Pith. sign in

However, at the moment the timing of SGR J1745-2900 has not yet reached sufficient levels of precision for this purpose, mainly due to the intrinsic variability of the source

the effect of ‘matter’ on the propagation time was investigated using a similar approach, showing that the presence of dark energy around Sgr A* would cause an additional delay of≃

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
browse 1 citing papers

citation-role summary

background 1

citation-polarity summary

support 1

fields

gr-qc 1

years

2024 1

verdicts

CONDITIONAL 1

roles

background 1

polarities

support 1

representative citing papers

Towards an exact approach to pulsar timing

gr-qc · 2024-12-13 · conditional · novelty 6.0

For pulsars orbiting stellar or intermediate-mass black holes, standard post-Newtonian timing formulas can differ from a full general-relativistic computation by 10^-7 to 10^-4 seconds, enough to affect future SKA timing.

citing papers explorer

Showing 1 of 1 citing paper.

  • Towards an exact approach to pulsar timing gr-qc · 2024-12-13 · conditional · none · ref 6

    For pulsars orbiting stellar or intermediate-mass black holes, standard post-Newtonian timing formulas can differ from a full general-relativistic computation by 10^-7 to 10^-4 seconds, enough to affect future SKA timing.