4.4 Article

r-mode astronomy

Journal

EUROPEAN PHYSICAL JOURNAL A
Volume 52, Issue 2, Pages -

Publisher

SPRINGER
DOI: 10.1140/epja/i2016-16038-9

Keywords

-

Ask authors/readers for more resources

Next-generation gravitational wave detectors will start taking data in the near future. Here we discuss the chances to detect the continuous emission from r-mode oscillations in compact stars and study which properties of compact stars we can infer from such novel data. In particular we show that the combination of the gravitational wave data with electromagnetic multi-messenger observations could give us detailed insight into compact star properties, ranging from precise mass-radius measurements to the determination of the equation of state and the phase structure of dense matter.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.4
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available