Hello and welcome back to another episode of Physics Partner. Today I joined you with a very unique and extremely interesting topic known as Bremstrelung Radiation. The term Bremstrelung is derived from the German word Bremsen to break an Australian radiation. Also called breaking radiation or declaration radiation. Bremstrelung radiation is a type of electromagnetic radiation emitted when a charged particle upon getting deflected by another charged particle is decelerated. These charged particles are mainly electrons or atomic nuclei. The particles in motion upon clashing loose kinetic energy, the lost energy is emitted as radiation is the form of photons. Thus the law of conservation of energies also is satisfied. This is known as Bremstrelung Radiation. The Bremstrelung radiation has a continuous spectrum. The peak intensity tends to shift towards higher frequency with the increase in the energy of decelerated charged particles. Let's recreate a historical movement by similar virtual lab to elaborate more about Brems. In 1895, Wilhelm Wrongton discovered that the beam of cathode rays could create a new type of radiation, X-rays. When allowed to impinge up on an obstacle such as a glass of the tube itself, the present demonstration recreates that discovery. A melty's cross CRT is the source of cathode rays as well as target. A modern Geiger Mooler counter detects the X-rays. The Bremstrelung X-rays are emitted when electrons get decelerated when fired against a metal target. These charged particles emit Bremstrelung radiation in the form of photons or Bremstrelung's X-rays. The continuous spectrum forms due to bombardment of electron lies in the x-ray region of the electromagnetic spectrum. Let's talk about the difference between Bremstrelung and characteristic radiation. The two unique mechanisms of which X-rays are produced are called Bremstrelung and characteristics processes. Brems X-rays produce a continuous X-rays spectrum whereas characteristics X-rays are produced as specific narrow bands of energies. In terms of astronomy, one of the most interesting examples of Bremstrelung radiation in the universe is that coming from the hot, an intra-clustered gas of Klexy clusters. The gas has X-rays luminousities of 210 to 38 watts, roughly 10 billions to 1 billion times the luminosity of the Sun and temperatures on the order of 10 million Kelvin. X-rays telescopes can detect this radiation as diffuse light as seen in the image of the comacluster. Bremstrelung is one of the process by which cosmic rays dissipate some of their energy in the Earth's atmosphere. So thank you very much for watching and listening. I hope you enjoyed the video. I hope this video is very useful for you. See you in the next video. Take care of yourself. Goodbye.