"Gamma Cas consists of a Be-type star surrounded by a disk of material; some of this material flows toward the companion; a second disk forms around the companion, and the material eventually flows toward the poles, where it emits X-rays (green arrows). Some of these X-rays are reflected by the surface of the white dwarf (purple arrows). Credit: University of Liège / Y.Nazé" (ScitechDaily, A Bright Star Hid a Massive Secret for 50 Years: Mystery of Gamma Cassiopeiae Finally Solved)
Gamma Cassiopeiae is a bright B-spectral class star. Astronomers found a hidden companion. The small white dwarf near that star. This means the Gamma Cassiopeiae is a binary star. And the thing that makes it interesting is the small white dwarf that orbits the center star and pulls matter from that star.
The massive star in the Gamma Cassiopeiae system is the source of the X-ray bursts from that star. The magnetic white dwarf is the thing. That accelerates the ionized gas around it. And when that ion belt impacts the plasma around the larger star, it causes a very high-energy reaction. And we see that reaction as X-ray bursts from around that star.
When particles in two separate plasma disks collide, they form X-ray bursts. This observation is the answer to the astronomical mystery. But. It can also make it possible to detect methods. To create artificial gamma- or X-rays. In history researchers thought that only black holes could create X- and gamma-rays. But today. We know that. Also, less massive objects. Like white dwarfs can form at least X-rays.
Those high-energy rays can form when a white dwarf pulls matter from its companion star. The matter that the white dwarf pulls from the companion star forms the ion cloud or halo around the white dwarf. And when that material flows. Impacts the plasma that orbits the white dwarf. That reaction forms X-ray bursts. The high-energy magnetic field. Puts the plasma into a whirl very fast around the white dwarf.
Magnetic white dwarfs interact through gravity. But it also interacts through a magnetic field. When the material impacts the white dwarf’s surface. That impact causes a nuclear reaction, which raises the energy level in plasma. That orbits the white dwarf.
When incoming material impacts. The white dwarf’s plasma fields. That causes. A high-energy interaction. This interaction causes a situation. Those impacting particles send high-energy radiation. The remarkable thing is this: in this reaction, the magnetic interaction is dominating.
And that thing causes a model, that if we create two crossing plasma wheels or plasma rings, we could create synthetic X- or even gamma rays. If we want to create synthetic gamma-rays, we must raise those particles' energy level so high that the quarks can interact with each other. Another way to create those high-energy radiation bursts is to use particle accelerators that accelerate quarks, electrons, or protons with high-power magnetic fields and aim laser beams into them.
Those photons can accelerate those particles or particle clusters to a high energy level. And that system. It can create high-energy radiation. The system can have two cyclotrons that create a plasma ring. That accelerates those particles with the highest possible energy level. Then that plasma will be conducted to the linear accelerators.
There. High-energy photons will accelerate those particles. That conducted. To crossing trajectories. Another way. Is to aim lasers at. The point where those plasma rings that rotate in opposite directions impact. When plasma rings orbit in opposite directions, that maximizes their impact force. These types of systems can be used to create synthetic gamma- or X-rays. Antimatter annihilation is the tool. That could create the gamma-rays. But. Creating gamma rays by using antimatter. It is quite an expensive method.
https://scitechdaily.com/a-bright-star-hid-a-massive-secret-for-50-years-mystery-of-gamma-cassiopeiae-finally-solved/
No comments:
Post a Comment
Note: Only a member of this blog may post a comment.