Search Results - "Malik, Tuhin"

Bayesian evaluation of hadron-quark phase transition models through neutron star observables in light of nuclear and astrophysics data by Guha Roy, Debanjan, Venneti, Anagh, Malik, Tuhin, Bhattacharya, Swastik, Banik, Sarmistha

“…We investigate the role of hybrid and nucleonic equations of state (EOSs) within neutron star (NS) interiors using Bayesian inference to evaluate their…”
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Analysis of Neutron Star f-mode Oscillations in General Relativity with Spectral Representation of Nuclear Equations of State by Guha Roy, Debanjan, Malik, Tuhin, Bhattacharya, Swastik, Banik, Sarmistha

“…Abstract We study quasi-normal f -mode oscillations in neutron star (NS) interiors within a linearized general relativistic formalism. We utilize approximately…”
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New equation of state involving Bose–Einstein condensate of antikaon for supernova and neutron star merger simulations by Malik, Tuhin, Banik, Sarmistha, Bandyopadhyay, Debades

“…We compute a new equation of state table including Bose–Einstein condensate of K - mesons for core collapse supernova and neutron star merger simulations…”
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Towards Uncovering Dark Matter Effects on Neutron Star Properties: A Machine Learning Approach by Thakur, Prashant, Malik, Tuhin, Jha, Tarun Kumar

“…Over the last few years, researchers have become increasingly interested in understanding how dark matter affects neutron stars, helping them to better…”
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Constraining nuclear matter parameters from correlation systematics: a mean-field perspective by Agrawal, B. K., Malik, Tuhin, De, J. N., Samaddar, S. K.

“…The nuclear matter parameters define the nuclear equation of state (EoS), they appear as coefficients of expansion around the saturation density of symmetric…”
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Inner crust equations of state for CompOSE by Malik, Tuhin, Pais, Helena

“…In this paper, we present some relativistic mean-field inner crust equations of state that have recently been uploaded in the CompOSE online repository. These…”
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Equation-of-state Table with Hyperon and Antikaon for Supernova and Neutron Star Merger by Malik, Tuhin, Banik, Sarmistha, Bandyopadhyay, Debades

“…Abstract We develop a new equation-of-state (EOS) table involving thermal (anti)kaons, Bose–Einstein condensate of K − mesons, and Λ-hyperons for core-collapse…”
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Relativistic Description of Dense Matter Equation of State and Compatibility with Neutron Star Observables: A Bayesian Approach by Malik, Tuhin, Ferreira, Márcio, Agrawal, B. K., Providência, Constança

“…Abstract The general behavior of the nuclear equation of state (EOS), relevant for the description of neutron stars (NSs), is studied within a Bayesian…”
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An Equation of State for Magnetized Neutron Star Matter and Tidal Deformation in Neutron Star Mergers by Patra, N. K., Malik, Tuhin, Sen, Debashree, Jha, T. K., Mishra, Hiranmaya

“…We derive an equation of state (EOS) for magnetized charge-neutral nuclear matter relevant for a neutron star (NS). The calculations are performed within an…”
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Equation of State for Dense Matter from Finite Nuclei to Neutron Star Mergers by Malik, Tuhin

“…Equation of state (EOS) of dense matter has been constrained from the experimental data available on the properties of finite nuclei and neutron stars. Towards…”
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Bayesian inference of signatures of hyperons inside neutron stars by Malik, Tuhin, Providência, Constança

“…The possible signatures of the presence of hyperons inside neutron stars are discussed within a Bayesian inference framework applied to a set of models based…”
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Inner crust equations of state for CompOSE by Malik, Tuhin, Pais, Helena

“…In this paper, we present some relativistic mean-field inner crust equations of state that have recently been uploaded in the CompOSE online repository. These…”
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Astrophysics and Nuclear Physics Informed Interactions in Dense Matter: Inclusion of PSR J0437-4715 by Malik, Tuhin, Dexheimer, Veronica, Providência, Constança

“…Phys.Rev.D 110 (2024) 4, 043042 We investigate how vector-isoscalar and vector-isovector interactions can be determined within the density regime of neutron…”
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The footprint of nuclear saturation properties on the neutron star $f$ mode oscillation frequencies: a machine learning approach by Kumar, Deepak, Malik, Tuhin, Mishra, Hiranmaya

“…We investigate the intricate relationships between the non-radial \(f\) mode oscillation frequencies of neutron stars (NS)s and the corresponding nuclear…”
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Unified neutron star equations of state calibrated to nuclear properties by Malik, Tuhin, Pais, Helena, Providência, Constança

“…A&A 689, A242 (2024) Recently, in Malik23, a dataset of several EoS for purely nucleonic stellar matter based on a non-linear RMF model prescription, and…”
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Towards Uncovering Dark Matter Effects on Neutron Star Properties: A Machine Learning Approach by Thakur, Prashant, Malik, Tuhin, Jha, T. K

“…Particles 2024, 7(1), 80-95 In recent years, researchers have become increasingly interested in understanding how dark matter affects neutron stars, helping…”
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Unveiling a universal relationship between the f(R) parameter and neutron star properties by Nobleson, K, Banik, Sarmistha, Malik, Tuhin

“…In recent years, modified gravity theories have gained significant attention as potential replacements for the general theory of relativity. Neutron stars,…”
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Constraining the high-density behavior of nuclear symmetry energy with direct Urca processes by Boukari, Olfa, Malik, Tuhin, Rabhi, Aziz, Providência, Constança

“…The density dependence of the symmetry energy in relativistic mean-field models with density dependent couplings is discussed in terms of the possible opening…”
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Hybrid Star Properties with NJL and MFTQCD Model: A Bayesian Approach by Albino, Milena, Malik, Tuhin, Ferreira, Márcio, Providência, Constança

“…The composition of the core of neutron stars is still under debate. One possibility is that because of the high densities reached in their cores, matter could…”
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Realizing the potential of deep neural network for analyzing neutron star observables and dense matter equation of state by Thete, Ameya, Banerjee, Kinjal, Malik, Tuhin

“…Phys.Rev.D 108 (2023) 6, 063028 The difficulty in describing the equation of state (EoS) for nuclear matter at densities above the saturation density…”
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