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Some of the material in is restricted to members of the community. By logging in, you may be able to gain additional access to certain collections or items. If you have questions about access or logging in, please use the form on the Contact Page.
Type Ia supernovae (SNe Ia) are rather homogeneous astrophysical objects and can be used as cosmological distance ladders. Despite that, significant diversity among SNe Ia luminosity (by a factor of ~ 10) and spectral properties have...
Observations indicate that massive stars ends their lives violently, but exactly how massive they need to be remains an astrophysical challenge. Stellar evolution predicts make two fundamental predictions about the fate of massive stars....
We performed forecasts of the uncertainty with which future surveys will measure the cosmological parameters of the non-flat ΛCDM model, extended to include the sum of neutrino masses Σν, and the effective number of relativistic species...
Understanding how massive stars explode as core-collapse supernovae (CCSN) remains an important challenge in stellar evolution theory. When massive stars reach the end of their lives, the central iron core can no longer support the...
Investigation of nuclei with neutron and proton imbalance is at the forefront of nuclear physics research today, along with how the nuclear structure varies with the movement of the nucleons. Experimental data and theoretical models work...
Reaction rates are critical in understanding the nuclear evolution of stellar environments suchas Classical Novae and Type I X-ray Bursts. Nuclear properties of the neutron-deficient nucleus 18Ne are needed to reduce uncertainties in the...
Massive stars play a crucial role in the universe. Yet, our understanding of massive stars remains incomplete due to their rarity, short lifetimes, complexity of binary interactions, and imprecise Galactic distances. An important...
Strongly correlated spin systems continue to draw significant interest due to the complex interplay between structural, charge, and spin degrees of freedom. This intricate relationship gives rise to a range of novel phenomena, such as...
Some of the material in is restricted to members of the community. By logging in, you may be able to gain additional access to certain collections or items. If you have questions about access or logging in, please use the form on the Contact Page.
