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Fundamental physics with the Square Kilometre Array

Research output: Contribution to journalLiterature review

  • A. Weltman
  • P. Bull
  • S. Camera
  • K. Kelley
  • H. Padmanabhan
  • J. Pritchard
  • A. Raccanelli
  • S. Riemer-Sørensen
  • L. Shao
  • S. Andrianomena
  • E. Athanassoula
  • R. Barkana
  • G. Bertone
  • C. Bœhm
  • C. Bonvin
  • A. Bosma
  • M. Brüggen
  • C. Burigana
  • F. Calore
  • J. A. R. Cembranos
  • C. Clarkson
  • R. M. T. Connors
  • De La Cruz-Dombriz
  • P. K. S. Dunsby
  • J. Fonseca
  • N. Fornengo
  • D. Gaggero
  • I. Harrison
  • J. Larena
  • Y. Z. Ma
  • M. Méndez-Isla
  • S. D. Mohanty
  • S. Murray
  • D. Parkinson
  • P. J. Quinn
  • M. Regis
  • P. Saha
  • M. Sahlén
  • M. Sakellariadou
  • J. Silk
  • T. Trombetti
  • F. Vazza
  • T. Venumadhav
  • F. Vidotto
  • F. Villaescusa-Navarro
  • Y. Wang
  • C. Weniger
  • L. Wolz
  • F. Zhang
  • B. M. Gaensler

The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey speed than any current radio telescope. The SKA will address many important topics in astronomy, ranging from planet formation to distant galaxies. However, in this work, we consider the perspective of the SKA as a facility for studying physics. We review four areas in which the SKA is expected to make major contributions to our understanding of fundamental physics: cosmic dawn and reionisation; gravity and gravitational radiation; cosmology and dark energy; and dark matter and astroparticle physics. These discussions demonstrate that the SKA will be a spectacular physics machine, which will provide many new breakthroughs and novel insights on matter, energy, and spacetime.

Original languageEnglish
Article numbere002
Number of pages52
JournalPublications of the Astronomical Society of Australia
Volume37
DOIs
Publication statusPublished - 27 Jan 2020

Documents

  • 1810.02680

    Rights statement: This article has been published in a revised form in the Publications of the Astronomical Society of Australia http://doi.org/10.1017/pasa.2019.42. This version is free to view and download for private research and study only. Not for re-distribution or re-use. © Astronomical Society of Australia 2020.

    Accepted author manuscript (Post-print), 8.87 MB, PDF document

    Due to publisher’s copyright restrictions, this document is not freely available to download from this website until: 27/07/20

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