Gotowe bibliografie tematyczne / Model gravitational field

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  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji

Gotowa bibliografia na temat „Model gravitational field”

Autor: Grafiati
Data publikacji: 2 czerwca 2025
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Model gravitational field"

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Chernitskii, Alexander A. "Induced gravitation in nonlinear field models." International Journal of Modern Physics: Conference Series 41 (January 2016): 1660119. http://dx.doi.org/10.1142/s2010194516601198.

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The description of gravitation in the framework of soliton interaction is considered for two nonlinear field models. These models are Born — Infeld nonlinear electrodynamics and so-called Born — Infeld type scalar field model. The last model can also be called the extremal space-time film one because of the specific form of the appropriate variational principle. Gravitational interaction is considered in the context of unification for all interactions of material particles. It is shown that long-range interaction of solitons of the models appears as force one and metrical one. The force intera
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Lukyantsev, Dmitriy, Nikolay Afanasiev, Ekaterina Kalashnikova, and Andrey Tanaev. "Mathematical Modeling of Refraction Characteristics of Electromagnetic Radiation at Stochastic Gravitational Field." Mathematical Physics and Computer Simulation 27, no. 2 (2024): 48–60. http://dx.doi.org/10.15688/mpcm.jvolsu.2024.2.4.

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Numerical-analytical modeling is used for estimation of gravitational noise influence on propagation of electromagnetic radiation at gravitational field of a group of astrophysical objects. The method bases on numerical integrate of system of light differential equations in the Euler’s form, added differential equations for calculation of statistic moments of side fluctuations of light at a picture plane of observer. The influence of gravitation was taken into account by introducing of the effective refraction index of vacuum, expressed through a gravitational potential. Visions about spatial
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Krot, Alexander M. "Derivation of field equations and investigation of gravitational waves in the gravitational field of a condensing cosmogonical body based on the statistical theory." Journal of Physics: Conference Series 3027, no. 1 (2025): 012004. https://doi.org/10.1088/1742-6596/3027/1/012004.

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Abstract This paper considers the statistical theory of cosmogonical body formation in order to derive field equations and investigate gravitational waves in the gravitational field of a condensing cosmogonical body. The models and evolution equations of the statistical mechanics have been proposed in this theory, while well-known problems of gravitational condensation of infinitely spread cosmic media have been solved on the basis of the proposed statistical model of a spheroidal body. Within the framework of the statistical theory, the presence of an ethereal medium (or a dark matter) around
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DANEHKAR, ASHKBIZ. "ON THE SIGNIFICANCE OF THE WEYL CURVATURE IN A RELATIVISTIC COSMOLOGICAL MODEL." Modern Physics Letters A 24, no. 38 (2009): 3113–27. http://dx.doi.org/10.1142/s0217732309032046.

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The Weyl curvature includes the Newtonian field and an additional field, the so-called anti-Newtonian. In this paper, we use the Bianchi and Ricci identities to provide a set of constraints and propagations for the Weyl fields. The temporal evolutions of propagations manifest explicit solutions of gravitational waves. We see that models with purely Newtonian field are inconsistent with relativistic models and obstruct sounding solutions. Therefore, both fields are necessary for the nonlocal nature and radiative solutions of gravitation.
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Chen, Yu-Jie, Shi-Lin Li, Yu-Zhu Chen, Wen-Du Li, and Wu-Sheng Dai. "Gravitational constant model and correction." Journal of Mathematical Physics 63, no. 11 (2022): 112503. http://dx.doi.org/10.1063/5.0095583.

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We construct a model for considering the quantum correction of the gravitational constant. In the model, the gravitational constant originates from a coupling between the gravitational field and a scalar field. If the scalar field, as it should be in the real physical world, is a quantum field, the gravitational constant will have a quantum correction. The quantum correction, generally speaking, varies with spacetime coordinates. Therefore, the gravitational constant is no longer a constant. In different spacetime, the quantum correction is different, for the coupling in different spacetime is
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Fedosin, Sergey G. "The Gravitational Field in the Relativistic Uniform Model within the Framework of the Covariant Theory of Gravitation." International Letters of Chemistry, Physics and Astronomy 78 (April 12, 2018): 39–50. https://doi.org/10.18052/www.scipress.com/ILCPA.78.39.

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For the relativistic uniform system with an invariant mass density the exact expressions are determined for the potentials and strengths of the gravitational field, the energy of particles and fields. It is shown that, as in the classical case for bodies with a constant mass density, in the system with a zero vector potential of the gravitational field, the energy of the particles, associated with the scalar field potential, is twice as large in the absolute value as the energy defined by the tensor invariant of the gravitational field. The problem of inaccuracy of the use of the field’s
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Fedosin, Sergey G. "The Gravitational Field in the Relativistic Uniform Model within the Framework of the Covariant Theory of Gravitation." International Letters of Chemistry, Physics and Astronomy 78 (April 2018): 39–50. http://dx.doi.org/10.18052/www.scipress.com/ilcpa.78.39.

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For the relativistic uniform system with an invariant mass density the exact expressions are determined for the potentials and strengths of the gravitational field, the energy of particles and fields. It is shown that, as in the classical case for bodies with a constant mass density, in the system with a zero vector potential of the gravitational field, the energy of the particles, associated with the scalar field potential, is twice as large in the absolute value as the energy defined by the tensor invariant of the gravitational field. The problem of inaccuracy of the use of the field’s stres
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Fedosin, Sergey G. "The Gravitational Field in the Relativistic Uniform Model within the Framework of the Covariant Theory of Gravitation." International Letters of Chemistry, Physics and Astronomy 78 (April 10, 2018): 39–50. http://dx.doi.org/10.56431/p-152cfg.

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For the relativistic uniform system with an invariant mass density the exact expressions are determined for the potentials and strengths of the gravitational field, the energy of particles and fields. It is shown that, as in the classical case for bodies with a constant mass density, in the system with a zero vector potential of the gravitational field, the energy of the particles, associated with the scalar field potential, is twice as large in the absolute value as the energy defined by the tensor invariant of the gravitational field. The problem of inaccuracy of the use of the field’s stres
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Fedosin, Sergey G. "The charged component of the vacuum field as the source of electric force in the modernized Le Sage's model." Journal of Fundamental and Applied Sciences 8, no. 3 (2016): 971–1020. https://doi.org/10.5281/zenodo.845357.

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The formula is derived for the electric force inside a uniformly charged spherical body, as well as for the Coulomb force between the charged bodies from the standpoint of the model of the vacuum field with charged particles. The parameters of the fluxes of charged particles are estimated, including the energy density, energy flux and cross section of interaction with the charged matter. The energy density of gravitons in the Le Sage’s gravitation model is expressed in terms of the strong gravitational constant. The charge to mass ratio is determined for the charged particles that make u
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Greyber, Howard D. "The Strong Magnetic Field Galactic Center-AGN-Quasar Model." Symposium - International Astronomical Union 136 (1989): 335–40. http://dx.doi.org/10.1017/s007418090018670x.

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The energy storage and dynamics at the center of galaxies is explained using a new construct, the gravitationally bound current loop (GBCL), produced when the galaxy formed under gravitational collapse. Thin toroidal plasma around the slender intense relativistic current loop is bound to it by the Maxwell “frozen-field” condition, and also binds gravitationally to the central object (presumably a black hole). The Strong Magnetic Field model (SMF) explains directly the Milky Way (MW) galactic center radio observations of a vertical magnetic field perpendicular to the galactic disk and the exten
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Rozprawy doktorskie na temat "Model gravitational field"

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Feix, Martin. "Extragalactic and cosmological tests of gravity theories with additional scalar or vector fields." Thesis, University of St Andrews, 2011. http://hdl.handle.net/10023/1901.

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Despite the many successes of the current standard model of cosmology on the largest physical scales, it relies on two phenomenologically motivated constituents, cold dark matter and dark energy, which account for approximately 95% of the energy-matter content of the universe. From a more fundamental point of view, however, the introduction of a dark energy (DE) component is theoretically challenging and extremely fine-tuned, despite the many proposals for its dynamics. On the other hand, the concept of cold dark matter (CDM) also suffers from several issues such as the lack of direct experime
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Gaset, Rifà Jordi. "A multisymplectic approach to gravitational theories." Doctoral thesis, Universitat Politècnica de Catalunya, 2018. http://hdl.handle.net/10803/620740.

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The theories of gravity are one of the most important topics in theoretical physics and mathematical physics nowadays. The classical formulation of gravity uses the Hilbert-Einstein Lagrangian, which is a singular second-order Lagrangian; hence it requires a geometric theory for second-order field theories which leads to several difficulties. Another standard formulation is the Einstein-Palatini or Metric-Affine, which uses a singular first order Lagrangian. Much work has been done with the aim of establishing the suitable geometrical structures for describing classical field theories. In
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Da, Silva Caroline Dos Santos. "Cosmic strings and scalar tensor gravity." Thesis, Durham University, 1999. http://etheses.dur.ac.uk/4577/.

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This thesis is concerned with the study of cosmic strings. We studied the values for the Higgs mass and string coupling for which the gravitational effect of an infinite cosmic string in the context of the Einstein theory is not only locally but also globally weak. We conclude this happens for strings formed at scales less or equal to the Planck one with Higgs mass being less or equal to the boson vectorial mass. Then we examined the metric of an isolated self-gravitating abelian-Higgs vortex in dilatonic gravity for arbitrary coupling of the vortex fields to the dilaton. We looked for solutio
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CUOFANO, Carmine. "Magnetic fields generated by r-modes in accreting millisecond pulsars." Doctoral thesis, Università degli studi di Ferrara, 2010. http://hdl.handle.net/11392/2389313.

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In rotating neutron stars the existence of the Coriolis force allows the presence of the so-called Rossby oscillations (r-modes) which are known to be unstable to emission of gravitational waves. In the Thesis, for the first time, we introduce the magnetic damping rate in the evolution equations of r-modes. We show that r-modes can generate very strong toroidal fields in the core of accreting millisecond pulsars by inducing differential rotation. We shortly discuss the instabilities of the generated magnetic field and its long time-scale evolution in order to clarify how the generated mag
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Xufen, Wu. "Numerical modeling of modified Newtonian dynamics in galaxies : testing the external field effects." Thesis, University of St Andrews, 2010. http://hdl.handle.net/10023/1706.

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Galaxies are natural laboratories for testing fundamental physics on the nature of the dark matter. MOdified Newtonian Dynamics (MOND) has been tested for over 20 years on small and large scales. While there are several versions of how MOND extrapolates to the large scales, and these versions are not yet fully successful, the original Bekenstein-Milgrom version of MOND is fully predictive and works very well on galaxy scales. However, little work has been done to explore this theory beyond fitting the rotation curves and Tully-Fisher relation of isolated disc galaxies. So far little is known o
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Guarnieri, Filippo. "Renormalization group flow of scalar models in gravity." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2014. http://dx.doi.org/10.18452/16976.

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In dieser Doktorarbeit werden wir das Renormierungsproblem von Gravitationstheorien im Kontext der Renormierungsgruppe (RG) unter Anwendung von perturbativen und nicht-perturbativen Methoden untersuchen. Insbesondere werden wir uns auf verschiedene Gravitationsmodelle und Näherungen konzentrieren, in welchen die zentrale Rolle von einem skalaren Freiheitsgrad eingenommen wird. Wir konzentrieren uns besonders auf zwei Ansätze für Quantengravitation, die in letzter Zeit viel Aufmerksamkeit erhalten haben, nämlich den asymptotisch sicheren Fall der Gravitation und die Hořava-Lifshitz Quantengra
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Martineau, Killian. "Quelques aspects de cosmologie et de physique des trous noirs en gravitation quantique à boucles Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi I universe with different inflaton potentials and initial conditions Some clarifications on the duration of inflation in loop quantum cosmology A first step towards the inflationary trans-Planckian problem treatment in loop quantum cosmology Scalar spectra of primordial perturbations in loop quantum cosmology Phenomenology of quantum reduced loop gravity in the isotropic cosmological sector Primordial Power Spectra from an Emergent Universe: Basic Results and Clarifications Fast radio bursts and the stochastic lifetime of black holes in quantum gravity Quantum fields in the background spacetime of a polymeric loop black hole Quasinormal modes of black holes in a toy-model for cumulative quantum gravity Seeing through the cosmological bounce: Footprints of the contracting phase and luminosity distance in bouncing models Dark matter as Planck relics without too exotic hypotheses A Status Report on the Phenomenology of Black Holes in Loop Quantum Gravity: Evaporation, Tunneling to White Holes, Dark Matter and Gravitational Waves." Thesis, Université Grenoble Alpes (ComUE), 2019. http://www.theses.fr/2019GREAY044.

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Cantonnée à la physique mathématique depuis des décennies, la gravitation quantique entre désormais dans le giron de la science expérimentale. Suivant cette mouvance nous considérons dans cette thèse trois cadres d’application de la gravitation quantique à boucles (LQG) : le système Univers, les trous noirs et les astroparticules. Le troisième n’est qu’esquissé tandis que les deux premiers sont présentés plus en détails.Le secteur cosmologique étant l’un des domaines les plus prometteurs pour tester et contraindre des théories de gravité quantique, le développement de différents modèles tentan
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Garolera, Huguet Blai. "Probing gauge theories: Exact results and holographic computations." Doctoral thesis, Universitat de Barcelona, 2015. http://hdl.handle.net/10803/289346.

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The holographic duality between gauge theories and string theories has opened a new door to access the strongly coupled regime of quantum field theories and offers, at the same time, a completely new way to understand the elusive nature of quantum gravity and the non-perturbative regime of string theory. After almost two decades of research, the current status of the correspondence is that of a solid conjecture that has passed a great number of nontrivial tests, to the point that it is generally believed to be true. The present thesis includes a collection of four pap
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Felker, Paige Shannon. "Design of a reduced-order spherical harmonics model of the Moon's gravitational field." Thesis, 2009. http://hdl.handle.net/2152/ETD-UT-2009-12-434.

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An important aspect for precision guidance, navigation, and control for lunar operations is environmental modeling. In particular, consider gravity field modeling. Available gravity field models for the Moon reach degree and order 165 requiring the use and storage of approximately 26,000 spherical harmonic coefficients. Although the high degree and order provide a means by which to accurately predict trajectories within the influence of the Moon's gravitational field, the size of these models makes using them computationally expensive and restricts their use in design environments with limited
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Mahlatji, Matsimele Ngwalodi. "Some models of relativistic radiating stars." Thesis, 2012. http://hdl.handle.net/10413/10616.

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In this dissertation we study radiating stars in strong gravitational elds. We generate new classes of exact solutions to the Einstein eld equations and the boundary condition applicable to radiating relativistic stars. The model of a radiating star in general relativity, matching to the Vaidya exterior spacetime, is reviewed. The boundary condition is converted to a Riccati equation and we consider both cases involving geodesic and non-geodesic particle trajectories. We present the metrics found previously. We rst solve the boundary condition for the geodesic case and nd the gravitational
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Książki na temat "Model gravitational field"

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Marsh, J. G. An improved model of the earth's gravitational field: *GEM-T1*. NASA, 1988.

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G, Marsh J., and Goddard Space Flight Center, eds. An improved model of the earth's gravitational field: GEM-T1. National Aeronautics and Space Administration, Goddard Space Flight Center, 1987.

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G, Marsh J., and Goddard Space Flight Center, eds. The GEM-T2 gravitational model. National Aeronautics and Space Administration, Goddard Space Flight Center, 1989.

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J, Bouman. Quality assessment of satellite-based global gravity field models. NCG, 2000.

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Green, James A. Gravitation & the electroform model: From general relativity to unified field theory. 7th ed. Greenwood Research, 1994.

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United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., ed. High degree gravitational sensitivity from Mars orbiters for the GMM-1 gravity model. National Aeronautics and Space Administration, Scientific and Technical Information Program, 1993.

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García, Pilar, J. A. de Azcárraga, Víctor Aldaya, and José Ma Cerveró. Symmetries in gravity and field theory: Homenaje al Profesor José Adolfo de Azcárraga. Ediciones Universidad de Salamanca, 2004.

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Freeden, W. Multiscale modelling of spaceborne geodata. Teubner, 1999.

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Loon, Jasper Van. Functional and stochastic modelling of satellite gravity data. NCG, Nederlandse Commissie voor Geodesie, 2008.

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Holman, Richard. Gravitational couplings of the inflaton in extended inflation. Fermi National Accelerator Laboratory, 1990.

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Części książek na temat "Model gravitational field"

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Sturani, Riccardo. "Effective Field Theory Methods to Model Compact Binaries." In Handbook of Gravitational Wave Astronomy. Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-16-4306-4_32.

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Sturani, Riccardo. "Effective Field Theory Methods to Model Compact Binaries." In Handbook of Gravitational Wave Astronomy. Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-15-4702-7_32-1.

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Yu, Boxi, and Di Huang. "Gravitational Field Simulation Based on Point-Array and Standard Model." In Lecture Notes in Electrical Engineering. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-6613-2_271.

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Rapp, Richard H., and R. Steven Nerem. "A Joint GSFC/DMA Project for Improving the Model of the Earth’s Gravitational Field." In International Association of Geodesy Symposia. Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79721-7_42.

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Veneziano, Gabriele. "From the Hadronic String to Quantum Gravity ... and Back." In Springer Proceedings in Physics. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-23042-4_9.

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AbstractI will outline the conceptual developments that led, through half a century, to the present formulation of string theory. The phenomenological observation of Dolen-Horn-Schmit “duality” in 1967, the formulation, a year later, of the Dual Resonance Model, and its eventual interpretation as a theory of quantum relativistic strings, marked the birth of the hadronic string. Immediately after, however, this elegant S-matrix theory of the strong interactions lost its phenomenological battle against a more, but not quite, conventional quantum field theory risking, around 1974, total oblivion.
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Freire-Torres, Mario, and Jaime Carpio. "Contribution to Mathematical Modeling and Numerical Simulation of Welding Processes." In Proceedings of the XV Ibero-American Congress of Mechanical Engineering. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-38563-6_4.

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AbstractThe present work describes a mathematical model for the numerical simulation of the welding process. Initially, the domain Ω is solid to which the heat is released in certain areas. This heat increases the temperature of the solid, and when the fusion temperature is reached, the phase change occurs. At the fusion temperature, there is a mixture between liquid and solid (modelled as a porous medium); above this temperature mentioned; we will find only liquid. Natural convection currents can occur in the liquid due to buoyancy induced by the gravitational field. In order to reproduce all
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Leng, Qing, Ming Zhang, Gensheng Zhao, Senhao Mao, and Ang Jiang. "Simulation and Hazard Map of Flooding Caused by the Break of a Concrete Gravitational Dam." In Lecture Notes in Civil Engineering. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-6138-0_109.

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AbstractThe simulation of Concrete Gravitational Dam burst floods is an important research content in the field of disaster prevention and mitigation in water conservancy projects. Due to the extreme rainfall, earthquake, structure failure and etc., the concrete gravitational dam usually breaks in a short time period. The dam break flood will give an extreme risk to the downstream communities. Taking the flood simulation of the Kaliwa Dam in the Philippines as an example, based on the downstream channel of the dam body and the measured terrain on both sides, a numerical simulation model of one
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Nath, G., and Sumeeta Singh. "An Exact Solution for Magnetogasdynamic Shock Wave Generated by a Moving Piston Under the Influence of Gravitational Field with Radiation Flux: Roche Model." In Lecture Notes in Mechanical Engineering. Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5862-7_43.

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Melnikov, V. N., and V. R. Gavrilov. "2-Component Cosmological Models with Perfect Fluid and Scalar Field: Exact Solutions." In The Gravitational Constant: Generalized Gravitational Theories and Experiments. Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2242-5_12.

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Sheng, Michael B., Petr Vaníček, Robert Kingdon, and Ismael Foroughi. "Rigorous Evaluation of Gravity Field Functionals from Satellite-Only Gravitational Models Within Topography." In International Symposium on Gravity, Geoid and Height Systems 2016. Springer International Publishing, 2017. http://dx.doi.org/10.1007/1345_2017_26.

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Streszczenia konferencji na temat "Model gravitational field"

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Moraes, P. H. R. S., and O. D. Miranda. "Cosmology from Kaluza-Klein gravitational model." In THE SIXTH INTERNATIONAL SCHOOL ON FIELD THEORY AND GRAVITATION-2012. AIP, 2012. http://dx.doi.org/10.1063/1.4756990.

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Sultanov, I. M. "Gravitational Fragmentation of Molecular Filament with Magnetic Field." In 52-st All-Russian with international participation student scientific conference "Physics of Space". Ural University Press, 2025. https://doi.org/10.15826/b978-5-7996-3986-0.75.

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We model gravitational fragmentation of cylindrical molecular cloud with large-scale magnetic field with numerical code FLASH. Simulations show that initial perturbations lead to formation of equally-spaced clumps according to the wavelength of initial perturbation. Gravitationally-bound clumps are formed when the initial perturbation wavelength is close to or exceeds critical value. Critical perturbations lead to the formation of the cores with size 1 700 au. Supercritical perturbations lead to the formation of the cores with size of 8 000 au. Sizes of cores insignificantly decrease with incr
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LEWIS, RAY A., and GIOVANNI MODANESE. "Gravitational Radiation of a Vibrating Physical String as a Model for the Gravitational Emission of an Astrophysical Plasma." In Unified Field Mechanics: Natural Science Beyond the Veil of Spacetime. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814719063_0011.

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Huang, Qin, Guohui Li, Zhili Liang, Jun Wu, Yu Lei, and Leren Yuan. "Interaction Behavior Measurement of Electrical Workers Based on Gravitational Field Model." In 2023 Panda Forum on Power and Energy (PandaFPE). IEEE, 2023. http://dx.doi.org/10.1109/pandafpe57779.2023.10140333.

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Ababneh, Mohammed T., Frank M. Gerner, Pramod Chamarthy, Peter de Bock, Shakti Chauhan, and Tao Deng. "Thermo-Fluid Model for High Thermal Conductivity Thermal Ground Planes." In ASME 2012 Third International Conference on Micro/Nanoscale Heat and Mass Transfer. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/mnhmt2012-75185.

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The thermal ground plane (TGP) is an advanced planar heat pipe designed for cooling microelectronics in high gravitational fields. A thermal resistance model is developed to predict the thermal performance of the TGP, including the effects of the presence of non-condensable gases (NCGs). Viscous laminar flow pressure losses are predicted to determine the maximum heat load when the capillary limit is reached. This paper shows that the axial effective thermal conductivity of the TGP decreases when the substrate and/or wick are thicker and/or with the presence of NCGs. Moreover, it was demonstrat
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Di Gioia, Federico, and Giovanni Montani. "Cosmological perturbations and gravitational instability of the Bianchi I model with a magnetic field." In Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0153.

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Hasanov, I. M., and L. A. Muravyev. "Comparison of the new gravity field model XGM2019e with other modern global models of the gravitational field for the Magadan region." In Geoinformatics: Theoretical and Applied Aspects 2020. European Association of Geoscientists & Engineers, 2020. http://dx.doi.org/10.3997/2214-4609.2020geo112.

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Andrianov, S. A. "Model of gravitational wave signal processing in framework of pulsar timing array." In 51-st All-Russian with international participation student scientific conference "Physics of Space". Ural University Press, 2024. http://dx.doi.org/10.15826/b978-5-7996-3848-1.10.

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This work describes a statistical model of detection of a weak stochastic gravitational wave (GW) present in the timing data of a pulsar array. The model consists of a generator of the low-frequency noise modeled the signal of the stochastic GW background and a block of pulsar timing array data processing. The data processing is carried out with the help of statistical methods based on the frequentist interpretation of probability. The model under discussion is used for processing one of the generated GW background realizations. The result of the data processing is the estimates of the likelih
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Grunskaya, L., V. Isakevich, and D. Isakevich. "Susceptibility of electromagnetic fields in the Solar System to gravitational wave effects from relativistic binary star systems." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.104.

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Using an eigenvector and signal component analyzer (eigenoscope), the problem of identifying the impact of gravitational waves of relativistic binary star systems (RBSS) with large and small eccentricity on the vertical component of the electric field strength ($E_\text{z}$) in the Earth's atmospheric surface layer in the infra-low frequency (ILF) range at high harmonics of the EDS circulation frequencies has been solved. The results were obtained using monitoring data at four spatially separated $E_\text{z}$ observation stations. A model is proposed to explain the effect of the gravitational
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Krylova, N., and V. Red'kov. "Dirac particle in gravitational field of black hole with Newman-Unti-Tamburino parameter." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.013.

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We study the quantum-mechanical problem of a spin 1/2 particle in gravitational field of the black hole with Newman-Unti-Tamburino (NUT) parameter. Separation of the variables has been performed in the Dirac equation. The system of angular equations has been solved analytically in terms of hypergeometric functions. The quantization condition for the angular parameter is derived. In the massless case, the radial system is reduced to separate systems of two first-order equations which are solved in terms of the confluent Heun functions. Generalized tortoise-like coordinate is introduced, and exp
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