The last decades brought impressive progress in synthesizing and studying properties of
nuclides located very far from the beta stability line. Among the most fundamental properties …

Spectroscopy of excited states of proton-rich nuclei has advanced considerably in recent
years. This is due to recent experimental developments in the identification of nuclei …

A digital data acquisition system for the Compton suppressed clover detector array has been
implemented at the TIFR-BARC accelerator facility for the high resolution gamma ray …

A 4π multi-detector gamma-ray spectrometer named the Indian National Gamma Array
(INGA) has been set up at the Inter University Accelerator Centre, New Delhi, for nuclear …

The nuclear structure in the 100Sn region is reviewed. State-of-the-art experimental
techniques involving stable and radioactive beam facilities have enabled access to exotic …

Abstract The B (E 2; 0+→ 2+) values for the first 2+ excited states of neutron-rich 1 3 2, 1 3 4,
1 3 6 Te have been measured using Coulomb excitation of radioactive ion beams. The B (E …

The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear
reactions taking place in stars in various astrophysical conditions. These reaction rates are …

By studying the Xe 109→ Te 105→ Sn 101 superallowed α-decay chain, we observe low-
lying states in Sn 101, the one-neutron system outside doubly magic Sn 100. We find that …

In this theoretical study, we establish a correlation between the neutron skin thickness and
the nuclear symmetry energy for the even-even isotopes of Fe, Ni, Zn, Ge, Se, and Kr within …

Two new α emitters Xe 109 and Te 105 were identified through the observation of the Xe
109→ Te 105→ Sn 101 α-decay chain. The Xe 109 nuclei were produced in the fusion …