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Dr Ningombam Chandrachani Devi

Designation: Assistant Professor

Specialization: Cosmology

Contact: 6009487525

Email: chandrachani[at]manipuruniv.ac.in or chandrachani[at]gmail.com

PhD

    • Faculty Name: Ningombam Chandrachani Devi
    • Description: Assistant Professor
    • Department: Physics
    • Phone: 6009487525
    • email: chandrachani[at]manipuruniv.ac.in or chandrachani[at]gmail.com
    • Highest Education Qualification: Ph.D
    • Specialization: Cosmology
    • Faculty Interest/Area of Interest:
Dark Energy, Dark Matter, Large Scale structures, N-body simulations, Galaxy Formation, The Early Universe, Gravitational waves, Reionization epoch
       

ORCID : 0000-0002-8939-7352

Web of Science : F-6910-2018

Details of Achievements, Memberships of different academic and professional bodies:

  • LACEGAL exchange program, Institute for Computational Cosmology, Durham University, Durham,UK (February 2019- February 2020)

  • Awarded Postdoctoral Fellowship by Direecion General de Asuntos del Personal Academico/Conacyt Fronteras Fellowship in Universidad Nacional Autonoma de Mexico, March 2016.

  • Awarded Postdoctoral Fellowship under Programa de Capacitao Institucional (PCI/ON)by Observatrio Nacional, Rio de Janeiro, Brazil, December 2012 - November 2015.

  • CSIR Senior Research Fellow, 2011-2013,Centre for Theoretical Physics, Jamia Millia Islamia, New Delhi, India

  • Major Research Project Fellow, 2008-2011, Centre for Theoretical Physics, Jamia Millia Islamia, New Delhi, India

Member, Indian Science Working Group on an Epoch of Reionization and Cosmology for Square Kilometer Array (SKA) project.

 

Some Recent Publications:

 

  1. The DESI N-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey

(arXiv:2112.09138)

  1. Testing the theory of gravity with DESI: estimators, predictions and simulation requirements (arXiv:2011.05771)

  2. Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State (arXiv:1911.02402)

  3. J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions (arXiv:1901.02540)

  4. The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function (arXiv:1901.02121)