Researchers enable detection of remarkable gravitational-wave signal

Credit: I. Markin (Potsdam University), T. Dietrich (Potsdam University and Max Planck Institute for Gravitational Physics), H. Pfeiffer, A. Buonanno (Max Planck Institute for Gravitational Physics).

The coalescence and merger of a lower mass-gap black hole (dark grey surface) with a neutron star with colours ranging from dark blue (60 grams per cubic centimetre) to white (600 kilograms per cubic centimetre) and highlight the strong deformations of the low-density material of the neutron star.

« Researchers enable detection of remarkable gravitational-wave signal

Credit: I. Markin (Potsdam University), T. Dietrich (Potsdam University and Max Planck Institute for Gravitational Physics), H. Pfeiffer, A. Buonanno (Max Planck Institute for Gravitational Physics).

This image shows the merger of a lower mass-gap black hole (dark grey surface) with a neutron star with colours ranging from dark orange (1 million tons per cubic centimetre) to white (600 million tons per cubic centimetre). The gravitational wave signal is 2 represented with a set of strain amplitude values of plus-polarisation using colours from dark blue to cyan.

« Researchers enable detection of remarkable gravitational-wave signal

0.05676

麻豆传媒

Expert Pitch

Expert Query

Expert Directory