Abstract
The LIGO collaboration recently reported the first gravitational-wave constraints on the tidal deformability of neutron stars. I discuss an inherent ambiguity in the notion of relativistic tidal deformability that, while too small to affect the present measurement, may become important in the future. I propose a new way to understand the ambiguity and discuss future prospects for reliably linking observed gravitational waveforms to compact object microphysics.
| Original language | English (US) |
|---|---|
| Article number | 085002 |
| Journal | Classical and Quantum Gravity |
| Volume | 35 |
| Issue number | 8 |
| DOIs | |
| State | Published - Mar 12 2018 |
Keywords
- black holes
- gravitational waves
- neutron stars
- tidal deformability
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)