16.10.2017 —

For the first time ever, scientists have measured the electromagnetic and gravitational signals generated by the collision of two neutron stars. Physicists of the Excellence Cluster Universe recorded the aftermath of the powerful event. Their findings will facilitate verification of theories on the exact progression of the merger – as well as the theoretical models on sizes, masses and matter properties of neutron stars.

The collision of the two neutron stars occurred in the galaxy NGC4993, about 130 million light years away from Earth. The gravitational waves of this massive event were observed by the U.S. Laser Interferometer Gravitational Wave Observatory (LIGO) and its European sister observatory Virgo, on August 17, 2017 (GW170817).

Neutron stars: matter existing under the most extreme conditions
These new observations bring us a step closer to answering a very fundamental question in physics: What is the state of matter in a neutron star? Of all the star types known to science, neutron stars are the smallest and most dense stars. They’re the final stage in the collapse of a massive star and typically have a radius of 10 to 20 kilometers, with about twice the mass of our own sun. According to models, they consist almost entirely of neutrons – because of the enormous density, the electrons of the atomic shells were squeezed into the atomic nuclei converting the protons into neutrons.

Strong nuclear forces preventing a further collapse
A further collapse of the matter in neutron stars is prevented by strong nuclear forces between their neutrons. “Until now, we knew close to nothing about the precise composition and the particle interactions of matter under such extreme conditions,” says Prof. Laura Fabbietti, Professor for Dense and Strange Hadronic Matter at Technical University of Munich (TUM) and leading scientist of the Excellence Cluster Universe. Fabbietti has been doing research in this field for years. “Now we can test and prove our theories for the first time.”

A short gamma ray burst
The gravitational wave event was accompanied by a short gamma ray burst (GRB170817A), which lasted less than two seconds and was measured by the two detectors – the Fermi-GBM and the spectrometer mounted on the INTEGRAL space telescope – both built at the Max Planck Institute for Extraterrestrial Physics (MPE). “For more than 30 years, the merger of two neutron stars has been suspected to be the cause of such a characteristic short gamma ray burst", says Dr. Jochen Greiner from the MPE, one of the leading scientist of the Excellence Cluster Univers. "Now, for the first time, we have a clear confirmation for the model.”

The afterglow of a kilonova
The physicists also expected to observe an afterglow in the optical/near infrared light part of the spectrum lasting for days, which is known as a kilonova. Matter – especially neutrons and, in small numbers, protons and helium nuclei – is ejected in all directions following the merger. Within a few seconds, the helium nuclei are converted into heavy elements with high atomic numbers by fusion, further neutron capture and subsequent radioactive decay and nuclear fission.

Radioactive nuclei decay
The newly formed radioactive nuclei subsequently decay into stable elements and emit gamma radiation for up to 10 days, which in turn heats the ejected material and results in a broadband electromagnetic emission. This kilonova was also detected by several teams of astronomers working independently of one another over the course of 12 hours in the approximately 100 square-degree error box of the gravitational wave event. Among other things with the help of the Dark Energy Camera of the Dark Energy Survey (DES), a collaboration of international scientists to study the sky in the optical and near-infrared spectral range. Leading scientists from the Excellence Cluster Universe, Prof. Jochen Weller and Prof. Joseph Mohr from the Ludwig-Maximilians-Universität, also belong to this research group.

Confirmation of the theories of the formation of the heaviest elements
“These observations confirm the theoretical models about the merger of neutron stars and their energetic processes, such as the ejection of a considerable amount of radioactive material,” notes Greiner. “Above all, they provide new insights into the astrophysical source of the formation of the heaviest of all elements,” adds Prof. Hans-Thomas Janka from the Max Planck Institute for Astrophysics, leading scientist with the Excellence Cluster Universe, and renowned expert for the modelling of neutron star mergers, supernovae and gamma ray bursts.

No significant neutrino signals detected
Neutrinos could be another kind of “cosmic witness” providing evidence of such high-energy cosmic events like neutron star collisions. However, researchers with the IceCube Collaboration, which operate the world’s largest neutrino telescope at the South Pole, did not detect any significant signals. The explanation is simple: “The event occurred too far away,” explains Elisa Resconi, Prof. for Experimental Physics with Cosmic Particles at TUM. “Neutrinos are very elusive particles. At such a distance it is almost impossible to trace the neutrino messengers with our detector. But we’re hoping that IceCube will have the chance to catch neutrino signals from events in the future.”

It’s just the beginning of what astronomy can learn from gravitational waves
Since last year, several gravitational wave signals of merging black holes have been measured – work which was honored with the Nobel Prize for Physics in 2017. The most recent findings on the neutron star event mark another decisive breakthrough in multi-messenger astronomy. “By using gravitational waves, a multitude of new measurements which are complementary to classical astronomy are now possible, and thus the answers to previously unanswered questions are within reach,” Resconi says.

Original Publications:
Antares, IceCube, Pierre Auger, LIGO Scientific and Virgo Collaborations: Search for High-Energy Neutrinos from Binary Neutron Star Merger GW170817 with Antares, IceCube and the Pierre Auger Observatory, submitted to The Astrophysical Journal

S.J. Smartt et al.: A kilonova as the electromagnetic counterpart to a gravitational wave source, Nature, to be published on 16 October 2017, 10:00 US Eastern Time/16:00 CEST, DOI: 10.1038/nature24303

Contacts:
Prof. Dr. Laura Fabbietti
Technical University of Munich
Physics Department
James-Franck-Straße
85748 Garching, Germany
T: +49 89 289 12433
E: laura.fabbietti@ph.tum.de

PD Dr. Jochen Greiner
Max Planck Institute for Extraterrestrial Physics
Gießenbachstraße 1
85748 Garching, Germany
T: + 49 89 30000-3847
E-Mail: jcg@mpe.mpg.de

Prof. Hans-Thomas Janka
Max Planck Institute for Astrophysics
Karl-Schwarzschild-Straße 1
85748 Garching, Germany
T: +49 89 30000-2228
E: thj@mpa-garching.mpg.de

Prof. Elisa Resconi
Technical University of Munich
Physics Department
James-Franck-Straße
85748 Garching, Germany
T: +49 89 289 12422
E: elisa.resconi@tum.de

Press Contact:
Stefan Waldenmaier
Excellence Cluster Universe
Boltzmannstraße 2
85748 Garching, Germany
T: +49 89 289 35831-7119
E: stefan.waldenmaier@universe-cluster.de