The Role of $r$-Modes in Pulsar Spindown, Pulsar Timing and Gravitational Waves
We investigate the role of r-modes in the spin-down of pulsars, focusing on their implications for pulsar timing and gravitational wave emissions. Our study employs a non-linear differential equation incorporating the contribution of r-modes to derive time-dependent rotational frequency and period f...
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Main Authors | , , , , |
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Format | Journal Article |
Language | English |
Published |
20.07.2023
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Subjects | |
Online Access | Get full text |
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Summary: | We investigate the role of r-modes in the spin-down of pulsars, focusing on
their implications for pulsar timing and gravitational wave emissions. Our
study employs a non-linear differential equation incorporating the contribution
of r-modes to derive time-dependent rotational frequency and period functions.
This model is validated against observational data from the Crab pulsar,
demonstrating a high degree of accuracy. By fitting the braking indices and
spin-down coefficients, we establish direct and analytical relationships
between observable pulsar properties and weak gravitational wave signals. We
also derive analytical expressions for neutron star compactness and tidal
deformability using Lambert W solutions, independent of the equation of state
(EoS). These solutions provide new insights into the mathematical relationships
between physical quantities, constraining the parameter space for r-mode
gravitational wave frequency searches. Our results show that incorporating
r-modes significantly enhances our ability to measure the neutron star EoS and
predict pulsar age, rotational velocity, and gravitational wave frequencies.
The seventh-order approximation used in our model is essential for accurately
capturing the contributions of r-modes to the spin-down process. This framework
can be applied to model pulsar timing residuals, account for glitches, and
improve the detection and analysis of continuous gravitational waves from
pulsars. With the advent of next-generation gravitational wave detectors, our
findings offer promising prospects for disentangling individual events from the
stochastic gravitational wave background, advancing our understanding of
neutron star interiors and their dynamic processes. |
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DOI: | 10.48550/arxiv.2307.11270 |