7 citations · 7 across the 1 of their papers we have counts for
6 papers
Effects of the neutrino electromagnetic form factors on the neutrino and antineutrino mean free paths in dense matter
P. T. P. Hutauruk, A. Sulaksono, T. Mart
We have studied the effects of the nucleon weak magnetism and the neutrino electromagnetic properties on the neutrino and antineutrino mean free paths for all types of neutrinos. I…
Neutrino Electromagnetic Form Factors Effect on the Neutrino Cross Section in Dense Matter
A. Sulaksono, C. K. Williams, P. T. P. Hutauruk +1
The sensitivity of the differential cross section of the interaction between neutrino-electron with dense matter to the possibly nonzero neutrino electromagnetic properties has bee…
Relativistic Mean Field Models at High Densities
A. Sulaksono, P. T. P. Hutauruk, C. K. Williams +1
The effects of vector-isovector terms predicted by relativistic mean field models based on effective field theory on the equation of state and the neutrino mean free path in neutro…
Isovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path
A. Sulaksono, P. T. P. Hutauruk, T. Mart
An improvement in the treatment of the isovector channel of relativistic mean field (RMF) models based on effective field theory (E-RMF) is suggested, by adding an isovector scalar…
Neutrino Electromagnetic Form Factor and Oscillation Effects on Neutrino Interaction With Dense Matter
C. K. Williams, P. T. P. Hutauruk, A. Sulaksono +1
The mean free path of neutrino - free electron gas interaction has been calculated by taking into account the neutrino electromagnetic form factors and the possibility of neutrino…
Neutron Fraction and Neutrino Mean Free Path Predictions in Relativistic Mean Field Models
P. T. P. Hutauruk, C. K. Williams, A. Sulaksono +1
The equation of state (EOS) of dense matter and neutrino mean free path (NMFP) in a neutron star have been studied by using relativistic mean field models motivated by effective fi…