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Dr. Himanshu Sekhar Sahoo

Dr. Himanshu Sekhar Sahoo

Assistant Professor

Qualification

  • Ph.D. (Physics), Ravenshaw University, Cuttack
  • M.Phil. (Physics), Ravenshaw University, Cuttack
  • M.Sc.(Physics), Banaras Hindu University, Varanasi
  • B.Sc. (Physics), Ravenshaw University, Cuttack

What subject you teach at SSU ?

  • Mathematical Physics
  • Computational Physics
  • Atomic & Molecular Spectroscopy

Awards

  • CSIR-SRF (2018)
  • Best Poster Award, 60th DAE-BRNS Symposium on Nuclear Physics-2015
  • Best Record of Publication-2018, Ravenshaw University, Cuttack

Interests

  • Nuclear Astrophysics,
  • Neutron Star Equation of State
  • Dense Matter Physics

Journals

1. Hybrid stars in a relativistic quark model, G. Mitra, H. S. Sahoo, R. N Mishra and P. K. Panda, Phys. Rev. C 105, 045802 (2022).
2. Symmetry energy dilemma within a relativistic quark model, H. S. Sahoo, S. Karan, R. N. Mishra and P. K. Panda, Phys. Rev. C 104, 055805 (2021).
3. Neutron star matter with strange interactions within constraints by GW170817 in a relativistic quark model, H. S. Sahoo, R. N.Mishra, D. K. Mohanty, P. K. Panda and N. Barik, Phys. Rev. C 99, 055803 (2019).
4. Neutron star matter with Δ isobars in a relativistic quark model, H. S. Sahoo, G. Mitra, R. N.Mishra, P. K. Panda and B. A. Li, Phys. Rev. C 98, 045801 (2018).
5. Hyperon stars in a modified quark meson coupling model, R. N. Mishra, H. S. Sahoo, P. K. Panda, N. Barik and T. Frederico, Phys. Rev. C 94, 035805 (2016); Erratum: Phys. Rev. C 98, 019903(E) (2018).
6. Nuclear symmetry energy in a modified quark meson coupling model, R. N. Mishra, H. S. Sahoo, P. K. Panda, N. Barik and T. Frederico, Phys. Rev. C 92, 045203 (2015).

Conference Proceedings:
1. Delta Matter in Neutron Stars in a Relativistic Quark Model, Proc. 13th Int. Conf. on Nucleus-Nucleus Collisions, JPS Conf. Proc. 32, 010054 (2020). [https://doi.org/10.7566/JPSCP.32.010054].
2. Compact Stars with Strange Interactions in a Modified Quark Meson Coupling Model (MQMC), Proc. 13th Int. Conf. on Nucleus-Nucleus Collisions, JPS Conf. Proc. 32, 010053 (2020). [https://doi.org/10.7566/JPSCP.32.010053].
3. Role of potential in neutron star matter in MQMC, Proceedings of the DAE-BRNS Symp. on Nucl. Phys. 63 (2018), Pg- 798.
4. Effects of strangeness on the Mass-Radius of neutron stars in MQMC, Proceedings of the DAE-BRNS Symp. on Nucl. Phys. 62 (2017), Pg- 718.
5. Effects of baryon in hyperon stars in a modified quark meson coupling model, Proceedings of the DAE-BRNS Symp. on Nucl. Phys. 61 (2016), Pg- 898.
6. Compact stars in a modified quark meson coupling model, Proceedings of the DAE-BRNS Symp. on Nucl. Phys. 60 (2015), Pg- 874.
7. Neutron star matter in a modified quark meson coupling model, Proceedings of the National Seminar on Ballistics-A Multi-disciplinary physical science, (2015), ISBN:978-2-642-24819-5, Pg 56.
8. Asymmetric nuclear matter in a modified quark meson coupling model, Proceedings of the DAE Symp. on Nucl. Phys. 59 (2014), Pg – 792

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