This is an article from NASA about a study on the electromagnetic forces acting on merging neutron stars. Here's a summary of the article:
**Title:** "Simulation Highlights Regions Producing Highest-Energy Light from Merging Neutron Stars"
**Summary:**
A team of researchers from NASA's Goddard Space Flight Center used supercomputer simulations to study the electromagnetic forces acting on merging neutron stars. The study found regions producing gamma rays with energies trillions of times greater than that of visible light, but likely none of it could escape. However, gamma rays at lower energies, with millions of times the energy of visible light, can exit the merging system, and the resulting particles may also radiate at still lower energies, including X-rays.
**Key Findings:**
* The simulations showed regions producing gamma rays with energies trillions of times greater than that of visible light, but likely none of it could escape.
* However, gamma rays at lower energies, with millions of times the energy of visible light, can exit the merging system, and the resulting particles may also radiate at still lower energies, including X-rays.
* The emission varies rapidly and is highly directional, but it could potentially be detected by future facilities.
**Implications:**
* Future medium-energy gamma-ray space telescopes, especially those with wide fields of view, may detect signals originating in the runup to the merger if gravitational-wave observatories can provide timely alerts and sky localization.
* ESA (European Space Agency) and NASA are collaborating on a space-based gravitational-wave observatory named LISA (Laser Interferometer Space Antenna), planned for launch in the 2030s.
**Research Team:**
* D. Skiathas et al., NASA's Goddard Space Flight Center, Greenbelt, Md.
* Alice Harding at the Los Alamos National Laboratory in New Mexico
* Paul Kolbeck at the University of Washington in Seattle
**Title:** "Simulation Highlights Regions Producing Highest-Energy Light from Merging Neutron Stars"
**Summary:**
A team of researchers from NASA's Goddard Space Flight Center used supercomputer simulations to study the electromagnetic forces acting on merging neutron stars. The study found regions producing gamma rays with energies trillions of times greater than that of visible light, but likely none of it could escape. However, gamma rays at lower energies, with millions of times the energy of visible light, can exit the merging system, and the resulting particles may also radiate at still lower energies, including X-rays.
**Key Findings:**
* The simulations showed regions producing gamma rays with energies trillions of times greater than that of visible light, but likely none of it could escape.
* However, gamma rays at lower energies, with millions of times the energy of visible light, can exit the merging system, and the resulting particles may also radiate at still lower energies, including X-rays.
* The emission varies rapidly and is highly directional, but it could potentially be detected by future facilities.
**Implications:**
* Future medium-energy gamma-ray space telescopes, especially those with wide fields of view, may detect signals originating in the runup to the merger if gravitational-wave observatories can provide timely alerts and sky localization.
* ESA (European Space Agency) and NASA are collaborating on a space-based gravitational-wave observatory named LISA (Laser Interferometer Space Antenna), planned for launch in the 2030s.
**Research Team:**
* D. Skiathas et al., NASA's Goddard Space Flight Center, Greenbelt, Md.
* Alice Harding at the Los Alamos National Laboratory in New Mexico
* Paul Kolbeck at the University of Washington in Seattle