output
20032026
most citedThe NUMEN project: NUclear Matrix Elements for Neutrinoless double beta decay

183 citations

79 papers

nucl-ex2026

Probing nuclear interactions à la Rutherford: Insights on He from scattering

F. Cappuzzello, V. Soukeras, S. Bacca +27

Nuclear interactions play a key role for the stability of atomic nuclei and stellar environments. Successful parametrization and models of these interactions, developed in the last…

hep-ph2026

Double SM-like Higgs production at future colliders in the 3-Higgs Doublet Model under the symmetry

Emine Yildirim

In this paper, we present the production of double Standard Model (SM)-like Higgs at the future electron positron colliders within the framework of the model with…

hep-ph2026

Solar Neutrino Probes of Light New Physics: Updated Limits from LUX-ZEPLIN Experiment

Mehmet Demirci, M. Fauzi Mustamin

The recent low-energy electron recoil (ER) results reported by the LUX-ZEPLIN (LZ) experiment have established the most stringent constraints to date on new physics scenarios, spec…

hep-ph2025★ 3 cited

Constraining neutrino electromagnetic properties with recent low-energy electron recoil data at dark matter direct detection experiments

M. Demirci, H. I. Sezer, M. F. Mustamin +1

Neutrinos that are elastically scattered off atomic electrons provide a unique opportunity to investigate the Standard Model (SM) and beyond SM physics. In this work, we explore th…

nucl-th2025★ 2 cited

Nuclear structure properties and decay rates of molybdenum isotopes

Jameel-Un Nabi, Tuncay Bayram

Electron capture and beta-minus decay are the dominant decay processes during the late phases of the evolution of heavy stars. Previous simulation results show that weak rates on i…

nucl-th2025★ 14 cited

The nuclear ground-state properties and stellar electron emission rates of 76Fe, 78Ni, 80Zn, 126Ru, 128Pd and 130Cd using RMF and pn-QRPA models

Jameel-Un Nabi, Tuncay Bayram, Gul Daraz +2

Our study consists of investigations of nuclear ground state properties and weak transition rates of even even waiting point nuclei. The calculation was performed for N = 50 and N…