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Published in , 2022
It is a review article of John Moffat theory of gravity
Recommended citation: Harikuamr. S 2022 , Universe 8 (2022) 5, 259
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Published in , 2025
The results we obtained could be valuable for further metric-affine gravity vs general relativity tests involving lensing of gravitational waves and comparison of luminosity distances measured from electromagnetic and gravitational wave sources.
Recommended citation: Harikumar, S. (2024). "Phys. Rev. D 109, 124014
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Published in , 2025
We introduce a novel method that is independent of the dark energy assumed in the model to investigate the mass density slopes of lensing galaxies and their redshift evolution using an extended power-law (EPL) model.
Recommended citation: A&A, 694, A196 (2025)
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Published in , 2025
This paper is about the number 1. The number 2 is left for future work.
Recommended citation: Suyamprakasam, S. (2025). "Phys.Rev.D 112 (2025) 12, 124019
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Until recently, everything we knew about the Universe came from electromagnetic waves like light in all its forms emitted by stars, galaxies, and other cosmic objects. However, observing black holes using light is extremely challenging because they do not emit light directly. In 2015, a revolutionary discovery changed the way we explore the cosmos. Scientists detected gravitational waves for the first time, tiny ripples in space and time produced when massive objects like binary black holes collide and merge. This marked the beginning of a completely new way of observing the Universe, using a messenger different from light. In this talk, I will introduce you to binary black holes and neutron stars, explain how we detect them using gravitational waves, and discuss how these observations are opening a new window onto the Universe and shaping the future of astronomy.
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The first direct detection of gravitational waves by the LIGO Scientific Collaboration in 2015 opened a completely new observational window on the Universe. Since then, gravitational wave (GW) observations have revealed merging black holes and neutron stars and have begun to transform our understanding of the most extreme objects in the cosmos.
Doctoral Studies, Room 30, Seminar Room CAMK, 2026
This course provides a introduction to gravitational waves (GWs), from their theoretical prediction in General Relativity to modern detection techniques and astrophysical applications. Students will learn the mathematical foundations of gravitational radiation, data analysis methods, gravitational lensing and the scientific discoveries enabled by current GW observatories.