Ultra-compact binaries section

NGO Yellow book

  • Verification binaries
  • Thousands of detections
  • Detect all (tens) NS, BH binaries
  • Binary evolution (Common envelope)
  • Onset mass transfer in WD+WD binaries (stability, mergers, SNIa)
  • Period evolution, physics of tides and mass transfer (not sure this is a strong case)
  • Detections (distances, inclinations) throughout Galaxy –> Galactic structure

What will have been done by 2028?

  • Gaia discovered few hundred(?) short period binaries (but V < ~20, i.e. only ~25 resolved eELISA sources, cf Littenberg et al. 2013)
  • Variability surveys (OmegaWhite etc, LSST?) will have found many(?) binaries (g < 22?)
  • Pdot measurement of at least J0651 and likely a few others will be exquisite
  • Gaia has mapped structure of Galaxy
  • EM follow-up facilities available? Deep, wide field images (BlackGEM?)
  • SKA likely not found the short period NS+NS (expected only 1/1e4 MSPs or so and signals very smeared out due to short orbital periods)
  • Do we understand binary evolution, common-envelope by 2028?

White paper

  • Verification binaries (quite a few by 2028 expected)
  • Thousands of resolved binaries (most still undiscovered by 2028) because too faint
  • Detect all (tens) NS, BH binaries, likely not found by SKA
  • Binary evolution, CE?
  • Onset mass transfer in WD+WD binaries (stability, mergers, SNIa)
 
white_paper.txt · Last modified: 2013/04/13 19:56 by 127.0.0.1
 
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