- DEPARTMENT_STAFF.QUALIFICATION
Ph.D
- DEPARTMENT_STAFF.DESIGNATION
Guest Faculty
- DEPARTMENT_STAFF.THRUST_AREA
Theoretical Nuclear Physics, Physics of Neutron Stars, Nuclear Astrophysics
- DEPARTMENT_STAFF.ADDRESS
C1, Azra Tower, Behind Jamia Urdu Aligarh-202002
- DEPARTMENT_STAFF.MOBILE
9634342003
- DEPARTMENT_STAFF.EMAIL
imran.phys.amu@gmail.com
- DEPARTMENT_STAFF.TIME_TABLE
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 under the supervision of Prof. Anisul Ain Usmani. My research interests are centered around strangeness nuclear physics, study of structural and decay properties of super heavy 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.
- Charge-changing cross section and interaction cross section for 4 \geq z \leq 9 isotopes
- Rotating neutron stars with quark cores
Ishfaq A. Rather, Usuf Rahaman , M. Imran, H. C. Das, A. A. Usmani, and S. K. Patra
http://dx.doi.org/10.1103/PhysRevC.103.055814
- Fully correlated variational Monte Carlo study of H-4(Lambda) and H-4(Lambda)* hypernuclei M Imran, A A Usmani, M Ikram, Z Hasan and F C Khanna
- Selient features of charge-changing cross section and interaction cross
- Constraining Bag constant for Hybrid Neutron stars Ishfaq A. Rather, Ankit Kumar, H. C. Das, M. Imran, A. A. Usmani and S. K. Patra
- A study of nuclear radii and neutron skin thickness of neutron-rich nuclei near the neutron drip line Usuf Rahaman, M. Ikram, M. Imran and A. A. Usmani
- Theoretical studies on structural properties and decay modes of (284 - 375) 119 isotopes
Asloob A Rather, M. Ikram, Ishfaq A Rather, M. Imran, A. A. Usmani, Bharat Kumar, K. P. Santhosh and S. K Patra
- 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
- Ground State Properties and Shape Evolution of Hg Isotopes within Covariant Density Functional Theory
- 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