论文代写:黑洞

18 4月 论文代写:黑洞

论文代写:黑洞

天体物理学家一直认为只有小规模的巨大黑洞。他们没有考虑中等大小的黑洞。然而,最近的研究已经发现中型黑洞的存在(IMBH)2014本的形成是由于几星碰撞形成一个链反应中间的黑洞。这可能最终成为超大质量黑洞(里德,2015)。

黑洞不会发出任何射线,任何被发送探测黑洞的光子都会被黑洞吸收,很难探测到黑洞的黑洞。为了探测黑洞,一些辅助性的间接方法被使用。检测黑体的“引力效应对发光物质”(赖登,2003)是一个最初的尝试做了探测黑洞。一些黑洞的检测新方法是利用X射线检测旋转星星或重力透镜(米勒,1996)。

黑洞的强烈引力会使附近的粒子加热,而且会放出大量的热量和X射线。天文学家用X光来隔离地区的黑洞。有时星星绕着一个区域旋转。天文学家们将从星星的黑洞的旋转位置检测(米勒,1996)。另一种检测黑洞的技术是利用引力透镜。

论文代写:黑洞

The astrophysicists had always assumed that there are only small sizes of massive size black hole. They had not considered the medium sized black holes. However, recent research has discovered the existence of medium-sized black holes (IMBH) in 2014 the formation of this is due to the fact that several stars collide and form an intermediate black hole in a chain reaction. This could eventually become supermassive black holes (Redd, 2015).

A black hole will not emit any rays and any photons that are sent to detect the black holes will be absorbed by the black hole making it difficult to detect black hole. In order to detect black holes some subsidiary indirect methods are used. Detection of the black bodies by their “gravitational effect on the luminous matter” (Ryden, 2003) is one of the initial attempts done to detect the black holes.  Some of the newer methods of detection of the black holes are by using X-Rays, detecting rotating stars or by gravity lenses (Miller, 1996).

The intense gravitational pull of the black hole will cause the nearby particles to heat and that will emit a lot of heat energy and X-Rays. The astronomer’s use this X-Rays to isolate the black holes in the region. Sometimes the star rotates around an area. The astronomers will detect from the rotation of the stars the location of the black holes (Miller, 1996). Another technique to detect the black holes is the use of gravitational lens.

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