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Physics of neutron stars: constraints from finite nuclei to gravitational waves

Implementing Organization

National Institute of Technology Rourkela
Principal Investigator
Dr Bharat Kumar
Assistant Professor
|
National Institute of Technology Rourkela
CO-Principal Investigator
Prof. Bijay Kumar Agrawal
Professor
|
Saha Institute of Nuclear Physics, Kolkata

About

This project aims to resolve some of the important issues related to finite nuclei and Neutron Stars (NS) by combining the data from terrestrial experiments and multi-messenger observations from space through theoretical studies. The project aims to investigate how the precise knowledge of nuclear physics inputs, which governs the behaviour of Equation of State (EoS) at the low-density, impact the properties of the NS.

Related Research

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Funding Organization
Funding Organization
Department of Science and Technology (DST)
Quick Information
Area of Research
Life Sciences & Biotechnology
Focus Area
Gravitation
Start Year
2022
Sanction Amount
₹ 20.53 L
Status
completed
Output
No. of Research Paper
00
Technologies (If Any)
00
No. of PhD Produced
N/A
Startup (If Any)
00
No. of Patents
Filed :00
Grant :00
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