Insights from Modeling Magnetar-driven Light Curves of Stripped-envelope Supernovae

Abstract

This work presents the semi-analytical light curve modelling results of 11 stripped-envelope SNe (SESNe), where millisecond magnetars potentially drive their light curves. The light-curve modelling is performed utilizing the $\chi^2$-minimisation code $\texttt{MINIM}$ considering millisecond magnetar as a central engine powering source. The magnetar model well regenerates the bolometric light curves of all the SESNe in the sample and constrains numerous physical parameters, including magnetar's initial spin period ($P_\textrm{i}$) and magnetic field ($B$), explosion energy of supernova ($E_\textrm{exp}$), progenitor radius ($R_\textrm{p}$), etc. Within the sample, the superluminous SNe 2010kd and 2020ank exhibit the lowest $B$ and $P_\textrm{i}$ values, while the relativistic Ic broad-line SN 2012ap shows the highest values for both parameters. The explosion energy for all SESNe in the sample (except SN 2019cad), exceeding $\gtrsim$2 $\times$ 10$^{51}$ erg, indicates there is a possibility of a jittering jet explosion mechanism driving these events. Additionally, a correlation analysis identifies linear dependencies among parameters derived from light curve analysis, revealing positive correlations between rise and decay times, $P_\textrm{i}$ and $B$, $P_\textrm{i}$ and $R_\textrm{p}$, and $E_\textrm{exp}$ and $R_\textrm{p}$, as well as strong anti-correlations of $P_\textrm{i}$ and $B$ with the peak luminosity. Principal Component Analysis is also applied to key parameters to reduce dimensionality, allowing a clearer visualization of SESNe distribution in a lower-dimensional space. This approach highlights the diversity in SESNe characteristics, underscoring unique physical properties and behaviour across different events in the sample. This study motivates further study on a more extended sample of SESNe to look for millisecond magnetars as their powering source.