Cosmological and Gravitational Wave Signatures of Particle Dark Matter Models - RA-I
Department of Physics, IIT Guwahati.
Assam - Guwahati, Assam, India
This application has expired
The last date to apply was 12 Jul 2026. Applications are no longer accepted for this post.
Vacancies
1
Salary
Rs. 58000 - Rs. 58000
Last Date
12 Jul 2026
⚠ Please verify all details (dates, eligibility, vacancies) from the official notification before applying. Rojgarpulse is an information aggregator and not a government body.
Important Dates
Salary / Pay Scale
Rs. 58000 - Rs. 58000
Eligibility
Eligibility criteria not specified here. See official notification.
Qualification / Education
Full Description
Project: Cosmological and
Gravitational Wave Signatures of Particle Dark Matter Models | Designation: RA-I | Interview Date: 2026-07-14 | Last Date to Apply: 2026-07-12 | Qualifications: See PDF for detailed qualifications
Important Links
Applications Closed
Last date has passed
Download Notification
https://www.iitg.ac.in/iitg_reqr_details.php?p=4233/advertisement-for-project-positions-in-the-department-of-physics-iit-guwahati-2627r-0192-phys1152dedb-
Official Website
https://www.iitg.ac.in/iitg_reqr_details.php?p=4233/advertisement-for-project-positions-in-the-department-of-physics-iit-guwahati-2627r-0192-phys1152dedb-
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Frequently Asked Questions
What is Cosmological and Gravitational Wave Signatures of Particle Dark Matter Models - RA-I?
Cosmological and Gravitational Wave Signatures of Particle Dark Matter Models - RA-I is a government recruitment notification published by Department of Physics, IIT Guwahati.. Apply before the last date to be considered.
When does the application start?
Online applications start on 10 July 2026.
What is the last date to apply?
The last date to submit the application is 12 July 2026.
What is the required qualification?
See PDF for detailed qualifications
How do I apply?
Apply online through the official link provided on Rojgarpulse. Always verify details from the official notification before applying.