Indian scientists have called for careful observations to detect gravitational waves as many fast spinning dense neutron stars generate gravitational waves continuously.
Neutron stars are the densest observable objects in the universe, with a fistful of stellar material outweighing a mountain on Earth.
While such stars are not bigger than a city, in size, they have more material than in the Sun crammed inside them.
Sudip Bhattacharyya from the Tata Institute of Fundamental Research (TIFR) in Mumbai and Deepto Chakrabarty from Massachusetts Institute of Technology (MIT) in the US have shown that a population of neutron stars should spin around their axes much faster than the highest observed spin rate of any neutron star.
They pointed out that the observed lower spin rates are possible if these neutron stars emit gravitational waves continuously, and hence spin down.
A population of neutron stars can increase their spin rate by the transfer of matter from a normal companion star.
Infact, some of them have been observed to spin several hundred times in a second around their own axes.
In the 1970s, it was theoretically worked out how fast these neutron stars could spin, and since then this has formed the basis of studies of these stars.
However, the new study has shown that for episodic mass transfer, which happens for many neutron stars, the stellar spin rate should be much higher, and the star could easily attain a spin rate more than a thousand times per second.
Since no neutron star has been observed with such a high spin rate, the team has pointed out that many of these stars are likely to be slowed down by continuously emitting gravitational waves.
Gravitational waves emitted by massive objects is a prediction of Einstein's general theory of relativity, which has recently been discovered during transient phenomena of black hole mergers.
However, the detection of continuous gravitational waves, which could provide an opportunity to study these waves almost permanently, is still elusive.
The research provides a strong indication that many fast spinning neutron stars generate gravitational waves continuously, and careful observations should be made to detect such waves.
The study appears in The Astrophysical Journal.
(With inputs from PTI)
