Gravitational Radiation From Pulsar Creation

TL;DR

This paper estimates the gravitational wave signals generated during pulsar formation, focusing on how magnetic fields, temperature, and duration influence the wave amplitude across frequencies.

Contribution

It provides a novel estimation framework for gravitational wave amplitudes during pulsar creation based on key physical parameters.

Findings

Estimated gravitational wave amplitude as a function of frequency.

Identified key physical parameters affecting gravitational wave production.

Provided insights into the detectability of such signals.

Abstract

We estimate the gravitational wave amplitude as a function of frequency produced during the creation of pulsars from the gravitational collapse of a massive star. The three main quantities needed are the magnitude of the magnetic field producing pulsar kicks, the temperature which determines the velocity of the pulsar and the duration time for the gravitational radiation.res