The exploration of the unique properties of stored and cooled beams of highly-charged ions
as provided by heavy-ion storage rings has opened novel and fascinating research …

Measurements of sulphur isotopes in presolar grains can help to identify the astrophysical
sites in which these grains were formed. A more precise thermonuclear rate of the 33 S (p, γ) …

High spin states of 34 Cl populated through 27 Al (12 C, α n) 34 Cl reaction at E (12 C)= 40
MeV, have been studied using the Indian National Gamma Array facility. The level scheme …

Background: The thermonuclear 34 g, m Cl (p, γ) 35 Ar reaction rates are unknown due to a
lack of experimental nuclear physics data. Uncertainties in these rates translate to …

The 33 S (p, γ) 34 Cl reaction is important for constraining predictions of certain isotopic
abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar …

Studying the nucleosynthesis in explosive astrophysical events is crucial for understanding
the origin of the elements in our solar system and the nature of nuclear matter. This thesis …

Background: The thermonuclear Cl-34g, Cl-m (p, gamma) Ar-35 reaction rates are unknown
due to a lack of experimental nuclear physics data. Uncertainties in these rates translate to …

The previous studies have shown that 33S (p, γ) 34Cl is the most important reaction that
affects the abundance of 33S in the product of nova nucleosynthesis. In this paper, a more …

Previous studies have shown that 33 S (p, γ) 34 Cl is the most important reaction that affects
the abundance of 33 S in the product of nova nucleosynthesis. In this paper, a more …

4262.0 (18) 12Ay04 12Ni01 4294.52 (10) 6− 0.23 (5) ps 12Ay04 12Ni01 90En08 98En04
4299.667 (14)< 0>+ 2 12Ni01 90En08 98En04 4315.61 (4)< 1, 2>− 12Ni01 88Pi07 …