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Abdel Magied Abdel Diab (Modern University for Information – MTI)09/09/2020, 13:30Talk
Based on quantum mechanical framework for the minimal length uncertainty, we demonstrate that the generalized uncertainty principle (GUP) parameter - on one hand - could be best constrained by recent gravitational waves observations, and - on other hand - suggest modified dispersion relations (MDRs) to calculate the difference between the group velocity of gravitons and that of photons....
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Abdel Nasser Tawfik (Nile University – NU)09/09/2020, 13:37Talk
When minimal length uncertainty emerging from generalized uncertainty principle (GUP) is thoughtfully implemented, it is of great interest to consider its impacts on Einstein’s gravitational field equations (EFE) and to find out whether the corresponding modification in the metric manifests properties of quantum geometry due to quantum gravity. GUP takes into account the gravitational impacts...
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Alejandro Cabo Montes de Oca (Instituto de Cibernética, Matemática y Física – ICIMAF)09/09/2020, 13:44Talk
Static (not stationary) solutions of the Einstein-Klein-Gordon (EKG) equations including matter are obtained for real scalar fields. The scalar field interaction with matter is considered. The introduced coupling allows the existence of static solutions in contraposition with the case of the simpler EKG equations for real scalar fields and gravity. Surprisingly, when the considered matter is a...
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Encieh Erfani (Institute for Advanced Studies in Basic Sciences)09/09/2020, 13:51Talk
With the discovery of gravitational waves from merging pairs of massive black holes, the interest in the question of whether Primordial Black Holes (PBHs) could constitute the Dark Matter (DM) has recently been revived. In this talk, I will review the different mechanisms for (DM) PBHs formation with a focus on inflation which can source the required large density fluctuations for PBHs...
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Igor Kulikov (ICMMG SB RAS)09/09/2020, 13:58Talk
A new code to simulate special relativistic hydrodynamic flows on supercomputer architectures with distributed memory is described. The code is based on a combination of Godunov's method and a piecewise parabolic method with a local stencil. This approach has good conservation properties, correctly reproduces shock waves, and ensures high accuracy on smooth solutions and low dissipation on...
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Lijing Shao (Peking University)09/09/2020, 14:05Talk
In Einstein’s general relativity, gravity is mediated by a massless metric field. The extension of general relativity to consistently include a mass for the graviton has profound implications for gravitation and cosmology. Salient features of various massive gravity theories can be captured by Galileon models, the simplest of which is the cubic Galileon. The presence of the Galileon field...
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Dr Surajit Chattopadhyay (Amity University, Kolkata)09/09/2020, 14:12Talk
Late time accelerated expansion of the Universe is well documented in the literature. An exotic matter, characterized by negative pressure is considered to be the driving force behind this late time acceleration of the Universe and it is dubbed as dark energy (DE). The negative pressure p leads to negative equation of state (EoS) parameter w = p/ρ, where ρ is the density of the Universe. In...
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Violetta Sagun (University of Coimbra)09/09/2020, 14:19Talk
We study an impact of asymmetric dark matter on properties of the neutron stars and their ability to reach the two solar masses limit, which allows us to present a new range of masses of dark matter particles and their fractions inside the star. Our analysis is based on the observational fact of the existence of three pulsars reaching this limit and on the theoretically predicted reduction of...
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Zhi-Fu Gao (Xinjiang Astronomical Observatory, Chinese Academy of Sciences)09/09/2020, 14:26Talk
Magnetars are a kind of pulsars powered mainly by superhigh magnetic fields. They are popular sources with many unsolved issues in themselves, but also linked to various high-energy phenomena, such as Quasi-periodic oscillation, giant flares, fast radio bursts and super-luminous supernovae. In this presentation, combining with the latest EoSs, we first introduce the eigen equations of Ohmic...
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Violetta Sagun (University of Coimbra)Poster
We study the thermal evolution of neutron stars described within the equation of state with induced surface tension (IST) that reproduces properties of normal nuclear matter, fulfills the proton flow constraint, provides a high-quality description of hadron multiplicities created during the nuclear-nuclear collision experiments, and is equally compatible with the constraints from astrophysical...
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Prof. Gao Zhifu (Xinjiang Astronomical Observatory, Chinese Academy of Sciences)Poster
It is of great importance to study the properties of a proto-neutron star (PNS) because of its complex evolution into a cold NS. Under the framework of relativistic mean field theory, the repulsion and attraction between hyperons and hyperons are considered simultaneously. In addition, the hyperon-meson couplings satisfy SU(6) symmetry. By considering entropy, temperature and neutrino,...
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Yong Gao (Peking University)Poster
A rapidly rotating, asymmetric neutron star (NS) in the Milky Way undergoes free precession,making it a potential source for multi-messenger observation. The free precession could manifest in (i) the spectra of continuous gravitational waves (GWs), and (ii) the timing behavior and pulse-profile of radio and/or X-ray pulsars. We extend previous work and investigate in...
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