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We discuss observational strategies to detect prompt bursts associated with gravitational wave (GW) events using the Australian Square Kilometre Array Pathfinder (ASKAP). Many theoretical models of binary neutron stars mergers predict that bright, prompt radio emission would accompany the merger. The detection of such prompt emission would greatly improve our knowledge of the physical conditions, environment, and location of the merger. However, searches for prompt emission are complicated by the relatively poor localisation for GW events, with the 90% credible region reaching hundreds or even thousands of square degrees. Operating in fly’s eye mode, the ASKAP field of view can reach
$\sim1\,000$ deg$^2$ at $\sim$$888\,{\rm MHz}$. This potentially allows observers to cover most of the 90% credible region quickly enough to detect prompt emission. We use skymaps for GW170817 and GW190814 from LIGO/Virgo’s third observing run to simulate the probability of detecting prompt emission for GW events in the upcoming fourth observing run. With only alerts released after merger, we find it difficult to slew the telescope sufficiently quickly as to capture any prompt emission. However, with the addition of alerts released before merger by negative-latency pipelines, we find that it should be possible to search for nearby, bright prompt fast radio burst-like emission from GW events. Nonetheless, the rates are low: we would expect to observe $\sim$0.012 events during the fourth observing run, assuming that the prompt emission is emitted microseconds around the merger.
The modern Very Long Baseline Interferometry (VLBI) relativistic delay model, as documented in the IERS Conventions, refers to the time epoch when the signal passes one of two stations of an interferometer baseline (selected arbitrarily from the pair of stations and called the ‘reference station’ or ‘station 1’). This model consists of the previous correlation procedure used before the year 2002. However, since 2002 a new correlation procedure that produces the VLBI group delays referring to the time epoch of signal passage at the geocenter has been used. A corresponding correction to the conventional VLBI model delay has to be introduced. However, this correction has not been thoroughly presented in peer reviewed journals, and different approaches are used at the correlators to calculate the final group delays officially published in the IVS database. This may cause an inconsistency up to 6 ps for ground-based VLBI experiments between the group delay obtained by the correlator and the geometrical model delay from the IERS Conventions used in data analysis software. Moreover, a miscalculation of the signal arrival moment to the ‘reference station’ could result in a larger modelling error (up to 50 ps). The paper presents the justification of the correction due to transition between two epochs elaborated from the Lorentz transformation and the approach to model the uncertainty of the calculation of the signal arrival moment. Both changes are particularly essential for upcoming broadband technology geodetic VLBI observations.
The Rapid ASKAP Continuum Survey (RACS) is the first large-area survey to be conducted with the full 36-antenna Australian Square Kilometre Array Pathfinder (ASKAP) telescope. RACS will provide a shallow model of the ASKAP sky that will aid the calibration of future deep ASKAP surveys. RACS will cover the whole sky visible from the ASKAP site in Western Australia and will cover the full ASKAP band of 700–1800 MHz. The RACS images are generally deeper than the existing NRAO VLA Sky Survey and Sydney University Molonglo Sky Survey radio surveys and have better spatial resolution. All RACS survey products will be public, including radio images (with
$\sim$
15 arcsec resolution) and catalogues of about three million source components with spectral index and polarisation information. In this paper, we present a description of the RACS survey and the first data release of 903 images covering the sky south of declination
$+41^\circ$
made over a 288-MHz band centred at 887.5 MHz.
Optical tracking systems typically trade off between astrometric precision and field of view. In this work, we showcase a networked approach to optical tracking using very wide field-of-view imagers that have relatively low astrometric precision on the scheduled OSIRIS-REx slingshot manoeuvre around Earth on 22 Sep 2017. As part of a trajectory designed to get OSIRIS-REx to NEO 101955 Bennu, this flyby event was viewed from 13 remote sensors spread across Australia and New Zealand to promote triangulatable observations. Each observatory in this portable network was constructed to be as lightweight and portable as possible, with hardware based off the successful design of the Desert Fireball Network. Over a 4-h collection window, we gathered 15 439 images of the night sky in the predicted direction of the OSIRIS-REx spacecraft. Using a specially developed streak detection and orbit determination data pipeline, we detected 2 090 line-of-sight observations. Our fitted orbit was determined to be within about 10 km of orbital telemetry along the observed 109 262 km length of OSIRIS-REx trajectory, and thus demonstrating the impressive capability of a networked approach to Space Surveillance and Tracking.
This Chapter describes the geometry of twistor space of a 4-dimensional manifold. We motivated the twistor space as a geometrical construction that realisesthe action of the conformal group in 4D as the direct analog of that in 2D. This explains why the coordinates of a 4D space can be naturally put into a 2x2 matrix. We describe both the complexified version of the twistor space, as well as treat all the 3 possible signatures in detail. We then specialise to the case of Euclidean twistors, and describe how the twistor space can be interpreted as the total space of the bundle of almost complex structures of a 4D Riemannian manifold. Quaternionic Hopf fibration and its relation to the Euclidean twistor space is desccribed. We then describe the geometry of 3-forms in seven dimensions, and describe two different G2 structures on the 7-sphere. We end with a description of a lift of the usual twistor construction of integrable almost complex structures into seven dimensions. This is based on the notion of nearly parallel G2 structures.
This is the first central Chapter of the book that describes Riemannian geometry using Cartan's notion of soldering. Gravity first appears in this Chapter as a dynamical theory of a collection of differential forms rather than a metric. We describe thegeneral notion of geometric structures and then specialise to the case of a geometric structure corresponding to a metric. We describe the notion of a spin connection, its torsion, and then present examples of caclulations of Riemann curvature in the tetrad formalism. We then describe the Einstein-Cartan formulation of GR in terms of differential forms, and present its teleparallel version. We introduce the idea of the pure connection formulation, and compute the corresponding actino perturbatively. We then describe theso-called MacDowell-Mansouri formulation. We briefly describe the computations necessary to carry out the dimensional reduction from 5D to 4D. We then describe the so-called BF formulation of 4D GR, which in particular allows to determine the pure connection action in a closed form. We then describe the field redefinitions that are available when one works in BF formalism, and the associated formulation of BF-type plus potential for the B field.
are considered: chiral Einstein-Cartan, and chiral pure connection one. It is explained why chiral 4D perturbative formalisms are particularly powerful - they work with the minimal possible number of auxiliary fields to achieve polynomiality of the action. Spinors and differential operators that are motivated by spinors play a particularly important role in this Chapter, and so Lorentzian signature spinors are reviewed here in some detail. We also treat Yang-Mills theory and show how its chiral first order formalism gives the most powerful perturbative description. We end by describing how to gauge-fix the pure connection action on an arbitrary Einstein background. This produces a very simple perturbative description, remarkably more economic than the usual metric one.
We define gravity as a gauge theory with soldering. We discuss some analogies between gravity and YM theory that become visible via the chiral description of GR. We end with a provocative remark that assigns significance to the demonstrated by this book fact that there are so many non-obviously equivalent reformulations of General Relativity.
We review, in concise manner, the standard Einstein-Hilbert metric formulation of GR, together with related to it desccriptions such as the first order Palatini formalism, as well as the Einstein-Schroedinger pure affine formulation. We also describe the linerisation of the Einstein-Hilbert action around an arbitrary Einstein background, with associated geometric notions such as the Lichnerowicz operator. Some less standard aspects are also reviewed, for example we show how to explicitly rewrite the Einstein-Hilbert action in terms of the metric.
This short Chapter describes a particular modification of 4D General Relativity that is "geometrically natural" in the sense explained. A Bianchi I setup solution of the modified theory is worked out, in particular to illustrate that the modified theory appears to be simpler than GR in the types of functions that get produced.
This Chapter describes the chiral pure connection formulation of 4D GR, which is singled out from all other reformulations because of the economy of the description that arises. We first obtain the chiral pure connection Lagrangian, and explain how the metric arises from a connection. We also discuss the reality conditions. We then introduce notions of definite and semi-definite connections, and discuss the question of whether the pure connection action can be defined non-perturbatively. The question is that of selecting an appropriate branch of the square root of a matrix that appears in the action. Many examples are looked at to get a better feeling for how this connection formalism works. Thus, we describe the Page metric, Bianchi I as well as Bianchi IX setups, and the spherically symmetric problem. All these are treated by the chiral pure connection formalism, to illustrate its power. We also give here the connection description of the gravitational instantons, and in particular describe the Fubini-Study metric. We also show how to use the connection formalism to describe some Ricci-flat metrics, and illustrate this on the examples of Schwarzschild and Eguchi-Hanson metrics. We finish with the description of the chiral pure connection perturbative description of GR.
This is a short Chapter introducing an index-free notation for 2+1 gravity, which encodes all objects into 2x2 matrix-valued one-forms. We then describe the Chern-Simons formulation of 2+1 gravity, as well as the pure spin connection formulation.
Historical introduction into the topic of formulations of General Relativity with their associated mathematical formalisms. We review the history of the idea that gravity is geometry, as well as the history of development of main geometical ideas of modern differential geometry. We start with metric geometry of Riemann, Levi and Civita, and describe the main contributions of Cartan. We touch upon the fact that spinors and differential forms are closely related, first observed by Chevalley. We give arguments for why formalisms based on differential forms may be superrior to the metric one.
This is the longest Chapter of the book introducing the "chiral" formulations of 4D GR. The most important concept here is that of self-duality. We describe the associated decomposition of the Riemann tensor, and then the chiral version of Einstein-Cartan theory, together with its Yang-Mills analog. The geometry that is necessary to understand the fact that the knowledge of the Hodge star is equivalent to the knowledge of the conformal metric is explained in some detail. We also describe the different signature pseudo-orthogonal groups in 4 dimensions, and in particular explain that it is natural to put coordinates of a 4D space into a 2x2 matrix, the fact that is going to play central role in the later description of twistors. The notions of the chiral part of the spin connection, as well as the chiral soldering form are introduced. We give an example of a computation of Riemann curvature using the chiral formalism, to illustrate its power. We then describe the Plebanski formulation, as well as its linearisation. This allows to derive the linearisation of the chiral pure connection action, to be studied in full in the following Chapter. We describe coupling to matter in Plebanski formalism, and then some alternative descriptions related to Plebanski formalism.