Parkes observations for project P455 semester 2021APRS_03

This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Recent results, including the first measurements of higher-order light-propagation effects and of the relativistic deformation of the orbit, highlight the importance of a long term observational campaign for this remarkable system. The main aims of this proposal are to exploit the high sensitivity of the UWL receiver to provide the strongest tests to date for general relativity and to measure for the first time the moment-of-inertia of a neutron star. Additionally, we will search for the reappearance of the B pulsar.

本项目旨在对首个双脉冲星系统开展持续计时与脉冲轮廓研究，该系统是引力物理学研究的独特实验室。近期的研究成果——包括首次测得高阶光传播效应与轨道相对论形变——凸显了针对这一特殊天体系统开展长期观测计划的重要性。本项目申请的核心目标为：利用UWL接收机（UWL receiver）的高灵敏度，为广义相对论提供迄今为止最为严苛的检验，并首次实现对中子星转动惯量的测量。此外，我们还将搜寻B脉冲星的重现信号。