The Gravitational Wave Universe
For centuries, mankind has observed the sky with the naked eye, and in recent times with bigger and bigger telescopes. Today we study the universe mainly by observing visible light and other forms of electromagnetic radiation, such as radio waves, X rays, and gamma rays. However, recently we have learnt to also exploit other cosmic “messengers”, such as high-energy particles including cosmic rays and neutrinos. With Advanced Virgo, we are attempting to detect a new type of astrophysical messenger, detected for the first time in September 2015: gravitational waves.
Gravitational waves are ripples in the fabric of spacetime, and are expected to be emitted by spinning stars in binary systems, black holes, massive stellar explosions, and even shortly after the birth of the Universe, the Big Bang. Most likely there are also as yet unknown astrophysical sources, which must enlarge this list: General Relativity states that any accelerated motion of mass that does not have spherical nor cylindrical symmetry could be a source of gravitational waves.
Advanced Virgo can detect gravitational waves with frequencies between 10 Hz and 10000 Hz. These are the same frequencies as the sound waves that are audible by humans. Therefore, any signal measured by Advanced Virgo can be sent to a loudspeaker, and we can hear the symphony of the Universe.
What are the main sources of gravitational waves in the sky? Below you can find out, and even listen to their “gravitational sound”!
Coalescences of black holes and neutron stars
When two compact and massive objects such as black holes and neutron stars spin one around the other, they slowly get closer and closer until they finally merge, forming a black hole. This phenomenon is known as coalescence. Such binary systems lose energy by the emission of gravitational waves with increasing frequency and increasing amplitude throughout their long lifetimes. The first experimental evidence for the emission of gravitational waves came from the study of the binary neutron star PSR 1913+16. Russel Hulse and Joseph Taylor were awarded the Nobel Prize for Physics in 1993 for observing that this binary star loses energy exactly as expected by the emission of gravitational waves. Several other binary stars discovered successively behave in the same way.
During the final stage of the merging phase, the gravitational waves are strong enough to be detected by Advanced Virgo just a few seconds before their collision, when they spin 10, 100, 1000 times per second around each other! Such collisions are very rare in a single galaxy, but Advanced Virgo will be searching for them in millions of galaxies. This should enable us to find a handful of them every year. Detecting binary systems will help us to understand how compact astrophysics objects interact, and if such violent collisions are related to the gamma-ray bursts detected by satellites since decades. The first ever detected gravitational wave (called GW150914) came from a binary black hole merger, and it already teached us that black holes as massive as 30 and 60 solar masses do exist!
Rotating neutron stars
A neutron star is a rapidly rotating, highly magnetised star, which represents the remnant core of a massive star has undergone a supernova explosion. Neutron stars are extreme objects: they have roughly the same mass as our Sun, but concentrated into a sphere of 10-km of radius, and they can spin up to 1000 times per second! If the star is not perfectly spherical, with only a tiny “mountain” on its surface, it will generate continuous gravitational waves.
Pulsars are special cases of magnetically asymmetric neutron stars, from which we receive periodic light flashes each time the star makes one turn on itself. Until now, Virgo has not detect any signals from known pulsars, which has allowed us to conclude that their deviation from being perfect balls is less than 1 mm! Observation of neutron stars will provide important information about their internal structure. Advanced Virgo will search for gravitational waves emitted by neutron stars in the neighbourhood of the Sun, and also in our own galaxy, the Milky Way.
Bursts and supernovae
“Gravitation wave bursts” is a generic name given to short gravitational wave signals that last from a few milliseconds to a few seconds.
Advanced Virgo will be able to observe the heart of a gravitational collapse of a massive star at the end of its life, known as a supernova. In a galaxy like the Milky Way there are only a few such supernovae per century. Their observation will allow us to better understand what is hidden behind the matter ejected during the explosion and how black holes are created.
Most cosmological models predict that we are bathed in a random background of gravitational waves generated in the first instants after the Big Bang. Detection of such a background would give us insight into the evolution of the Universe, providing a unique probe of the very early Universe.
In addition, an astrophysical background of gravitational waves must result from the superposition of all the faint and distant sources that have emitted gravitational waves since the beginning of the Universe. Detection of this background would help elucidate the star formation history and the evolution of astrophysical sources.
Facing the Unexpected
Every time humans have observed the sky with a new instrument, utilised new light wavelengths or messengers, unexpected objects and phenomena have been discovered. Hence, looking for gravitational waves, we are also expecting surprises! Cosmic strings are just one of the exotic sources that may emit gravitational waves.
Play with the Gravitational Universe!
Playing and listening to gravitational waves: Black Hole Hunter game