Periodic Reporting for period 1 - BHianca (Black Hole Interactions and Neutron star Collisions Across the universe)
Reporting period: 2022-01-01 to 2023-06-30
The blossoming field of multi-messenger astrophysics opens a new window onto the invisible Universe, in which different cosmic messengers - such as gravitational waves, neutrinos and light - provide complementary views of the same source. We can learn more from the Universe by combining these multiple messengers, just as we combine colors, sounds and flavors to know about the world. Gravitational waves and neutrinos probe the innermost regions - impenetrable to light - of extreme astrophysical events, and carry unique information about the behavior of masses and the production of energy. These novel astrophysical observations allow us to move beyond the realm usually probed by light, transforming our way to think about the Universe.
This ERC project aims at understanding the violent encounters of the densest objects in the Universe, such as neutron stars (NSs) and black holes (BHs). These extreme stellar collisions create gravitational waves and light that we will combine to address some of the most fundamental questions of modern astrophysics: from the exotic states of matter at supra-nuclear densities to the expansion rate of the Universe and the origin of the heaviest metals, such as gold and platinum. Breakthrough results will be achieved by making first detections of light from NS-NS and NS-BH encounters in our cosmic backyard.
The project was inaugurated by the discovery of GRB211211A, a minute-long explosion followed by a glow of red light known as kilonova. The kilonova is the telltale signature for the production of radioactive heavy nuclei via rapid neutron capture processes (WP2). However, a kilonova is a rare event that only happens with a neutron star encounters another compact object such as another neutron star or a black hole. The association of a kilonova with a long GRB shows that not all long GRBs are the product of the explosive death of a massive star, challenging our long-established beliefs about how long GRBs and their progenitors.
The PI had a central role in the discovery and characterization of the kilonova, the results of her research were published on December 7 in the journal Nature.
A few months later we were surprised by the brightest gamma-ray burst (GRB) ever observed, GRB221009A, which pushed our models to the extreme. This titanic explosion surpassed in brightness any previous gamma-ray burst and was so bright it effectively blinded most gamma-ray instruments in space. All this energy was shot into space in the form of a jet by a black hole, born in the GRB explosion. In just about every previously observed gamma-ray burst, the jet remained remarkably compact and there was little to no stray light or material outside the narrow beam. By contrast, in GRB 221009A the jet had a narrow core with wider, sloping sides. These properties, also shared by a small group of insanely bright bursts, allow us a better understanding of how black holes release their power through ultra-fast jets (WP1).
The PI and her team had a central role in this study, which was published on June 7 in the journal Science Advances.
Finally, we have been using the peculiar explosion dubbed GRB230307A to study what happens before two compact objects collide, what sort of electromagnetic radiation may become visible and how its brightness and duration may help us probe the interior of neutron stars (WP3). This study is currently in preparation and about to be submitted to ApJ Letters.
In the next two years, breakthrough discoveries are to be expected. The reactivation of the LIGO detectors marked the beginning of the O4 observing run, when gravitational wave detectors will chase NS-NS and NS-BH in the nearby Universe with a predicted tenfold improvement in discovery rates. We will observe new GW sources with the goal of finding their electromagnetic counterparts, thus discovering the next multi-messenger source.
By combining gravitational waves and electromagnetic radiation, we can learn more information about our cosmic history than any one of these messengers can provide in isolation. These multi-messenger events will reveal the Universe as never before.