Article
Astronomy & Astrophysics
Gary Nash
Summary: MGR is the natural extension of GR, which uses a smooth regular line element vector field (X,-X) to construct a connection-independent symmetric tensor representing the energy-momentum of the gravitational field. It solves the localization problem of gravitational energy-momentum in GR and maintains the equivalence principle. The line element field provides MGR with the extra freedom to describe dark energy and dark matter.
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
(2023)
Article
Physics, Particles & Fields
Yogendra Srivastava, Giorgio Immirzi, John Swain, Orlando Panella, Simone Pacetti
Summary: This article discusses a general class of axially symmetric metrics in general relativity that includes rotations, which are used to study the dynamics of rotationally supported galaxies. The exact vacuum solutions of the Einstein equations for this extended Weyl class of metrics lead to the following rigorous deductions: (i) The rotational velocity in general relativity always exceeds the Newtonian velocity due to Lenz's law. (ii) A non-zero intrinsic angular momentum for a galaxy requires the asymptotic constancy of the Weyl length parameter, similar to the Kerr metric. (iii) The asymptotic constancy of the parameter also implies a plateau in the rotational velocity. Unlike the Kerr metric, the extended Weyl metric can be extended within the galaxy, and it has been shown that Gauss and Ampere laws emerge along with Ludwig's extended gravito-electromagnetism (GEM) theory and non-linear rate equations for the velocity field. More accurate estimates for the Sun's escape velocity than those obtained from Newtonian theory have been presented.
EUROPEAN PHYSICAL JOURNAL C
(2023)
Article
Physics, Multidisciplinary
Mikhail Shaposhnikov, Andrey Shkerin, Inar Timiryasov, Sebastian Zell
Summary: This passage discusses a novel mechanism for producing singlet fermions in the early Universe through gravity-induced interactions. These fermions can act as dark matter particles and are applicable to a wide range of dark matter particle masses. The potential observational consequences of producing keV-scale dark matter in this way, particularly for right-handed neutrinos, are also explored. The authors suggest that determining the momentum distribution of primordial dark matter may shed light on gravity-induced fermionic interactions.
PHYSICAL REVIEW LETTERS
(2021)
Article
Astronomy & Astrophysics
Artyom V. Astashenok, Sergey D. Odintsov, Vasilis K. Oikonomou
Summary: In this paper, we investigate realistic models of compact objects, focusing on neutron and strange stars composed of dense matter and dark energy. We consider different scenarios for dark energy, including simple fluid or scalar field interacting with matter, modified gravity combined with dark energy, and dark energy as scalar field non-minimally interacting with gravity.
PHYSICS OF THE DARK UNIVERSE
(2023)
Article
Astronomy & Astrophysics
P. Mafa Takisa, S. D. Maharaj, M. L. Lekala
Summary: This work models compact stars using an equation of state of dark matter with admixed matter, exploring physical features and mass limits, and showing the influence of the nonlinear term on matter distribution. In particular, the maximum stellar mass of PSRJ0030+0451 is found for the admixed matter distribution.
ASTROPHYSICS AND SPACE SCIENCE
(2021)
Article
Physics, Multidisciplinary
Patryk Mach, Andrzej Odrzywolek
Summary: This study examines the accretion of dark matter onto a moving Schwarzschild black hole, deriving a relationship between the accretion rate and the black hole velocity, with a monotonic relation found in high-temperature situations. The results are relevant for understanding the growth of primordial black holes in the early Universe.
PHYSICAL REVIEW LETTERS
(2021)
Article
Astronomy & Astrophysics
H. C. Das, Ankit Kumar, Bharat Kumar, S. K. Biswal, S. K. Patra
Summary: The study found that dark matter has a significant impact on the curvatures of neutron stars, especially the surface curvature of massive stars. The effects of dark matter on the compactness of maximum neutron star mass are less pronounced, but it can make the system unstable as the binding energy of the neutron star becomes positive with increasing dark matter momentum.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Nan Jiang, Kent Yagi
Summary: Gravitational-wave sources can be used as standard sirens to probe cosmology by measuring their luminosity distance and redshift, as well as theories beyond general relativity. By extracting redshift from tidal measurements of binary neutron stars, it is possible to use gravitational-wave observations alone to explore gravity.
Article
Astronomy & Astrophysics
Billy K. K. Lee, Ming-chung Chu, Lap-Ming Lin
Summary: The investigation explores the possibility of a 2.6 M(circledot) compact object in the gravitational wave event GW190814 being a compact star admixed with bosonic dark matter. Constraints on the mass, radius, and stability of the object suggest that the dark matter may be composed of QCD axions, with their particle mass range potentially overlapping with constraints from black hole superradiance processes.
ASTROPHYSICAL JOURNAL
(2021)
Article
Physics, Particles & Fields
Igor E. Bulyzhenkov
Summary: Temporal derivatives of the attracting mass in Newton's law can balance accelerations for the rotating periphery of a spiral galaxy. Thermal losses of the mass-energy integral inside the circle of rotation cause the mega-vortex organization of the emitting galaxy. Rejecting dark matter in cosmic distributions involves modifying Euler/Navier-Stokes hydrodynamics using adaptive tensor responses with metric waves, not gravimagnetic corrections from General Relativity.
EUROPEAN PHYSICAL JOURNAL C
(2021)
Article
Astronomy & Astrophysics
Tobias Mistele
Summary: Research indicates that on galactic scales, the dual role of the phonon field in superfluid dark matter is in tension, and splitting these roles into different fields can elegantly resolve a stability issue. This also calls for a reevaluation of standard estimates for the size of a galaxy's superfluid core.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Physics, Particles & Fields
Federico Re
Summary: This research proposes a relativistic effect to explain dark matter and dark energy. Inhomogeneous matter generates gravitational distortions, significantly affecting the expansion of the universe and requiring corrections to the parameters of the standard cosmological model. Relativistic models offer various solutions, including those that fully explain dark energy and dark matter.
EUROPEAN PHYSICAL JOURNAL C
(2021)
Article
Astronomy & Astrophysics
Andreas Bauswein, Gang Guo, Jr-Hua Lien, Yen-Hsun Lin, Meng-Ru Wu
Summary: In this study, the long-lasting gravitational wave emission from compact dark objects in binary neutron-star mergers is estimated. By performing relativistic simulations, it is found that these dark matter components can remain gravitationally bound and generate gravitational wave signals with frequencies in the kilohertz range. Furthermore, relations between the gravitational wave frequency of the dark matter components and the properties of the merger remnant are established. The detectability of these gravitational wave signals suggests that only dark matter objects with masses of about 0.01 to 0.1 times the solar mass can be observed with existing and projected gravitational wave instruments.
Article
Astronomy & Astrophysics
Antonio De Felice, Shinji Mukohyama
Summary: This paper introduces a new cosmological framework integrating dark matter into a minimally modified gravity model, maintaining the same number of gravitational degrees of freedom through a series of transformations. The framework includes two time-dependent free functions to achieve desired evolutions of Hubble expansion rate and effective gravitational constant for dark matter.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
H. C. Das, Ankit Kumar, S. K. Patra
Summary: The study analyzes the observational data of GW190814 to put constraints on its secondary component. Using relativistic mean-field models, the researchers calculate the mass-radius profile and tidal deformability of the compact object, treating it as a massive neutron star with dark matter particles. It is observed that the predicted properties are consistent with the observational data, suggesting the possibility of a dark matter admixed neutron star if the nuclear equation of state is sufficiently stiff.
Article
Astronomy & Astrophysics
S. K. Maurya, Ksh Newton Singh, M. Govender, Sudan Hansraj
Summary: The recent advance in the minimal geometric deformation (MGD) method has sparked interest in investigating higher-curvature gravitational effects in relativistic astrophysics. This study models a strange star using the MGD technique within the framework of Einstein-Gauss-Bonnet gravity. The findings demonstrate the existence of stable compact objects with masses exceeding the mass of a black hole without the need for exotic matter.
ASTROPHYSICAL JOURNAL
(2022)
Article
Physics, Multidisciplinary
M. Zubair, Allah Ditta, Saira Waheed, Francisco Tello-Ortiz
Summary: This paper studies the structure of compact objects such as PSRJ 1614 - 2230, LMXB 4U1608 - 52, CenX - 3, EX01785 - 248, and SMCX - 1 in the framework of f(T, tau) gravity. The study finds that the constructed model matches well with the realistic nature of compact stars.
CHINESE JOURNAL OF PHYSICS
(2022)
Article
Physics, Particles & Fields
S. K. Maurya, M. Govender, Simranjeet Kaur, Riju Nag
Summary: In this research, a hierarchical solution-generating technique is proposed for bounded compact objects in classical general relativity. The Minimum Gravitational Decoupling (MGD) Method and the generalized concept of Complexity are employed to obtain two classes of solutions as candidates for physically realizable compact objects.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Particles & Fields
S. K. Maurya, Riju Nag
Summary: In this paper, we discuss the role of gravitational decoupling in isotropizing the anisotropic solution of Einstein's field equations. We also analyze its influence on the complexity factor in static self-gravitating systems. Additionally, we propose a simple and effective technique to generate new solutions for self-gravitating objects using the complete geometric deformation approach.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Particles & Fields
S. K. Maurya, M. Govender, Ksh Newton Singh, Riju Nag
Summary: In this study, we investigate the characteristics of an anisotropic stellar object using the polytropic solution within the framework of Einstein-Gauss-Bonnet (EGB) gravity. Anisotropy is introduced through the minimally gravitational decoupling method. The analysis of the exact solution for the gravitational potentials reveals novel features of the compact object. The EGB coupling constant and the decoupling parameter are found to play important roles in modifying the effective density and radial profiles at each interior point of the object, as well as inducing a change in the trends of the effective tangential pressure.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Multidisciplinary
A. S. Agrawal, Francisco Tello-Ortiz, B. Mishra, S. K. Tripathy
Summary: In this paper, a bouncing cosmological model of the Universe in extended gravity theory is presented, exploring the dynamic behavior, singularity of geometrical parameters, and the role of coupling parameters in achieving stability at the bouncing epoch. The study also demonstrates the significance of scale factor parameters in bouncing behavior and shows the dynamical stability of the model through linear homogeneous perturbation calculations.
FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS
(2022)
Article
Physics, Multidisciplinary
Milko Estrada, Francisco Tello-Ortiz, Ksh. Newton Singh, S. K. Maurya
Summary: This work focuses on representing 4D spherically symmetric and static compact stellar configurations into a 5D space-time using the black string framework. By introducing a function A(z), the 4D and 5D quantities are related, resulting in the reduction of the 5D equations to the usual form of 4D equations of motion. The chosen methodology has the potential to represent other types of 4D objects into an extra dimension.
CHINESE JOURNAL OF PHYSICS
(2023)
Article
Astronomy & Astrophysics
Alvaro Restuccia, Francisco Tello-Ortiz
Summary: An anisotropic model describing gravity-vector gauge coupling is proposed, based on the 4+1 dimensional non-projectable Ho.rava-Lifshitz gravity theory with a geometrical restriction. Renormalizability arguments require including interactions up to terms with z = 4 spatial derivatives on the geometrical tensor fields. The reduction to 3+1 dimensions results in a model invariant under FDiff and U(1) symmetry groups, propagating the same spectrum as the Einstein-Maxwell theory at the kinetic conformal point.
CLASSICAL AND QUANTUM GRAVITY
(2023)
Article
Physics, Multidisciplinary
Francisco Tello-Ortiz, B. Mishra, A. Alvarez, Ksh. Newton Singh
Summary: This article presents new wormhole solutions in the framework of General Relativity. By utilizing minimal geometric deformation approach and noncommutative geometry density profiles, new asymptotically wormhole solutions are obtained. By constraining parameters, the energy-momentum tensor and positive density are obtained.
FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS
(2023)
Article
Physics, Multidisciplinary
Hina Azmat, Francisco Tello-Ortiz, M. Zubair, A. Alvarez
Summary: In this work, the incidence of gravitational decoupling in the framework of f(R, T) gravity theory is analyzed using the extended minimal geometric deformation (e-MGD) approach. The analysis is applied to a spherically symmetric and static charged isotropic matter distribution. The study examines the feasibility of the model and explores the consequences of e-MGD on relevant astrophysical parameters.
Article
Physics, Multidisciplinary
Francisco Tello-Ortiz, Pedro Bargueno, A. Alvarez, Ernesto Contreras
Summary: In this work, curved Lorentzian manifolds are generated from a flat Minkowskian space-time using the Gravitational Decoupling by the Minimal Geometric Deformation method. The decoupling sector is interpreted as a generator of curvature and matter distribution, leading to new wormhole geometries. These solutions are analyzed in detail, including their energy conditions, geometric behavior, and embedding diagrams.
FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS
(2023)
Article
Astronomy & Astrophysics
M. K. Jasim, Ksh. Newton Singh, Abdelghani Errehymy, S. K. Maurya, M. V. Mandke
Summary: In this paper, the authors explore the possibility of exact solutions for anisotropic stellar systems using the massive Brans-Dicke theory of gravity. They use the minimal geometric deformation method and the embedding class-one space-time to study anisotropic solutions for matter sources. They also analyze the physical characteristics of anisotropic celestial objects by conducting several physical tests.
Article
Astronomy & Astrophysics
J. Mestra-Paez, Alvaro Restuccia, Francisco Tello-Ortiz
Summary: We analyze the dispersion relation for an anisotropic gravity-electromagnetic theory at very high energies, focusing on highly energetic photons. The proposed anisotropic gravity-gauge vector field model, inspired by the Horava-Lifshitz anisotropic proposal, exhibits consistency and stability. In particular, we determine the exact zone where the transverse-traceless tensorial degrees of freedom and the transverse vectorial degrees of freedom propagate according to a linear wave equation, despite the presence of a non-trivial Newtonian background.
JOURNAL OF HIGH ENERGY ASTROPHYSICS
(2023)
Correction
Physics, Particles & Fields
Francisco Tello-Ortiz, S. K. Maurya, Pedro Bargueno
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Particles & Fields
S. K. Maurya, Ayan Banerjee, Anirudh Pradhan, Dhananjay Yadav
Summary: In this study, the possibility of the existence of compact charged spheres made of a charged perfect fluid in five-dimensional spacetime within the framework of Einstein-Gauss-Bonnet theory was investigated. Using a systematic and direct approach called minimal geometric deformation, it was proven that the fluid must be anisotropic and an exact and physically acceptable solution was found.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Multidisciplinary
G. Mustafa, S. K. Maurya, Saibal Ray, Faisal Javed
Summary: In this study, we investigate the geometry of wormholes in the framework of general relativity and explore how quantum wave dark matter affects the dynamical configuration of the shell surrounding the wormhole. By using specific shape functions and introducing quantum wave dark matter, we obtain reasonable wormhole solutions and observe its effects on the stability of the shell.
Article
Physics, Multidisciplinary
Pritha Dolai, Christian Maes
Summary: Calorimetry for equilibrium systems aims to determine the energy levels' occupation and distribution by measuring thermal response, while nonequilibrium versions provide additional information on the dynamical accessibility of these states. Using calculations on a driven exclusion process, it is confirmed that a fermionic nonequilibrium steady state with exact computation of specific heat can be achieved. The divergence at zero temperature occurs when the Fermi energy and the kinetic barrier for loading and emptying are approximately equal. Additionally, a stable low temperature regime of negative specific heat appears when the kinetic barrier is density-dependent, indicating an anti-correlation between the stationary occupation's temperature-dependence and excess heat.
Article
Physics, Multidisciplinary
F. F. Nascimento, V. B. Bezerra, J. M. Toledo
Summary: We obtained the metric of the Hayward black hole surrounded by a cloud of strings, and analyzed the effects of the string cloud on the regularity of the solution and the energy conditions. Various aspects such as horizons, geodesics, effective potential, and thermodynamics were investigated. We compared the obtained results with the literature corresponding to the Hayward black hole without a string cloud.