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Zeitschriftenartikel zum Thema „Nuclear properties“

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Veröffentlicht am 15. Februar 2025

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1

Chung, K. C., C. S. Wang und A. J. Santiago. „Nuclear matter properties from nuclear masses“. Europhysics Letters (EPL) 47, Nr. 6 (15.09.1999): 663–67. http://dx.doi.org/10.1209/epl/i1999-00440-4.

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2

Poenaru, D. N., W. Greiner und E. Hourani. „C12emission fromBa114and nuclear properties“. Physical Review C 51, Nr. 2 (01.02.1995): 594–600. http://dx.doi.org/10.1103/physrevc.51.594.

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3

PASSAMANI, TOMAZ, und MARIA LUIZA CESCATO. „HOT NUCLEAR MATTER PROPERTIES“. International Journal of Modern Physics E 16, Nr. 09 (Oktober 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 und Soo-Jin Park. „Nuclear Graphites (II) : Mechanical Properties“. Carbon letters 11, Nr. 1 (30.03.2010): 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 (01.10.2008): 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 und Gy Wolf. „Resonance properties in nuclear matter“. Physical Review C 47, Nr. 6 (01.06.1993): R2467—R2469. http://dx.doi.org/10.1103/physrevc.47.r2467.

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7

Akaishi, Yoshinori, Akinobu Doté und 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 (01.04.2006): 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 und V. K. Milinchuk. „Refractive properties of nuclear microfilters“. Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms 155, Nr. 3 (August 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 und M. MacCormick. „NUBASE2012 Evaluation of Nuclear Properties“. Nuclear Data Sheets 120 (Juni 2014): 6–7. http://dx.doi.org/10.1016/j.nds.2014.06.127.

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12

Baldo, M., und G. F. Burgio. „Properties of the nuclear medium“. Reports on Progress in Physics 75, Nr. 2 (09.01.2012): 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, Nr. 1 (01.01.2013): 37–59. http://dx.doi.org/10.3844/pisp.2013.37.59.

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14

LEJEUNE, A., J. CUGNON und P. GRANGE. „PROPERTIES OF HOT NUCLEAR MATTER“. Le Journal de Physique Colloques 47, Nr. C4 (August 1986): C4–373—C4–376. http://dx.doi.org/10.1051/jphyscol:1986442.

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15

Wendler, W., P. Smeibidl und F. Pobell. „Nuclear magnetic properties of aluminium“. Journal of Low Temperature Physics 108, Nr. 3-4 (August 1997): 291–304. http://dx.doi.org/10.1007/bf02398716.

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16

Close, F. E., R. G. Roberts und G. G. Ross. „Nuclear properties from perturbative QCD“. Physics Letters B 168, Nr. 4 (März 1986): 400–404. http://dx.doi.org/10.1016/0370-2693(86)91652-7.

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17

Benhar, Omar, Alessandro Lovato und Lucas Tonetto. „Properties of Hot Nuclear Matter“. Universe 9, Nr. 8 (25.07.2023): 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 und T. Yu Tretyakova. „Nuclear shell structure in the systematics of nuclear properties“. Bulletin of the Russian Academy of Sciences: Physics 78, Nr. 5 (Mai 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, Nr. 2 (29.02.2016): 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 (Juli 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 (03.07.2015): 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, Nr. 1-2 (Dezember 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, Nr. 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, Nr. 2 (01.02.2009): 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 und V. I. Seledtsov. „Antitumor properties of nuclear erythroid cells“. Siberian journal of oncology 21, Nr. 3 (29.06.2022): 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 (17.04.2013): 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, Nr. 09 (September 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 und J. Hiura. „Properties of Hot Asymmetric Nuclear Matter“. Progress of Theoretical Physics 92, Nr. 1 (01.07.1994): 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, Nr. 2 (Februar 1987): 309. http://dx.doi.org/10.13182/nt87-a33886.

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31

Carbone, Arianna, und Omar Benhar. „Transport properties ofβ-stable nuclear matter“. Journal of Physics: Conference Series 336 (28.12.2011): 012015. http://dx.doi.org/10.1088/1742-6596/336/1/012015.

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32

Hayano, Ryugo S., und Tetsuo Hatsuda. „Hadron properties in the nuclear medium“. Reviews of Modern Physics 82, Nr. 4 (27.10.2010): 2949–90. http://dx.doi.org/10.1103/revmodphys.82.2949.

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33

Von-Eiff, D., W. Stocker und M. K. Weigel. „Relativistic investigation of nuclear surface properties“. Physical Review C 50, Nr. 3 (01.09.1994): 1436–44. http://dx.doi.org/10.1103/physrevc.50.1436.

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34

Dickhoff, W. H., und H. Muther. „Nucleon properties in the nuclear medium“. Reports on Progress in Physics 55, Nr. 11 (01.11.1992): 1947–2023. http://dx.doi.org/10.1088/0034-4885/55/11/002.

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35

Starosta, K., I. Hamamoto, T. Koike und C. Vaman. „Electromagnetic properties of nuclear chiral partners“. Physica Scripta T125 (28.06.2006): 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 und M. MacCormick. „The Nubase2012 evaluation of nuclear properties“. Chinese Physics C 36, Nr. 12 (Dezember 2012): 1157–286. http://dx.doi.org/10.1088/1674-1137/36/12/001.

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37

Rapp, R. E., und H. Godfrin. „Nuclear magnetic properties ofHe3adsorbed on graphite“. Physical Review B 47, Nr. 18 (01.05.1993): 12004–17. http://dx.doi.org/10.1103/physrevb.47.12004.

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38

DUTRA, M., O. LOURENÇO, A. DELFINO und J. S. SÁ MARTINS. „SKYRME MODELS AND NUCLEAR MATTER PROPERTIES“. International Journal of Modern Physics D 19, Nr. 08n10 (August 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 und Xinzhong Chen. „Nuclear Properties of Kinematically Distinct Cores“. Astrophysical Journal 491, Nr. 2 (20.12.1997): 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, Nr. 2-3 (November 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 und S. Naimi. „The NUBASE2016 evaluation of nuclear properties“. Chinese Physics C 41, Nr. 3 (März 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 und N. C. Hyatt. „Mechanical properties of nuclear waste glasses“. Journal of Nuclear Materials 408, Nr. 2 (Januar 2011): 188–93. http://dx.doi.org/10.1016/j.jnucmat.2010.11.034.

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43

Abd-Alla, M., S. Ramadan und M. Y. M. Hassan. „Thermostatic properties of polarized nuclear matter“. Physical Review C 36, Nr. 4 (01.10.1987): 1565–72. http://dx.doi.org/10.1103/physrevc.36.1565.

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44

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

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45

Jiang, M. F., und T. T. S. Kuo. „Thermodynamic properties of superconducting nuclear matter“. Nuclear Physics A 481, Nr. 2 (Mai 1988): 294–312. http://dx.doi.org/10.1016/0375-9474(88)90498-8.

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46

Kiderlen, D., H. Hofmann und F. A. Ivanyuk. „Dynamical aspects of thermal nuclear properties“. Nuclear Physics A 550, Nr. 3 (Dezember 1992): 473–506. http://dx.doi.org/10.1016/0375-9474(92)90019-g.

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47

Hassan, Israa M., und Freed M. Mohammed. „Employing Some of Nuclear Models to Study the Energy Levels of Odd Atomic Mass Nuclei“. NeuroQuantology 20, Nr. 3 (26.03.2022): 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 und 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., und U. LOMBARDO. „SIGMA MESON AND PROPERTIES OF NUCLEAR MATTER“. International Journal of Modern Physics E 18, Nr. 05n06 (Juni 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, Nr. 04 (April 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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