Deriving fundamental parameters of millisecond pulsars via AIC in white dwarfs

TL;DR

This paper investigates millisecond pulsars' properties by analyzing their magnetic fields, spin periods, and masses through the AIC process of white dwarfs, revealing evolutionary links between neutron stars and white dwarfs in binary systems.

Contribution

It introduces a method to derive MSP parameters using AIC in white dwarfs, enhancing understanding of MSP population characteristics and their evolutionary connection to neutron stars.

Findings

MSPs' magnetic fields, spin periods, and masses are characterized.

A strong evolutionary link between neutron stars and white dwarfs is demonstrated.

The AIC scenario effectively explains MSP observational properties.

Abstract

We present a study of the observational properties of Millisecond Pulsars (MSPs) by way of their magnetic fields, spin periods and masses. These measurements are derived through the scenario of Accretion Induced Collapse (AIC) of white dwarfs (WDs) in stellar binary systems, in order to provide a greater understanding of the characteristics of MSP populations. In addition, we demonstrate a strong evolutionary connection between neutron stars and WDs with binary companions from a stellar binary evolution perspective via the AIC process.