1,535 research outputs found
Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors
We present a review of modern optical techniques being used and developed for the field of gravitational wave detection. We describe the current state-of-the-art of gravitational waves detector technologies with regard to optical layouts, suspensions and test masses. We discuss the dominant sources and noise in each of these subsystems and the developments that will help mitigate them for future generations of detectors. We very briefly summarise some of the novel astrophysics that will be possible with these upgraded detectors
The declining representativeness of the British party system, and why it matters
In a recent article, Michael Laver has explained ‘Why Vote-Seeking Parties May Make Voters Miserable’. His model shows that, while ideological convergence may boost congruence between governments and the median voter, it can reduce congruence between the party system and the electorate as a whole. Specifically, convergence can increase the mean distance between voters and their nearest party. In this article we show that this captures the reality of today’s British party system. Policy scale placements in British Election Studies from 1987 to 2010 confirm that the pronounced convergence during the past decade has left the Conservatives and Labour closer together than would be optimal in terms of minimising the policy distance between the average voter and the nearest major party. We go on to demonstrate that this comes at a cost. Respondents who perceive themselves as further away from one of the major parties in the system tend to score lower on satisfaction with democracy. In short, vote-seeking parties have left the British party system less representative of the ideological diversity in the electorate, and thus made at least some British voters miserable
'Word from the street' : when non-electoral representative claims meet electoral representation in the United Kingdom
Taking the specific case of street protests in the UK – the ‘word from the street’– this article examines recent (re)conceptualizations of political representation, most particularly Saward’s notion of ‘representative claim’. The specific example of nonelectoral claims articulated by protestors and demonstrators in the UK is used to illustrate: the processes of making, constituting, evaluating and accepting claims for and by constituencies and audiences; and the continuing distinctiveness of claims based upon electoral representation. Two basic questions structure the analysis: first, why would the political representative claims of elected representatives trump the nonelectoral claims of mass demonstrators and, second, in what ways does the ‘perceived legitimacy’ of the former differ from the latter
Inferring Core-Collapse Supernova Physics with Gravitational Waves
Stellar collapse and the subsequent development of a core-collapse supernova
explosion emit bursts of gravitational waves (GWs) that might be detected by
the advanced generation of laser interferometer gravitational-wave
observatories such as Advanced LIGO, Advanced Virgo, and LCGT. GW bursts from
core-collapse supernovae encode information on the intricate multi-dimensional
dynamics at work at the core of a dying massive star and may provide direct
evidence for the yet uncertain mechanism driving supernovae in massive stars.
Recent multi-dimensional simulations of core-collapse supernovae exploding via
the neutrino, magnetorotational, and acoustic explosion mechanisms have
predicted GW signals which have distinct structure in both the time and
frequency domains. Motivated by this, we describe a promising method for
determining the most likely explosion mechanism underlying a hypothetical GW
signal, based on Principal Component Analysis and Bayesian model selection.
Using simulated Advanced LIGO noise and assuming a single detector and linear
waveform polarization for simplicity, we demonstrate that our method can
distinguish magnetorotational explosions throughout the Milky Way (D <~ 10kpc)
and explosions driven by the neutrino and acoustic mechanisms to D <~ 2kpc.
Furthermore, we show that we can differentiate between models for rotating
accretion-induced collapse of massive white dwarfs and models of rotating iron
core collapse with high reliability out to several kpc.Comment: 22 pages, 9 figure
Inference on inspiral signals using LISA MLDC data
In this paper we describe a Bayesian inference framework for analysis of data
obtained by LISA. We set up a model for binary inspiral signals as defined for
the Mock LISA Data Challenge 1.2 (MLDC), and implemented a Markov chain Monte
Carlo (MCMC) algorithm to facilitate exploration and integration of the
posterior distribution over the 9-dimensional parameter space. Here we present
intermediate results showing how, using this method, information about the 9
parameters can be extracted from the data.Comment: Accepted for publication in Classical and Quantum Gravity, GWDAW-11
special issu
Status of the GEO600 gravitational wave detector
The GEO600 laser interferometric gravitational wave detector is approaching the end of its commissioning phase which started in 1995.During a test run in January 2002 the detector was operated for 15 days in a power-recycled michelson configuration. The detector and environmental data which were acquired during this test run were used to test the data analysis code. This paper describes the subsystems of GEO600, the status of the detector by August 2002 and the plans towards the first science run
On the complementarity of pulsar timing and space laser interferometry for the individual detection of supermassive black hole binaries
Gravitational waves coming from Super Massive Black Hole Binaries (SMBHBs)
are targeted by both Pulsar Timing Array (PTA) and Space Laser Interferometry
(SLI). The possibility of a single SMBHB being tracked first by PTA, through
inspiral, and later by SLI, up to merger and ring down, has been previously
suggested. Although the bounding parameters are drawn by the current PTA or the
upcoming Square Kilometer Array (SKA), and by the New Gravitational Observatory
(NGO), derived from the Laser Interferometer Space Antenna (LISA), this paper
also addresses sequential detection beyond specific project constraints. We
consider PTA-SKA, which is sensitive from 10^(-9) to p x 10^(-7) Hz (p=4, 8),
and SLI, which operates from s x 10^(-5) up to 1 Hz (s = 1, 3). A SMBHB in the
range 2x 10^(8) - 2 x 10^(9) solar masses (the masses are normalised to a (1+z)
factor, the red shift lying between z = 0.2 and z=1.5) moves from the PTA-SKA
to the SLI band over a period ranging from two months to fifty years. By
combining three Super Massive Black Hole (SMBH)-host relations with three
accretion prescriptions, nine astrophysical scenarios are formed. They are then
related to three levels of pulsar timing residuals (50, 5, 1 ns), generating
twenty-seven cases. For residuals of 1 ns, sequential detection probability
will never be better than 4.7 x 10^(-4) y^(-2) or 3.3 x 10^(-6) y^(-2) (per
year to merger and per year of survey), according to the best and worst
astrophysical scenarios, respectively; put differently this means one
sequential detection every 46 or 550 years for an equivalent maximum time to
merger and duration of the survey. The chances of sequential detection are
further reduced by increasing values of the s parameter (they vanish for s =
10) and of the SLI noise, and by decreasing values of the remnant spin. REST OF
THE ABSTRACT IN THE PDF FILE.Comment: To appear in the Astrophysical Journa
Report on the first round of the Mock LISA Data Challenges
The Mock LISA Data Challenges (MLDCs) have the dual purpose of fostering the
development of LISA data analysis tools and capabilities, and demonstrating the
technical readiness already achieved by the gravitational-wave community in
distilling a rich science payoff from the LISA data output. The first round of
MLDCs has just been completed: nine data sets containing simulated
gravitational wave signals produced either by galactic binaries or massive
black hole binaries embedded in simulated LISA instrumental noise were released
in June 2006 with deadline for submission of results at the beginning of
December 2006. Ten groups have participated in this first round of challenges.
Here we describe the challenges, summarise the results, and provide a first
critical assessment of the entries.Comment: Proceedings report from GWDAW 11. Added author, added reference,
clarified some text, removed typos. Results unchanged; Removed author, minor
edits, reflects submitted versio
Exploring sex differences in attitudes towards the descriptive and substantive representation of women
This article unpacks the rationales that might be behind individual-level support for the idea that there ought to be more women present in political institutions. We outline two distinct rationales: the substantive position that sees an increase in women’s descriptive representation as important in bringing about a subsequent improvement in women’s substantive representation, or the justice-plus position that sees an increase in the descriptive representation of women as important for reasons of justice or other symbolic benefits. We find that women are more likely than men to support an increase in descriptive representation and that women are more likely to hold both the view that an increase in descriptive representation was desirable and that such an increase would improve the representation of women’s political interests. Men are found to be more likely to support an increase in descriptive representation but not relate descriptive representation to substantive representation in any way: the justice-plus rationale
The Sensitivity of the Parkes Pulsar Timing Array to Individual Sources of Gravitational Waves
We present the sensitivity of the Parkes Pulsar Timing Array to gravitational
waves emitted by individual super-massive black-hole binary systems in the
early phases of coalescing at the cores of merged galaxies. Our analysis
includes a detailed study of the effects of fitting a pulsar timing model to
non-white timing residuals. Pulsar timing is sensitive at nanoHertz frequencies
and hence complementary to LIGO and LISA. We place a sky-averaged constraint on
the merger rate of nearby () black-hole binaries in the early phases
of coalescence with a chirp mass of 10^{10}\,\rmn{M}_\odot of less than one
merger every seven years. The prospects for future gravitational-wave astronomy
of this type with the proposed Square Kilometre Array telescope are discussed.Comment: fixed error in equation (4). [13 pages, 6 figures, 1 table, published
in MNRAS
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