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Ksh. Newton Singh

Associate Professor

University of Delhi

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Research Interests

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Articles (20)

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Collaborators (2)

Akram Ali

Professor

king khalid university

SAUDI ARABIA

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Bivudutta Mishra

Professor

Birla Institute of Technology and Science, Pilani - Hyderabad Campus

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Ksh. Newton Singh

Research Interests

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Articles (20)

Realistic neutron star structures and tidal deformability in f(R,Lm,T) gravity with modified Chaplygin-type equation of state

Implications of Matter–Curvature Coupled Gravity on Chandrasekhar Mass Limit of White Dwarfs

Stability of neutron stars in f(Q,T) gravity

Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows

Tidal deformability of neutron stars with exotic equation of state in f(R,Lm)−gravity

Constraining parameters of Einstein–Power–Maxwell black hole from M87* and Sgr A* data and frequencies analysis with particle dynamics

Compact star models with power-law and nonlinear f(R,Lm)−gravity

Quantum-corrected slowly rotating wormholes: Frame dragging, photon rings, and shadows

Constraining f(R,Lm,T) gravity with millisecond pulsar observations

Observational constraints on f(Q, T) gravity from the mass-radius relation and stability of compact stars

On perturbation induced minimal geometric decoupling in spacetime and its impact on mass-gap stability: Insights from the binary mergers GW190814, GW200210, and millisecond pulsars PSR J1614-2230 and PSR J0952-0607

Realistic modeling of neutron star structures with linear and non-linear matter-curvature coupling in f(R,Lm,T)− gravity using SLy4, Togashi, and Walecka equation of state

Influence of dark matter induced by gravitational decoupling on maximum mass and stability of compact stars and understanding the mass gap phenomenon

Relativistic massive compact stars supported by decoupled matter: implications for mass-radius bounds

Constraining radii and stability of neutron stars in 4D Einstein–Gauss–Bonnet gravity

Effects of matter and non-metricity couplings on the structure of neutron stars

Role of gravitational decoupling on theoretical insights of relativistic massive compact stars in the mass gap

Stability of compact stars in a uniform density background cloud

Influence of pressure anisotropy on mass-radius relation and stability of millisecond pulsars in f(Q) gravity

Modeling Compact Object Mergers GW190814 and GW200210 and Other Self-bound Compact Stars with Dark Matter Induced by Gravitational Decoupling and Its Significance to the Mass Gap

Collaborators (2)

Akram Ali

Bivudutta Mishra

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