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Názov Charged rho-meson condensation in neutron stars Aut.údaje Evgeni E. Kolomeitsev, K. A. Maslov ... [et al.] Autor Kolomeitsev Evgeni E. 1970- (34%) UMBFP06 - Katedra fyziky
Spoluautori Maslov K. A. (33%)
Voskresensky Dmitri (33%)
Zdroj.dok. Nuclear Physics A. Vol. 970, (2018), pp. 291-315. - Amsterdam : Elsevier B.V., 2018 Kľúč.slová neutron stars equation of state condensation Jazyk dok. angličtina Krajina Holandsko Systematika 53 Anotácia We extend relativistic mean-field models with hadron masses and meson–baryon coupling constants dependent on the scalar field σ, including hyperons and (1232)baryons, to incorporate a possibility of the charged ρmeson condensation in neutron star matter. The influence of the ρ−condensation on the equation of state proves to be strongly model dependent. In our models of one type (KVORcut-based ones) the ρ−condensation arises by a second-order phase transition above a critical density and the maximum value of the neutron star mass diminishes only slightly. The matter composition changes more significantly. In our models of other type (MKVOR*-based ones), if the system is considered at fixed density, the ρ−condensation arises by a second-order phase transition at the baryon density n =n(II)c,ρand at a slightly higher density n =n(I)c,ρthere occurs a first-order phase transition. In a neutron star matter starting with a density n <n(II)c,ρthere appears a region of a mixed phase, or the system is described by Maxwell construction, that results in a substantial decrease of the value of the maximum neutron star mass. Nevertheless in the models under consideration the observational constraint on the maximum neutron star mass is fulfilled. Besides, in MKVOR*-based models the appearance of the ρ−condensate is accompanied by a strong rearrangement of the matter composition. Dependence of the results on a choice of the ρmeson scaling functions for the effective ρmeson mass and coupling constants is also investigated URL Link na plný text Kategória publikačnej činnosti ADC Číslo archívnej kópie 43905 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika 
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Názov On cooling of neutron stars with a stiff equation of state including hyperons Aut.údaje Hovik Grigorian, Evgeni E. Kolomeitsev ... [et al.] Autor Grigorian Hovik (25%)
Spoluautori Kolomeitsev Evgeni E. 1970- (25%) UMBFP06 - Katedra fyziky
Maslov Konstantin A. (25%)
Voskresensky Dmitri (25%)
Zdroj.dok. Universe. Vol. 4, no. 2 (2018), pp. 1-6. - Basel : Multidisciplinary Digital Publishing Institute, 2018 Kľúč.slová equation of state neutron stars neutrína - neutrinos Jazyk dok. angličtina Krajina Švajčiarsko Systematika 53 Anotácia Exploiting a stiff equation of state of the relativistic mean-field model MKVORHf with sigma-scaled hadron effective masses and couplings, including hyperons, we demonstrate that the existing neutron-star cooling data can be appropriately described within “the nuclear medium cooling scenario” under the assumption that different sources have different masses URL Link na zdrojový dokument Kategória publikačnej činnosti ADM Číslo archívnej kópie 43911 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Charged rho meson condensate in neutron stars within RMF models Aut.údaje Konstantin A. Maslov, Evgeni E. Kolomeitsev, Dmitry N. Voskresensky Autor Maslov Konstantin A. (34%)
Spoluautori Kolomeitsev Evgeni E. 1970- (33%) UMBFP06 - Katedra fyziky
Voskresensky Dmitri (33%)
Zdroj.dok. Universe. Vol. 4, no. 1 (2018), pp. 1-8. - Basel : Multidisciplinary Digital Publishing Institute, 2018 Poznámka Príspevok je evidovaný v databáze WoS. Kľúč.slová neutron stars equation of state rho meson condensation maximum mass Delta resonances Jazyk dok. angličtina Krajina Švajčiarsko Systematika 53 Anotácia Knowledge of the equation of state (EoS) of cold and dense baryonic matter is essential for the description of properties of neutron stars (NSs). With an increase of the density, new baryon species can appear in NS matter, as well as various meson condensates. In previous works, we developed relativistic mean-field (RMF) models with hyperons and Δ -isobars, which passed the majority of known experimental constraints, including the existence of a 2 M ⊙ neutron star. In this contribution, we present results of the inclusion of ρ − -meson condensation into these models. We have shown that, in one class of the models (so-called KVOR-based models, in which the additional stiffening procedure is introduced in the isoscalar sector), the condensation gives only a small contribution to the EoS. In another class of the models (MKVOR-based models with additional stiffening in isovector sector), the condensation can lead to a first-order phase transition and a substantial decrease of the NS mass. Nevertheless, in all resulting models, the condensation does not spoil the description of the experimental constraints URL https://www.mdpi.com/2218-1997/4/1/1 Kategória publikačnej činnosti AFC Číslo archívnej kópie 43907 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov The effect of inclusion of delta resonances in relativistic mean-field model with scaled hadron masses and coupling constants Aut.údaje K. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky Autor Maslov Konstantin A. (1%)
Spoluautori Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
Voskresensky Dmitri (1%)
Zdroj.dok. Journal of Physics: Conference Series. Vol. 798 (2017), pp. 1-5. - Bristol : IOP Publishing, 2017 ; International conference on particle physics and astrophysics ICPPA 2017 medzinárodná konferencia Kľúč.slová astrofyzika - astrophysics neutron stars relativita - relativity Jazyk dok. angličtina Krajina Veľká Británia Systematika 53 Anotácia © Published under licence by IOP Publishing Ltd.Knowledge of the equation of state of the baryon matter plays a decisive role in the description of neutron stars. With an increase of the baryon density the filling of Fermi seas of hyperons and Δ isobars becomes possible. Their inclusion into standard relativistic mean-field models results in a strong softening of the equation of state and a lowering of the maximum neutron star mass below the measured values. We extend a relativistic mean-field model with scaled hadron masses and coupling constants developed in our previous works and take into account now not only hyperons but also the Δ isobars. We analyze available empirical information to put constraints on coupling constants of Δs to mesonic mean fields. We show that the resulting equation of state satisfies majority of presently known experimental constraints. Kategória publikačnej činnosti AFC Číslo archívnej kópie 39068 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Symmetry parameter constraints from a lower bound on neutron-matter energy Aut.údaje Ingo Tews ... [et al.] Autor Tews Ingo (1%)
Spoluautori Lattimer James M. (1%)
Ohnishi Akira (1%)
Kolomeitsev Evgeni E. 1970- (97%) UMBFP06 - Katedra fyziky
Zdroj.dok. The Astrophysical Journal. Vol. 848, no. 2 (2017), pp. [1-15]. - Bristol : IOP Publishing - Institute of Physics Publishing, 2017 Kľúč.slová neutron stars equation of state symmetry energy Jazyk dok. angličtina Krajina Veľká Británia Systematika 53 Anotácia We propose the existence of a lower bound on the energy of pure neutron matter (PNM) on the basis of unitary-gas considerations. We discuss its justification from experimental studies of cold atoms as well as from theoretical studies of neutron matter. We demonstrate that this bound results in limits to the density-dependent symmetry energy, which is the difference between the energies of symmetric nuclear matter and PNM. In particular, this bound leads to a lower limit to the volume symmetry energy parameter S 0. In addition, for assumed values of S 0 above this minimum, this bound implies both upper and lower limits to the symmetry energy slope parameter L ,which describes the lowest-order density dependence of the symmetry energy. A lower bound on neutron-matter incompressibility is also obtained. These bounds are found to be consistent with both recent calculations of the energies of PNM and constraints from nuclear experiments. Our results are significant because several equations of state that are currently used in astrophysical simulations of supernovae and neutron star mergers, as well as in nuclear physics simulations of heavy-ion collisions, have symmetry energy parameters that violate these bounds. Furthermore, below the nuclear saturation density, the bound on neutron-matter energies leads to a lower limit to the density-dependent symmetry energy, which leads to upper limits to the nuclear surface symmetry parameter and the neutron-star crust–core boundary. We also obtain a lower limit to the neutron-skin thicknesses of neutron-rich nuclei. Above the nuclear saturation density, the bound on neutron-matter energies also leads to an upper limit to the symmetry energy, with implications for neutron-star cooling via the direct Urca process Kategória publikačnej činnosti ADC Číslo archívnej kópie 40513 Kategória ohlasu TANG, Shao-Peng - JIANG, Jin-Liang - HAN, Ming-Zhe - FAN, Yi-Zhong - WEI, Da-Ming. Constraints on the phase transition and nuclear symmetry parameters from PSR J0740+6620 and multimessenger data of other neutron stars. In Physical review D. ISSN 2470-0010, 2021, vol. 104, no. 6, pp. 1-12.
SAMMARRUCA, Francesca - MILLERSON, Randy. Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory. In Physical review C. ISSN 2469-9985, 2021, vol. 104, no. 3, pp. 1-9.
HAN, Ming-Zhe - JIANG, Jin-Liang - TANG, Shao-Peng - FAN, Yi-Zhong. Bayesian nonparametric inference of the neutron star equation of state via a neural network. In Astrophysical journal. ISSN 0004-637X, 2021, vol. 919, no. 1, pp. 1-8.
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MENEZES, Debora Peres. A neutron star is born. In Universe. ISSN 2218-1997, 2021, vol. 7, no. 8, pp. 1-41.
WU, Xuhao - BAO, Shishao - SHEN, Hong - XU, Renxin. Effect of the symmetry energy on the secondary component of GW190814 as a neutron star. In Physical review C. ISSN 2469-9985, 2021, vol. 104, no. 1, pp. 1-8.
VARTANYAN, David - LAPLACE, Eva - RENZO, Mathieu - GOTBERG, Ylva - BURROWS, Adam - DE MINK, Selma E. Binary-stripped stars as core-collapse supernovae progenitors. In Astrophysical journal letters. ISSN 2041-8205, 2021, vol. 916, no. 1, pp. 1-10.
NEWTON, William G. - CROCOMBE, Gabriel. Nuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian framework. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 6, pp. 1-21.
LI, Bao-An - CAI, Bao-Jun - XIE, Wen-Jie - ZHANG, Nai-Bo. Progress in constraining nuclear symmetry energy using neutron star observables since GW170817. In Universe. ISSN 2218-1997, 2021, vol. 7, no. 6, pp. 1-39.
BISWAS, Bhaskar - CHAR, Prasanta - NANDI, Rana - BOSE, Sukanta. Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter. In Physical review D. ISSN 2470-0010, 2021, vol. 103, no. 10, pp. 1-13.
BOUKARI, Olfa - PAIS, Helena - ANTIC, Sofija - PROVIDENCIA, Constanca. Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 5, pp. 1-13.
JI, Fan - HU, Jinniu - SHEN, Hong. Nuclear pasta and symmetry energy in the relativistic point-coupling model. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 5, pp. 1-14.
AGRAWAL, B. K. - MALIK, Tuhin - DE, J. N. - SAMADDAR, S. K. Constraining nuclear matter parameters from correlation systematics : a mean-field perspective. In European physical journal : special topics. ISSN 1951-6355, 2021, vol. 230, no. 2, special issue, pp. 517-542.
POWELL, Jade - MUELLER, Bernhard - HEGER, Alexander. The final core collapse of pulsational pair instability supernovae. In Monthly notices of the royal astronomical society. ISSN 0035-8711, 2021, vol. 503, no. 2, pp. 2108-2122.
RHO, Mannque - MA, Yong-Liang. Manifestation of hidden symmetries in baryonic matter : from finite nuclei to neutron stars. In Modern physics letters A. ISSN 0217-7323, 2021, vol. 36, no. 13, pp. 1-17.
MINAMIKAWA, Takuya - KOJO, Toru - HARADA, Masayasu. Quark-hadron crossover equations of state for neutron stars : constraining the chiral invariant mass in a parity doublet model. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 4, pp. 1-14.
JOKELA, Niko - JARVINEN, Matti - NIJS, Govert - REMES, Jere. Unified weak and strong coupling framework for nuclear matter and neutron stars. In Physical review D. ISSN 2470-0010, 2021, vol. 103, no. 8, pp. [1-23].
SHIBAGAKI, Shota - KURODA, Takami - KOTAKE, Kei - TAKIWAKI, Tomoya. Characteristic time variability of gravitational-wave and neutrino signals from three-dimensional simulations of non-rotating and rapidly rotating stellar core collapse. In Monthly notices of the royal astronomical society. ISSN 0035-8711, 2021, vol. 502, no. 2, pp. 3066-3084.
IVANOV, Mario - FERNANDEZ, Rodrigo. Mass ejection in failed supernovae : equation of state and neutrino loss dependence. In Astrophysical journal. ISSN 0004-637X, 2021, vol. 911, no. 1, pp. 1-15.
GIL, Hana - KIM, Young-Min - PAPAKONSTANTINOU, Panagiota - HYUN, Chang Ho. Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the Korea-IBS-Daegu-SKKU framework. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 3, pp. 1-15.
TANG, Shao-Peng - JIANG, Jin-Liang - GAO, Wei-Hong - FAN, Yi-Zhong - WEI, Da-Ming. Constraint on phase transition with the multimessenger data of neutron stars. In Physical review D. ISSN 2470-0010, 2021, vol. 103, no. 6, pp. 1-9.
CAI, Bao-Jun - LI, Bao-An. Intrinsic correlations among characteristics of neutron-rich matter imposed by the unbound nature of pure neutron matter. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 3, pp. 1-10.
BURGIO, G. Fiorella - SCHULZE, Hans-Josef - VIDANA, Isaac - WEI, Jin-Biao. A modern view of the equation of state in nuclear and neutron star matter. In Symmetry (Basel). ISSN 2073-8994, 2021, vol. 13, no. 3, pp. 1-16.
CHOI, Soonchul - MIYATSU, Tsuyoshi - CHEOUN, Myung-Ki - SAITO, Koichi. Constraints on nuclear caturation properties from terrestrial experiments and astrophysical observations of neutron stars. In Astrophysical journal. ISSN 0004-637X, 2021, vol. 909, no. 2, pp. 1-9.
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DEXHEIMER, V - GOMES, R. O. - KLAEHN, T. - HAN, S. - SALINAS, M. GW190814 as a massive rapidly rotating neutron star with exotic degrees of freedom. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 2, pp. 1-11.
HUTH, S. - WELLENHOFER, C. - SCHWENK, A. New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter. In Physical review C. ISSN 2469-9985, 2021, vol. 103, no. 2, pp. 1-21.
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BASTIAN, Niels-Uwe F. Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications. In Physical review D. ISSN 2470-0010, 2021, vol. 103, no. 2, pp. 1-13.
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WELLENHOFER, C. - PHILLIPS, D. R. - SCHWENK, A. From weak to strong : constrained extrapolation of perturbation series with applications to dilute Fermi systems. In Physical review research. ISSN 2643-1564, 2020, vol. 2, no. 4, pp. [1-11].
FAN, Yi-Zhong - JIANG, Jin-Liang - TANG, Shao-Peng - JIN, Zhi-Ping - WEI, Da-Ming. Strong post-merger gravitational radiation of GW170817-like events. In Astrophysical journal. ISSN 0004-637X, 2020, vol. 904, no. 2, pp. 1-6.
MIAO, Zhiqiang - LI, Ang - ZHU, Zhenyu - HAN, Sophia. Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars. In Astrophysical journal. ISSN 0004-637X, 2020, vol. 904, no. 2, pp. 1-12.
DRISCHLER, C. - FURNSTAHL, R. J. - MELENDEZ, J. A. - PHILLIPS, D. R. How well do we know the neutron-matter equation of state at the densities inside neutron stars? A bayesian approach with correlated uncertainties. In Physical review letters. ISSN 0031-9007, 2020, vol. 125, no. 20, pp. 1-7.
JIANG, W. G. - EKSTROM, A. - FORSSEN, C. - HAGEN, G. - JANSEN, G. R. - PAPENBROCK, T. Accurate bulk properties of nuclei from A=2 to infinity from potentials with Delta isobars. In Physical review C. ISSN 2469-9985, 2020, vol. 102, no. 5, pp. [1-8].
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ZHANG, Nai-Bo - LI, Bao-An. GW190814's secondary component with mass 2.50-2.67M(circle dot) as a superfast pulsar. In Astrophysical journal. ISSN 0004-637X, 2020, vol. 902, no. 1, pp. 1-12.
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Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Delta isobars in relativistic mean-field models with sigma-scaled hadron masses and couplings Aut.údaje E. E. Kolomeitsev, K. A. Maslov, D. N. Voskresensky Autor Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
Spoluautori Maslov Konstantin A. (1%)
Voskresensky Dmitri (1%)
Zdroj.dok. Nuclear Physics A. Vol. 961 (2017), pp. 106-141. - Amsterdam : Elsevier B.V., 2017 Kľúč.slová neutron stars equation of state heavy ion collisions Jazyk dok. angličtina Krajina Holandsko Systematika 53 Anotácia We extend the relativistic mean-field models with hadron masses and meson-baryon coupling constants dependent on the scalar sigma field, studied previously to incorporate Delta(1232) baryons. Available empirical information is analyzed to put constraints on the couplings of Delta s with meson fields. Conditions for the appearance of Delta s are studied. We demonstrate that with inclusion of the Delta s our equations of state continue to fulfill majority of known empirical constraints including the pressure-density constraint from heavy-ion collisions, the constraint on the maximum mass of the neutron stars, the direct Urea and the gravitational baryon mass ratio constraints. (C) 2017 Elsevier B.V. All rights reserved. Kategória publikačnej činnosti ADC Číslo archívnej kópie 39909 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Hyperon puzzle and the RMF model with scaled hadron masses and coupling constants Aut.údaje E. E. Kolomeitsev, K. A. Maslov, D. N. Voskresensky Autor Kolomeitsev Evgeni E. 1970- (96%) UMBFP06 - Katedra fyziky
Spoluautori Maslov K. A. (2%)
Voskresensky Dmitri (2%)
Zdroj.dok. Journal of Physics: Conference Series. Vol. 668 (2016), pp. 1-6. - Bristol : IOP Publishing, 2016 ; SQM 2015 medzinárodná konferencia Kľúč.slová stavová rovnica relativistický model stredného poľa neutrónové hviezdy equation of state relativistic mean-field models neutron stars Jazyk dok. angličtina Krajina Veľká Británia Systematika 533 Anotácia The equation of state of cold baryonic matter is studied within a relativistic mean-field model with hadron masses and coupling constants depending on a scalar field. We demonstrate that if the effective nucleon mass stops to decrease with a density increase at densities n > n > n0, where n0 is the nuclear saturation density, the equation of state stiffens for these densities and the limiting neutron star mass increases. The stabilization of the nucleon mass can be realised if in the equation of motion for the scalar mean-field there appear a term sharply varying in a narrow vicinity of the field value corresponding to the density n . We show several possible realizations of this mechanism getting sufficiently stiff equations of state. The appearance of hyperons in dense neutron star interiors is accounted for. The obtained equations of state remain sufficiently stiff if the reduction of the ϕ meson mass is incorporated. Thereby, the hyperon puzzle can be resolved Kategória publikačnej činnosti AFC Číslo archívnej kópie 35029 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Relativistic mean-field models with scaled hadron masses and couplings Podnázov hyperons and maximum neutron star mass Aut.údaje K. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky Autor Maslov K. A. (1%)
Spoluautori Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
Voskresensky Dmitri (1%)
Zdroj.dok. Nuclear Physics A. Vol. 950 (2016), pp. 64-109. - Amsterdam : Elsevier B.V., 2016 Kľúč.slová stavová rovnica equation of state neutrónové hviezdy neutron stars fyzika - physics Jazyk dok. angličtina Krajina Holandsko Systematika 53 Kategória publikačnej činnosti ADC Číslo archívnej kópie 36997 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Solution of the hyperon puzzle within a relativistic mean-field model Aut.údaje K. A. Maslov, Evgeni E. Kolomeitsev, D. N. Voskresensky Autor Maslov K. A. (34%)
Spoluautori Kolomeitsev Evgeni E. 1970- (33%) UMBFP06 - Katedra fyziky
Voskresensky Dmitri (33%)
Zdroj.dok. Physics Letters B. Vol. 748 (2015), pp. 369-375. - Amsterdam : Elsevier B.V., 2015 Kľúč.slová neutrónové hviezdy neutron stars relativistic mean-field models hyperons Jazyk dok. angličtina Krajina Holandsko Kategória publikačnej činnosti ADC Číslo archívnej kópie 33613 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný
Názov Making a soft relativistic mean-field equation of state stiffer at high density Aut.údaje K. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky Autor Maslov K. A. (25%)
Spoluautori Kolomeitsev Evgeni E. 1970- (50%) UMBFP06 - Katedra fyziky
Voskresensky Dmitri (25%)
Zdroj.dok. Physical Review C : Nuclear Physics. Vol. 92, no. 5 (2015), pp. [1-5]. - Maryland : American Physical Society, 2015 Kľúč.slová neutrónové hviezdy stavová rovnica relativistický model stredného poľa neutron stars equation of state relativistic mean-field models Jazyk dok. angličtina Krajina Spojené štáty Systematika 531 Kategória publikačnej činnosti ADC Číslo archívnej kópie 34334 Katal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Báza dát xpca - PUBLIKAČNÁ ČINNOSŤ Odkazy PERIODIKÁ-Súborný záznam periodika nerozpoznaný