7 research outputs found
Self-forced gravitational waveforms for Extreme and Intermediate mass ratio inspirals
We present the first orbit-integrated self force effects on the gravitational
waveform for an I(E)MRI source. We consider the quasi-circular motion of a
particle in the spacetime of a Schwarzschild black hole and study the
dependence of the dephasing of the corresponding gravitational waveforms due to
ignoring the conservative piece of the self force. We calculate the cumulative
dephasing of the waveforms and their overlap integral, and discuss the
importance of the conservative piece of the self force in detection and
parameter estimation. For long templates the inclusion of the conservative
piece is crucial for gravitational-wave astronomy, yet may be ignored for short
templates with little effect on detection rate. We then discuss the effect of
the mass ratio and the start point of the motion on the dephasing.Comment: 9 pages, 15 figures. Substantially expanded and revised. We added:
description of the orbits and analysis of the dependence of the dephasing
effect on the parameter space, specifically the mass ratio and starting point
of the motion. Also added a more thorough description of out metho
The LISA Data Challenge Radler Analysis and Time-dependent Ultra-compact Binary Catalogues
Context. Galactic binaries account for the loudest combined continuous
gravitational wave signal in the Laser Interferometer Space Antenna (LISA)
band, which spans a frequency range of 0.1 mHz to 1 Hz.
Aims. A superposition of low frequency Galactic and extragalactic signals and
instrument noise comprise the LISA data stream. Resolving as many Galactic
binary signals as possible and characterising the unresolved Galactic
foreground noise after their subtraction from the data are a necessary step
towards a global fit solution to the LISA data. Methods. We analyse a simulated
gravitational wave time series of tens of millions of ultra-compact Galactic
binaries hundreds of thousands of years from merger. This data set is called
the Radler Galaxy and is part of the LISA Data challenges. We use a Markov
Chain Monte Carlo search pipeline specifically designed to perform a global fit
to the Galactic binaries and detector noise. Our analysis is performed for
increasingly larger observation times of 1.5, 3, 6 and 12 months.
Results. We show that after one year of observing, as many as ten thousand
ultra-compact binary signals are individually resolvable. Ultra-compact binary
catalogues corresponding to each observation time are presented. The Radler
Galaxy is a training data set, with binary parameters for every signal in the
data stream included. We compare our derived catalogues to the LISA Data
challenge Radler catalogue to quantify the detection efficiency of the search
pipeline. Included in the appendix is a more detailed analysis of two corner
cases that provide insight into future improvements to our search pipeline
A Gaussian-processes approach to fitting for time-variable spherical solar wind in pulsar timing data
Propagation effects are one of the main sources of noise in high-precision pulsar timing. For pulsars below an ecliptic latitude of 5°, the ionized plasma in the solar wind can introduce dispersive delays of order 100 µs around solar conjunction at an observing frequency of 300 MHz. A common approach to mitigate this assumes a spherical solar wind with a time-constant amplitude. However, this has been shown to be insufficient to describe the solar wind. We present a linear, Gaussian-process piecewise Bayesian approach to fit a spherical solar wind of time-variable amplitude, which has been implemented in the pulsar software RUN_ENTERPRISE. Through simulations, we find that the current EPTA+InPTA data combination is not sensitive to such variations; however, solar wind variations will become important in the near future with the addition of new InPTA data and data collected with the low-frequency LOFAR telescope. We also compare our results for different high-precision timing data sets (EPTA+InPTA, PPTA, and LOFAR) of 3 ms pulsars (J0030+0451, J1022+1001, J2145−0450), and find that the solar-wind amplitudes are generally consistent for any individual pulsar, but they can vary from pulsar to pulsar. Finally, we compare our results with those of an independent method on the same LOFAR data of the three millisecond pulsars. We find that differences between the results of the two methods can be mainly attributed to the modelling of dispersion variations in the interstellar medium, rather than the solar wind modelling
Bound orbits and virialized systems in a dark energy universe
It is shown that at sufficiently large radii dark energy modifies the behavior of (a) bound orbits around a galaxy, and (b) virialized gas in a cluster of galaxies. In (a), there exists a maximum circular orbit beyond which periodic motion is no longer possible, and the evolution of orbits near critical binding is analytically calculable using an adiabatic invariant integral. The finding may have application to wide galaxy pairs. In (b), dark energy necessitates the use of the generalized Virial Theorem to describe gas at the outskirts of a cluster. As a result, gas at a radius of 4 Mpc or above will readily escape. A simple model indicates that this mechanism can lead to mass loss via an outflow
Global Analysis of the Gravitational Wave Signal from Galactic Binaries
International audienceGalactic ultracompact binaries are expected to be the dominant source of gravitational waves in the milli-Hertz frequency band. Of the tens of millions of Galactic binaries with periods shorter than an hour, it is estimated that a few tens of thousand will be resolved by the future Laser Interferometer Space Antenna (LISA). The unresolved remainder will be the main source of “noise” between 1 and 3 mHz. Typical Galactic binaries are millions of years from merger, and consequently their signals will persist for the duration of the LISA mission. Extracting tens of thousands of overlapping Galactic signals and characterizing the unresolved component is a central challenge in LISA data analysis, and a key contribution to arriving at a global solution that simultaneously fits for all signals in the band. Here we present an end-to-end analysis pipeline for Galactic binaries that uses transdimensional Bayesian inference to develop a time-evolving catalog of sources as data arrive from the LISA constellation