- Qualification
Ph.D
- Designation
Guest Faculty
- Thrust Area
Theoretical Nuclear Physics, Physics of Neutron Stars, Nuclear Astrophysics
- Address
C1, Azra Tower, Behind Jamia Urdu Aligarh-202002
- Mobile
9634342003
- Email
imran.phys.amu@gmail.com
- Time Table
Time Table (Even Semester) 2025-26Time Table (Even Semester) 2024-25
I did B.Sc. (Hons) Physics and M.Sc. Physics from Aligarh Muslim University, Aligarh and also obtained PhD in Theoretical Nuclear Physics from Aligarh Muslim University, Aligarh, India. My research interests are centered around strangeness nuclear physics, study of structural and decay properties of nuclei and superheavy nuclei, and nuclear astrophysics. Currently, I am working on nuclear astrophysics mainly focusing on the neutron stars equation of state (EoS). Using the Relativistic Mean Field theory (RMF), we are trying to constrain the neutron star EoS and also studying the possible presence of exotic phases like quarks, kaons, and hyperons in neutron stars.
- On energy-dependent scaling factor for the charge-changing cross sections of light elements (IF=2.5)
- Theoretical investigation of charge-changing cross section and interaction cross section for Be, B, C, N, O, and F isotopes on 12C at 200-1050 MeV/nucleon (IF=3.4)
- Theoretical Investigation of {\alpha} -decay in Heavy and Superheavy Isomers (IF=1.013)
- Charge-changing cross section and interaction cross section for 4 \geq z \leq 9 isotopes (IF=3.4))
- Theoretical studies on structural properties and decay modes of (284 - 375) 119 isotopes (IF=2.9)
- Rotating neutron stars with quark cores (IF=3.4)
- A study of nuclear radii and neutron skin thickness of neutron-rich nuclei near the neutron drip (IF-1.103) line
- Constraining Bag constant for Hybrid Neutron stars (IF=1.013)
- Fully correlated variational Monte Carlo study of H-4(Lambda) and H-4(Lambda)* hypernuclei (IF=3.6)
- Ground State Properties and Shape Evolution of Hg Isotopes within Covariant Density Functional Theory
- Theoretical Investigation of Probable Decay Modes in Superheavy Nuclei from Z = 121-126
- Matter radii of Be isotopes using 2pF density distribution
- Relativistic mean-field study of neutron skin thickness and charge radii of $^{118-134}Sn$ isotopes
- Charge symmetry breaking in (lambda) He4 - (lambda) H4 hypernuclei
- GW190814 secondary component as massively rotating hybrid star
- Role of Hyperons in Neutron stars
- Behaviour of the Potentials due to Strangeness degree of freedom in $_{\Lambda}^{4}$H and. . $_{\Lambda}^{4}$H$^${*} Hypernuclei
- Role of Space-Exchange Correlation in Light Hypernuclei
M. Imran, M. Ikram, Asloob A. Rather, Z. Hasan and A. A. Usmani
http://www.sympnp.org/proceedings/61/A125.pdf
- Spin-Orbit Interaction Potential in Nuclei and Hypernuclei