gw170817

There are 0 repository under gw170817 topic.

• 2-ogc

  gwastro / 2-ogc

  Second Open Gravitational-wave Catalog of Compact Binary Mergers. Parameter estimates for O1 and O2 mergers. Sub-threshold BNS/NSBH/BBH candidates.

  gravitational-wavesneutron-starblack-holeligodata-releasegw150914gw151012gw151226gw151205gw170104gw170121gw170304gw170727gw170729gw170809gw170814gw170817gw170818gw170823gw170608
  Language:Shell 11

• sugwg / gw170817-inclination-angle

  Measuring the viewing angle of GW170817 with electromagnetic and gravitational waves

  gw170817gravitational-wavesligovirgoparameter-estimationastronomybayesian-inferencepycbc
  Language:Jupyter Notebook 7

• sugwg / gw170817-common-eos

  Results from the common equation of state constraint analysis of GW170817

  gw170817gravitational-wavesligovirgoparameter-estimationastronomybayesian-inferencepycbc
  Language:Jupyter Notebook 4

• gwastro / bns-eccentric-pe

  Parameter estimates for the eccentricity of GW170817 and GW190425

  gw190425gw170817eccentricitygravitational-wavesdata-releasepycbcbayesian-inference
  3

• ffronimo / Reheating

  We provide a consistent description of the reheating era of a constrained Gauss-Bonnet model by using the same free parameters that result in a viable inflationary era. The theory predicts a propagation velocity of tensor perturbations which is equal to unity in order to be in agreement with the GW170817 event. The reheating era turns out to be viable if one considers that the effective EoS is equal to unity thus a primordial stiff matter era prior to the reheating era is predicted. In the end, a comparison between gravitational baryogenesis during the stiff matter era induced by CP violating terms containing either the Ricci scalar of the Gauss-Bonnet invariant is available.

  gauss-bonnetinflationreheatingbaryogenesisgw170817
  Language:Mathematica 1