its properties, and the moment of inertia is one of the important parameters in determining energy levels. accordingly many nuclear models have been developed in successive periods of time for this study, according to the movement of the nuclei. The energy levels were calculated for all values of the total nuclear momentum and parity by applying the nuclear shell model and the Generalized Variable Moment of Inertia with the addition of some limits in order to obtain accurate and inclusive results for all Nuclei. In This paper we have include nuclie whom their energy levels have not previously been studied theoretically and for which only experimental data are available and these Nuclei are: (11Na27, 26Fe59, 35Br79, 40Zr81, 39Y91, 38Sr97, 49In107 48Cd121, 77Ir191, 89Ac221) and this model was designed with a developed program (Matlab-2020) and the results were compared with the practical data and they were in good agreement.

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48

Denikin, Andrey, Alexander Karpov, Mikhail Naumenko, Vladimir Rachkov, Viacheslav Samarin e Vycheslav Saiko. "Synergy of Nuclear Data and Nuclear Theory Online". EPJ Web of Conferences 239 (2020): 03021. http://dx.doi.org/10.1051/epjconf/202023903021.

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The paper describes the NRV web knowledge base on low-energy nuclear physics developed in the Joint Institute for Nuclear Research. The NRV knowledge base working through the Internet integrates a large amount of digitized experimental data on the properties of nuclei and nuclear reaction cross sections with a wide range of computational programs for modeling of nuclear properties and nuclear dynamics. Today, the NRV becomes a powerful instrument for nuclear physics research as well as for educational applications. Advantages of the functioning scheme of the knowledge base provide the synergy of coexistence of the experimental data and computational codes within one platform.

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49

SANTRA, A. B., e U. LOMBARDO. "SIGMA MESON AND PROPERTIES OF NUCLEAR MATTER". International Journal of Modern Physics E 18, n.º 05n06 (junho de 2009): 1191–205. http://dx.doi.org/10.1142/s0218301309013440.

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We have calculated the saturation observables of symmetric nuclear matter and nuclear symmetry energy in the framework of Brueckner-Hartree-Fock (BHF) formalism with Bonn-B potential as two-body interaction, including modification of hadronic parameter inside nuclear medium. We have found that it is possible to understand all the saturation observables of symmetric nuclear matter by incorporating in-medium modification of the parameters of sigma meson alone. Linear density dependent reduction of σ-nucleon coupling constant by about 6.8% and density independent reduction σ-meson mass by about 3.5% is sufficient to understand nuclear matter saturation observables. We find with the calculated symmetry energy that neutron skin thickness of 208Pb is 0.20 fm and the radius of 1.4 solar mass neutron stars as 11.98 ± 0.75 km.

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50

Rożynek, Jacek. "Nucleon properties inside the compressed nuclear matter". International Journal of Modern Physics E 27, n.º 04 (abril de 2018): 1850030. http://dx.doi.org/10.1142/s0218301318500301.

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In this work, we show the modifications of nucleon mass and nucleon radius with the help of the extended Relativistic Mean Field (RMF) model. We argue that even small departures above nuclear equilibrium density with constant nucleon mass require an energy transfer from the repulsive mean field to the quarks forming nucleon massive bags in Nuclear Matter (NM), together with the decrease in the nucleon volume. The transfer, which is proportional to pressure and absent in a standard RMF approach, provides good values for nuclear compressibility, symmetry energy and its slope. Different courses of the Equation of State (EOS), which depend on the energy transfer, are considered.

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