V. Kota

activity

20212026

S U (3)

algebras in interacting boson model and shell model: Results for

(β, γ

) bands and scissors

1^{+}

band

7 citations · 7 across the 5 of their papers we have counts for

collaborators

Showing 2025Show all

3 papers · 1 filter

hep-ph2025

Coherent and incoherent antineutrino scattering on stable even-even isotopes of molybdenum detectors

T. S. Kosmas, R. Sahu, V. K. B. Kota

The recent observations of the coherent neutrino- and antineutrino-nucleus scattering have opened up a plethora of opportunities to probe physics within standard and non-standard t…

nucl-th2025

Next highest weight and other lower $S U (3)$ irreducible representations with proxy- $S U (4)$ symmetry for nuclei with $32 \le \mbox{Z,N} \le 46$

V. K. B. Kota

In the applications of proxy-SU(3) model in the context of determining $(β, γ)$ values for nuclei across the periodic table, for understanding the preponderance of triaxial shapes i…

nucl-th2025

Statistical shell model for neutrinoless double $β$ -decay nuclear transition matrix elements: Results for $^{76}$ Ge, $^{82}$ Se, $^{100}$ Mo, $^{124}$ Sn, $^{130}$ Te and $^{136}$ Xe

V. K. B. Kota, R. Sahu

Statistical shell model (also called spectral distribution method or statistical spectroscopy method) based on random matrix theory and spherical shell model gives a theory for cal…

Coherent and incoherent antineutrino scattering on stable even-even isotopes of molybdenum detectors

Next highest weight and other lower SU(3) irreducible representations with proxy-SU(4) symmetry for nuclei with $32 \le \mbox{Z,N} \le 46$

Statistical shell model for neutrinoless double β-decay nuclear transition matrix elements: Results for 76Ge, 82Se, 100Mo, 124Sn, 130Te and 136Xe

Next highest weight and other lower $S U (3)$ irreducible representations with proxy- $S U (4)$ symmetry for nuclei with $32 \le \mbox{Z,N} \le 46$

Statistical shell model for neutrinoless double $β$ -decay nuclear transition matrix elements: Results for $^{76}$ Ge, $^{82}$ Se, $^{100}$ Mo, $^{124}$ Sn, $^{130}$ Te and $^{136}$ Xe