Relevant bibliographies by topics / Relativistic mean field

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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 'Relativistic mean field'

Author: Grafiati
Published: 25 January 2025

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Journal articles on the topic "Relativistic mean field"

1

Afanasjev, A. V. "Superdeformations in Relativistic and Non-Relativistic Mean Field Theories." Physica Scripta T88, no. 1 (2000): 10. http://dx.doi.org/10.1238/physica.topical.088a00010.

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Wang, S. J., and W. Cassing. "Extended relativistic mean field theory and relativistic transport equations." Nuclear Physics A 495, no. 1-2 (April 1989): 371–80. http://dx.doi.org/10.1016/0375-9474(89)90334-5.

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Rego, R. A. "Mean free path in the relativistic mean field." Physical Review C 44, no. 5 (November 1, 1991): 1944–46. http://dx.doi.org/10.1103/physrevc.44.1944.

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ROTA NODARI, SIMONA. "THE RELATIVISTIC MEAN-FIELD EQUATIONS OF THE ATOMIC NUCLEUS." Reviews in Mathematical Physics 24, no. 04 (May 2012): 1250008. http://dx.doi.org/10.1142/s0129055x12500080.

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In nuclear physics, the relativistic mean-field theory describes the nucleus as a system of Dirac nucleons which interact via meson fields. In a static case and without nonlinear self-coupling of the σ meson, the relativistic mean-field equations become a system of Dirac equations where the potential is given by the meson and photon fields. The aim of this work is to prove the existence of solutions of these equations. We consider a minimization problem with constraints that involve negative spectral projectors and we apply the concentration-compactness lemma to find a minimizer of this problem. We show that this minimizer is a solution of the relativistic mean-field equations considered.
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Del Zanna , Luca, Niccolò Tomei, Kevin Franceschetti, Matteo Bugli, and Niccolò Bucciantini. "General Relativistic Magnetohydrodynamics Mean-Field Dynamos." Fluids 7, no. 2 (February 21, 2022): 87. http://dx.doi.org/10.3390/fluids7020087.

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Large-scale, ordered magnetic fields in several astrophysical sources are supposed to be originated, and maintained against dissipation, by the combined amplifying action of rotation and small-scale turbulence. For instance, in the solar interior, the so-called α−Ω mean-field dynamo is known to be responsible for the observed 22-years magnetic cycle. Similar mechanisms could operate in more extreme environments, like proto neutron stars and accretion disks around black holes, for which the physical modelling needs to be translated from the regime of magnetohydrodynamics (MHD) and Newtonian gravity to that of a plasma in a general relativistic curved spacetime (GRMHD). Here we review the theory behind the mean field dynamo in GRMHD, the strategies for the implementation of the relevant equations in numerical conservative schemes, and we show the most important applications to the mentioned astrophysical compact objects obtained by our group in Florence. We also present novel results, such as three-dimensional GRMHD simulations of accretion disks with dynamo and the application of our dynamo model to a super massive neutron star, remnant of a binary neutron star merger as obtained from full numerical relativity simulations.
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Diakonov, Dmitri. "Relativistic mean field approximation to baryons." European Physical Journal A 24, S1 (February 2005): 3–8. http://dx.doi.org/10.1140/epjad/s2005-05-001-3.

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WARRIER, LATHA S., J. P. MAHARANA, and Y. K. GAMBHIR. "ALPHA STAGGERING: RELATIVISTIC MEAN FIELD DESCRIPTION." Modern Physics Letters A 09, no. 26 (August 30, 1994): 2371–80. http://dx.doi.org/10.1142/s0217732394002240.

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The α-staggering for the nuclei in the 2p−1f region is investigated in the relativistic mean field approach. The observed behavior similar to the well known odd-even staggering is well reproduced. The decomposition of densities for these nuclei shows almost identical characteristics beyond the rms radii indicating that the alpha cluster, if exists, is confined to the surface, as expected.
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Gambhir, Y. K., and A. Bhagwat. "Relativistic mean field for nuclear periphery." Nuclear Physics A 722 (July 2003): C354—C359. http://dx.doi.org/10.1016/s0375-9474(03)01389-7.

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Fogaça, D. A., and F. S. Navarra. "Solitons in relativistic mean field models." Physics Letters B 639, no. 6 (August 2006): 629–34. http://dx.doi.org/10.1016/j.physletb.2006.07.002.

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BARRIOS, S. CRUZ, and M. C. NEMES. "ANATOMY OF RELATIVISTIC MEAN-FIELD APPROXIMATIONS." Modern Physics Letters A 07, no. 21 (July 10, 1992): 1915–21. http://dx.doi.org/10.1142/s0217732392001622.

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In the present work we have set up a scheme to treat field theoretical Lagrangians in the same bases of the well known non-relativistic many-body techniques. We show here that fermions and bosons can be treated quantum mechanically in a symmetric way and obtain results for the mean field approximation.
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Dissertations / Theses on the topic "Relativistic mean field"

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Centelles, Aixalà Mario. "Semiclassical approach to relativistic nuclear mean field theory." Doctoral thesis, Universitat de Barcelona, 1992. http://hdl.handle.net/10803/1593.

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The nuclear many-body problem is nowadays being increasingly approached on the basis of a relativistic formalism. Microscopic Dirac-Brueckner-Hartree-Fock (DBHF) calculations starting from a realistic nucleon-nucleon interaction seem to be very promising. In the theory of quantum hadrodynamics, nucleons interact through the exchange of virtual mesons and the dynamics is specified by Lorentz covariant Lagrangian densities. In the simplest version, only a vector field (associated with the w meson) accounting for short-range repulsion and a scalar field ("sygma" meson) responsible for attraction are needed to describe saturation in nuclear matter. Calculations in mean field Hartree approximation, neglecting exchange terms and without including any contribution from antiparticles, give an accurate description of many of the features of nuclear systems.

The success of semi-classical models in non-relativistic nuclear physics provides a very strong motivation for investigating similar methods in the relativistic context, where only the pure Thomas-Fermi approximation had been studied. In this thesis we set up the semi-classical expansion in relativistic nuclear mean field theory, including gradient corrections of order h(2) to the Thomas-Fermi model, and investigate several applications to nuclear systems.

On the basis of Wigner transform techniques, a. recursive scheme to obtain the semi-classical h(2) expansion of the propagator associated with a time-independent single-particle Hamiltonian with matrix structure is presented. We focus our attention on the application of the method to a Dirac Hamiltonian related to relativistic nuclear mean field theory, i.e., including a position-dependent effective mass and the time-like component of a. four-vector field. Compared with the non-relativistic case, the procedure is considerably more complicated owing to the matrix structure of the Hamiltonian. For this reason the "h", expansion is pushed to order h(2) only. A detailed derivation is given of the h(2)-order Wigner-Kirkwood expansion of the relativistic density matrix, in terms of the gradients of the vector and the scalar field, as well as of the expansion of the particle and energy densities. The idempotency of the semi-classical density matrix to second order in "h" is proven. The Wigner-Kirkwood expressions, as they stand, are not suitable to be employed in a self-consistent problem. Therefore, we obtain the corresponding density functional results. In this case the energy densities are expressed as a functional of the local density, the effective mass and their gradients.

The accuracy of the Wigner-Kirkwood series is tested on a. relativistic harmonic oscillator and perfect agreement with the Strutinsky averaged observables is found even in the highly relativistic regime. The density functional version is shown to be slightly less accurate, a feature already known in the non-relativistic case. It turns out that the semi-classical expressions represent the different quantities on average, that is, quantum fluctuations are averaged out. This model study shows that, for positive energy states, the derived semi-classical expansions contain all the relativistic ingredients, the difference with quantal results being due mainly to shell effects.

Extended Thomas-Fermi calculations, which· include h(2)-order gradient corrections, are performed for relativistic non-linear "sigma"- "omega" models using two kinds of Lagrangians which differ in the form of the scalar coupling for the isoscalar sigma meson. Comparing the semi-classical results of order h(2) (TFh(2)) with the Hartree results, we find that the TFh(2) approximation yields some underbinding when the effective mass (mº) of the model is small, and some overbinding when mº is large. For a value around mº/m = 0.65, both TFh(2) and Hartree would roughly yield the same binding energy. However, since semi-classical and quantal results must differ in the so-called shell energy, this indicates that it is not properly estimated by the TFh(2) approximation.

When the h(2)-order gradient corrections are taken into account (TFh(2), we have found a numerical instability in the solution of the semi-classical Klein-Gordon equation obeyed by the scalar field in the case of parameterizations which have mº/m
Second-order corrections in "h" to the TFh(0) approximation improve the agreement with Hartree solutions in a sensitive way, always yielding more bound nuclei than within the Hartree approach. The sign of the h(2) corrections depends on mº, and they are found to vanish around mº/m = 0.75 for the models of the type considered here. In several respects, the semi-classical relativistic phenomenology quite resembles the one met in the non-relativistic regime using Skyrme forces, in spite of the different origin of mº in both situations. Extending the so-called expectation value method to the relativistic problem, and using the TFh(2) semi-classical mean field as a starting point, perturbative quantal solutions are found which are in good agreement with the Hartree results.

The semi-classical TFh(0) and TFh(2) density distributions do not present oscillations due to the absence of shell effects, but they average the Hartree results. In the interior of the nucleus the TFh(0) and TF1i2 densities are very similar. However, in the surface and the outer region the TF1i2 densities come appreciably closer than TFh(0) to the Hartree results, due to the gradient corrections incorporated by the TF1i2 functionals, and show an exponential drop off.

Liquid drop model coefficients are calculated for some parameter sets of the "sygma-omega" model. We have found reasonable results for the surface thickness and for the surface and curvature energies, which are within the range of the values obtained in non-relativistic calculations using density-dependent Skyrme forces. Therefore, the relativistic effects do not seem to avoid the disagreement of the calculated value of the curvature energy with the empirical value.

In this work we also study the effects of the density-dependent Dirac spinor for the nucleons, as is determined microscopically in the DBHF approach, on various properties of the structure and scattering of finite nuclei. To enable this, we construct a relativistic energy density functional that contains the semi-classical kinetic energy density of order h(2). The effective mass and the volume term in the potential energy arise from a DBHF calculation of nuclear matter. This volume term is supplemented by some conventional correction terms and the few free parameters are suitably adjusted. It turns out that the radii of nuclei calculated with the present approach agree better with the experimental value than those obtained in similar studies using a potential energy derived from a non-relativistic G-matrix. This demonstrates that the Dirac effects improve the calculation of ground-state properties of finite nuclei also in our relativistic extended Thomas-Fermi (RETF) approximation.

However, this study of ground-state properties is not the main goal of our investigation.
The capabilities of our RETF functional are actually appraised in situations in which a full microscopic relativistic calculation, or even a phenomenological one, cannot be easily made, such as nuclear fission of rotating nuclei and heavy ion scattering. In these situations, the method constitutes a reliable tool. For the nuclear fission barriers, the present calculations are the first ones carried out with a relativistic model. We have shown that the model yields results comparable to the non-relativistic ones, with the conceptual-advantage of being relativistic and thus automatically incorporating the spin-orbit force. For the calculations of heavy ion elastic scattering cross sections, we have been able to improve previous results due to achieving a better description of the nuclear, densities.

Let us summarize the two apparent merits which the TFh(2) approximation has over the simple TFh(0) one. On the one hand, it provides fully variational densities that go exponential to zero. On the other hand, it takes into account non-local spin-orbit and effective mass contributions up to order h(2), yielding a more reliable average value.
Se establece el desarrollo semi-clásico hasta orden h(2) en la teoría nuclear relativista de campo medio. Así, se obtienen las densidades semi-clásicas relativistas de partículas y de energía para un conjunto de fermiones sometidos a un campo escalar y a un campo vector, en las teorías de campo medio de Wigner-Kirkwood y de Thomas-Fermi, incluyendo correcciones en gradientes hasta orden h(2). El método semi-clásico se aplica a un oscilador armónico relativista. Después se utiliza en modelos T-W no lineales, para los cuales se resuelven las ecuaciones variacionales en núcleos finitos y en materia nuclear semi-infinita. Los resultados semi-clásicos son comparados con los correspondientes resultados cuánticos Hartree.

Para estudiar los efectos de los espinores de Dirac para los nucleones sobre diversas propiedades de la estructura y de la dispersión de núcleos finitos, se construye un funcional de la densidad de energía relativista. El funcional contiene la densidad de energía cinética relativista de orden h(2). La masa efectiva y la parte potencial se obtienen a partir de cálculos Dirac-Brueckner de materia nuclear. Se presta especial atención al cálculo de barreras de fisión de núcleos en rotación y del potencial óptico para la dispersión de iones pesados a energías intermedias.
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Ban, Shufang. "Investigation of effective interactions in relativistic mean field theory." Licentiate thesis, Stockholm, 2005. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-4074.

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姚昌銓 and Cheong-chuen Yao. "Properties of neutron stars in the relativistic mean field theory." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1996. http://hub.hku.hk/bib/B30409135.

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Yao, Cheong-chuen. "Properties of neutron stars in the relativistic mean field theory /." Hong Kong : University of Hong Kong, 1996. http://sunzi.lib.hku.hk/hkuto/record.jsp?B19668867.

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Paar, Nils. "Relativistic mean field description of exotic excitations in finite nuclei." [S.l. : s.n.], 2003. http://deposit.ddb.de/cgi-bin/dokserv?idn=969358199.

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Diener, Jacobus Petrus Willem. "Relativistic mean-field theory applied to the study of neutron star properties." Thesis, Link to the online version, 2008. http://hdl.handle.net/10019/760.

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Acar, Fatma. "Spinodal Instabilities In Symmetric Nuclear Matter Within A Nonlinear Relativistic Mean-field Approach." Master's thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613472/index.pdf.

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Spinodal instability mechanism and early development of density fluctuations for symmetric nuclear matter at finite temperature are studied. A stochastic extension of Walecka-type relativistic mean-field model including non-linear self-interactions of scalar mesons with NL3 parameter set is employed in the semi-classical approximation. The growth rates of unstable collective modes are investigated below the normal density and at low temperatures. The system exhibits most unstable behavior in longer wave lengths at baryon densities &rho
B = 0.4 &rho
0 , while most unstable behavior occurs in shorter wavelengths at lower baryon densities &rho
B = 0.2 &rho
0 . The unstable response of the system shifts towards longer wavelengths with the increasing temperature at both densities. The early growth of the density correlation functions are calculated, which provide valuable information about the initial size of the condensation and the average speed of condensing fragments. Furthermore, the relativistic results are compared with Skyrme type non-relativistic calculations. Qualitatively similar results are found in both non-relativistic and relativistic descriptions.
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Danisman, Betul. "Spinodal Instabilities In Symmetric Nuclear Matter Within A Density-dependent Relativistic Mean-field Approach." Master's thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613473/index.pdf.

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The nuclear matter liquid-gas phase transition is expected to be a signal of nuclear spinodal instabilities as a result of density fluctuations. Nuclear spinodal instabilities in symmetric nuclear matter are studied within a stochastic relativistic density-dependent model in semi-classical approximation. We use two parameterization for the Lagrange density, DDME1 and TW sets. The early growth of density fluctuations is investigated by employing relativistic Vlasov equation based on QHD and discussed the cluster size of the condensations from the early growth of density correlation functions. Expectations are that hot nuclear matter behaves unstable around &rho
b &asymp
&rho
0/4 (below the saturation density) and at low temperatures. We therefore present our results at low temperature T=1 MeV and at higher temperature T=5 MeV, and also at a lower initial baryon density &rho
b = 0.2 &rho
0 and a higher value &rho
b = 0.4 &rho
0 where unstable behavior is within them. Calculations in density-dependent model are compared with the other calculations obtained in a relativistic non-linear model and in a Skyrme type nonivrelativistic model. Our results are consistent with them. Qualitatively similar results show that the physics of the quantities are model-independent. The size of clusterization is estimated in two ways, by using half-wavelength of the most unstable mode and from the width of correlation function at half maximum. Furthermore, the average speed of condensing fragments during the initial phase of spinodal decomposition are determined by using the current density correlation functions.
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Voskresenskaya, Maria Verfasser], Karlheinz [Akademischer Betreuer] [Langanke, and Robert [Akademischer Betreuer] Roth. "Correlations in nuclear matter at low densities in an extended relativistic mean-field model / Maria Voskresenskaya. Betreuer: Karlheinz Langanke ; Robert Roth." Darmstadt : Universitäts- und Landesbibliothek Darmstadt, 2013. http://d-nb.info/1106454383/34.

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Voskresenskaya, Maria [Verfasser], Karlheinz [Akademischer Betreuer] Langanke, and Robert [Akademischer Betreuer] Roth. "Correlations in nuclear matter at low densities in an extended relativistic mean-field model / Maria Voskresenskaya. Betreuer: Karlheinz Langanke ; Robert Roth." Darmstadt : Universitäts- und Landesbibliothek Darmstadt, 2013. http://nbn-resolving.de/urn:nbn:de:tuda-tuprints-33606.

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Books on the topic "Relativistic mean field"

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Bednarek, Ilona. Relativistic mean field models of neutron stars. Katowice: Wydawn. Uniwersytetu Śla̜skiego, 2007.

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Bednarek, Ilona. Relativistic mean field models of neutron stars. Katowice: Wydawn. Uniwersytetu Śla̜skiego, 2007.

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Rutz, Klemens. Struktur von Atomkernen im Relativistic-Mean-Field-Modell. Ibidem Verlag, 1999.

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Triaxial deformation of unstable nuclei in the relativistic mean field theory. Wako, Saitama, Japan: Institute of Physical and Chemical Research (RIKEN), 1996.

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Freeman, Richard R., James A. King, and Gregory P. Lafyatis. Electromagnetic Radiation. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198726500.001.0001.

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Electromagnetic Radiation is a graduate level book on classical electrodynamics with a strong emphasis on radiation. This book is meant to quickly and efficiently introduce students to the electromagnetic radiation science essential to a practicing physicist. While a major focus is on light and its interactions, topics in radio frequency radiation, x-rays, and beyond are also treated. Special emphasis is placed on applications, with many exercises and homework problems. The format of the book is designed to convey the basic concepts of a topic in the main central text in the book in a mathematically rigorous manner, but with detailed derivations routinely relegated to the accompanying side notes or end of chapter “Discussions.” The book is composed of four parts: Part I is a review of basic E&M, and assumes the reader has a had a good upper division undergraduate course, and while it offers a concise review of topics covered in such a course, it does not treat any given topic in detail; specifically electro- and magnetostatics. Part II addresses the origins of radiation in terms of time variations of charge and current densities within the source, and presents Jefimenko’s field equations as derived from retarded potentials. Part III introduces special relativity and its deep connection to Maxwell’s equations, together with an introduction to relativistic field theory, as well as the relativistic treatment of radiation from an arbitrarily accelerating charge. A highlight of this part is a chapter on the still partially unresolved problem of radiation reaction on an accelerating charge. Part IV treats the practical problems of electromagnetic radiation interacting with matter, with chapters on energy transport, scattering, diffraction and finally an illuminating, application-oriented treatment of fields in confined environments.
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Baulieu, Laurent, John Iliopoulos, and Roland Sénéor. From Classical to Quantum Fields. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198788393.001.0001.

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Quantum field theory has become the universal language of most modern theoretical physics. This book is meant to provide an introduction to this subject with particular emphasis on the physics of the fundamental interactions and elementary particles. It is addressed to advanced undergraduate, or beginning graduate, students, who have majored in physics or mathematics. The ambition is to show how these two disciplines, through their mutual interactions over the past hundred years, have enriched themselves and have both shaped our understanding of the fundamental laws of nature. The subject of this book, the transition from a classical field theory to the corresponding Quantum Field Theory through the use of Feynman’s functional integral, perfectly exemplifies this connection. It is shown how some fundamental physical principles, such as relativistic invariance, locality of the interactions, causality and positivity of the energy, form the basic elements of a modern physical theory. The standard theory of the fundamental forces is a perfect example of this connection. Based on some abstract concepts, such as group theory, gauge symmetries, and differential geometry, it provides for a detailed model whose agreement with experiment has been spectacular. The book starts with a brief description of the field theory axioms and explains the principles of gauge invariance and spontaneous symmetry breaking. It develops the techniques of perturbation theory and renormalisation with some specific examples. The last Chapters contain a presentation of the standard model and its experimental successes, as well as the attempts to go beyond with a discussion of grand unified theories and supersymmetry.
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Book chapters on the topic "Relativistic mean field"

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Reinhard, P. G., and M. Bender. "9 Mean Field: Relativistic versus Non-relativistic." In Extended Density Functionals in Nuclear Structure Physics, 249–68. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39911-7_9.

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Jaminon, M., and C. Mahaux. "Critical survey of relativistic mean field approaches." In Medium Energy Nucleon and Antinucleon Scattering, 479–96. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-16054-x_188.

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Savushkin, Lev N., and Hiroshi Toki. "The Relativistic Mean-Field Approximation for Nuclear Structure." In The Atomic Nucleus as a Relativistic System, 39–74. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-10309-8_4.

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Ginocchio, Joseph N. "7 Symmetry in the Relativistic Mean Field Approximation." In Extended Density Functionals in Nuclear Structure Physics, 219–37. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39911-7_7.

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Mareš, J. "Hyperon(S) in the Relativistic Mean Field Theory." In Mesons and Light Nuclei, 423–29. Vienna: Springer Vienna, 1992. http://dx.doi.org/10.1007/978-3-7091-7617-7_54.

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Afanasjev, A. V., S. G. Frauendorf, and P. Ring. "Rotating Nuclei in the Relativistic Mean Field Theory." In The Nuclear Many-Body Problem 2001, 103–10. Dordrecht: Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0460-2_14.

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Centelles, M. "Density Functional Formalism in Relativistic Nuclear Mean Field Theory." In NATO ASI Series, 173–89. Boston, MA: Springer US, 1995. http://dx.doi.org/10.1007/978-1-4757-9975-0_8.

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Estal, M., M. Centelles, X. Viñas, and S. K. Patra. "Pairing Properties in Relativistic Mean Field Models Based on Effective Field Theory." In The Nuclear Many-Body Problem 2001, 175–80. Dordrecht: Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0460-2_24.

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Reinhard, P. G., H. G. Döbereiner, V. Blum, J. Fink, M. Rufa, J. Maruhn, H. Stöcker, and W. Greiner. "The Relativistic Mean-Field Model of Nuclear Structure and Dynamics." In The Nuclear Equation of State, 635–47. Boston, MA: Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-0583-5_50.

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Typel, S., and H. H. Wolter. "Relativistic Mean Field Approach with Density and Momentum-Dependent Coupling Vertices." In The Nuclear Many-Body Problem 2001, 89–96. Dordrecht: Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0460-2_12.

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Conference papers on the topic "Relativistic mean field"

1

Taurines, Andre R., Cesar A. Z. Vasconcellos, and Manuel Malheiro. "Naturalness in relativistic mean field theories." In Proceedings of the International Workshop. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811653_0038.

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Toki, Hiroshi. "RELATIVISTIC MEAN FIELD THEORY AND SPIN EXCITATIONS." In Proceedings of the RCNP-TMU Symposium. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792297_0011.

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LEJA, J., and Š. GMUCA. "RELATIVISTIC MEAN-FIELD DESCRIPTION OF LIGHT NUCLEI." In Proceedings of the 6th International Conference. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812837530_0027.

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Sulaksono, A., P. T. P. Hutauruk, C. K. Williams, and T. Mart. "Relativistic Mean Field Models at High Densities." In Proceedings of the 3rd Asia-Pacific Conference. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812706881_0068.

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AFANASJEV, A. V. "RELATIVISTIC MEAN FIELD STUDIES OF SUPERHEAVY NUCLEI." In Proceedings of the Fourth International Conference. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812833433_0040.

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LALAZISSIS, G. A., D. VRETENAR, N. PAAR, and P. RING. "RELATIVISTIC MEAN-FIELD DESCRIPTION OF EXOTIC NUCLEAR STRUCTURE." In Proceedings of the 5th International Conference. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776723_0032.

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Moszkowski, S. A. "Relativistic nuclear mean field and equation of state." In Strong, weak, and electromagnetic interactions in nuclei, atoms, and astrophysics. AIP, 1991. http://dx.doi.org/10.1063/1.41437.

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Soares, Bruno Alves de Moura, César Henrique Lenzi, and Mariana Dutra. "Relativistic Mean Field Model constrained by Astrophysical Measurements." In XV International Workshop on Hadron Physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.408.0033.

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Dutra, M., O. Lourenço, B. V. Carlson, A. Delfino, D. P. Menezes, S. S. Avancini, J. R. Stone, C. Provide^ncia, and S. Typel. "Relativistic mean-field models and nuclear matter constraints." In XXXV BRAZILIAN WORKSHOP ON NUCLEAR PHYSICS. AIP, 2013. http://dx.doi.org/10.1063/1.4804125.

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Gangopadhyay, G., Madhubrata Bhattacharya, and Subinit Roy. "Relativistic mean field calculations in neutron-rich nuclei." In FRONTIERS IN GAMMA-RAY SPECTROSCOPY 2012 - FIG12. AIP Publishing LLC, 2014. http://dx.doi.org/10.1063/1.4893254.

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Reports on the topic "Relativistic mean field"

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Glendenning, N. K., D. Von-Eiff, M. Haft, H. Lenske, and M. K. Weigel. Relativistic mean-field calculations of {Lambda} and {Sigma} hypernuclei. Office of Scientific and Technical Information (OSTI), October 1992. http://dx.doi.org/10.2172/10163884.

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