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The Black Hole, An Ocean of Mystery

 

                    There is no doubt or disagreement that the ‘Black Hole’ is one of the most talked about and enigmatic aspects of space exploration. Scientists have been researching this subject for many years and even decades. Today we will try to know a little bit about this subject.

                    The subject was first highlighted in 1784 by the English clergyman John Mitchell. He identified this celestial object as a 'Dark star' and later as a 'Gravitationally Collapsed Object'. This idea was later supported by the mathematician Pierre Simon Laplace. The term black hole was probably first used by the American astronomer Robert Dicke. The word was first printed in 1963 by journalist Ann Ewing in her article. A few days later, in a lecture by scientist John Wheeler, a young student suggested the use of the word 'Black Hole', and scientist Wheeler accepted it, and the use of the word 'Black Hole' has increased since then. So many give credit to John Wheeler for introducing the word Black Hole'.

                    A black hole is a dark region whose very strong force of attraction attracts any object, even electromagnetic waves (light). Einstein's 'Law of General Relativity' states that what we perceive as a gravitational force is actually obtained from the curvature of space and time. According to that theory of relativity, a large amount of mass condenses together to form this black hole. John Mitchell was the first to say through his mathematical method that the escape velocity of a black hole must be greater than the speed of light. (Escape Velocity: The minimum speed required to get out of the gravitational force of a cosmic object.) Of course, John Mitchell also said about one and an half hundred years ago that in order to identify the black hole, one must analyze its gravitational effect on the surrounding objects of the black hole, which is accepted today as a recognized method.

                    Now we will try to understand how this black hole is actually created. Hydrogen acts as the fuel for any major star. This hydrogen produces helium through the process of nuclear fusion, which in turn produces light energy and heat energy and radiates. Thus, after hundreds of billions of runs, when hydrogen is depleted, the process of atomic addition of helium begins and it produces carbon. Then in this way neon, oxygen and silicon are produced respectively and finally iron is produced. This iron is a very strong, compact and stable substance. So after that the process of nuclear fusion is completely stopped and as a result the process of heat and light energy production also comes to a standstill. In this case the mass of the star increases drastically and the force of gravity also increases. A star is stable as long as the value of radiation as the Centrifugal force and gravitational force as its inverse Centripetal force is equal. This stable state is called the Tolman-Oppenheimer-Volkoff Limit. The center of the star is broken by a massive cosmic explosion when the amount of gravitational force inside the star increases further and the value of the equilibrium of the star's interior exceeds the Tolman-Oppenheimer-Volkoff limit. This phenomenon is called Supernova explosion.

                    After this explosion, most of the parts of stars spread far and wide in different parts of space. Here the remnants of a star can pass through two states and it depends on the mass of that state. Indian scientist S. Chandrasekhar explains what can happen in any situation. This system is called Chandrasekhar Limit in recognition of Chandrasekhar's work. If the mass of the remaining stars is equal to or greater than 2.17 times the mass of the Sun, then the remnants of that star will inevitably end up in the black hole. Not only is the black hole created in this way, but the huge amount of gas that was in dense condition in the universe right after the Big Bang came together and formed the black hole. Later, under the influence of their attraction, more gas, dust and even small black holes came and increased the size of these black holes, creating extremely heavy black holes known as Super Massive Black Hole which are usually in the center of a galaxy. For example, at the centre of our Milky Way galaxy is Sagittarius A*. Apart from this, collisions of high energy and high speed objects can also cause black holes. For example, a man-made experiment on earth can be mentioned here. Deep inside the ground near Geneva, Switzerland, CERN's Large Hadron Collider created a black hole-like situation after collision of two objects.


                    There are four types of the black hole, based on its size. Black holes with a mass of 105-1010 times the mass of the sun is called Super Massive Black Hole, a mass between103-104 times that of sun is called Intermediate Mass Black Hole, and a mass of stars between 2.17-102 of that of sun is called Stellar Black Hole and those whose mass is equal to the mass of the moon are called the Micro Black Hole. However, the last mentioned black hole  persisted only for a short time after the Big Bang and now does not exist at present except theoretically. Again, there are four types of black holes based on rotation and electric charge. Non-rotating, charged black hole is called Reissner-Nordstrom-Metric Black Hole, rotating, non-charged black hole is called Ker-Metric Black Hole, non-rotating, non-charged black hole to Schwarzschild Black Hole and rotating, charged black hole is called Merr-Newman-Metric Black Hole. We understand this last to mean black holes because they are so many in numbers.

                     If we talk about the structure of the black hole, then it can be seen that it consists of several parts. The central part of the black hole is called Singularity. According to Einstein's theory of relativity, the centre is a place where the curvature of time and matter, in the three-dimensional universe, is infinite. In a non-rotating black hole, the position of the singularity is like a point, but in a rotating black hole, its position is like a ring. In both cases, however, all the mass of the black hole is concentrated in this volume less space, and the value of its density is infinite. When an object moves under a black hole, it first disintegrates as it moves into infinite density and then turns into smaller parts, eventually merging with the singularity of the black hole. This phenomenon is called ‘Noodle Effect’.

                    The functional part of the ring centered on the singularity of the black hole, after which no object can return out of the black hole, is called the ‘Schwarzschild Radius’. The 'Event Horizon' is marked as the boundary of the functional part of the black hole where this Schwarzschild radius ends. Although the Event Horizon of the non-rotating black hole is completely round where as the Event Horizon of the rotating black hole is oblate. But in reality, the Event Horizon of a black hole is a hypothetical boundary line, so it is never possible to determine such a boundary depending on the size of a black hole. The reason for naming Event Horizon is that it is not yet possible to know the full details of the events that took place on that side of the border.

                    Another ring has been found to be about 1.5 times the distance from the Singularity to the Event Horizon, which is made up of zero-density photon particles. (Photon: The smallest isolated part of an electromagnetic wave or light) This photon is orbitally located around a black hole. If a ray of light passes through this photon ring, then that light travels towards the black hole at a faster speed.

                    The area around the black hole from which the objects lose control and move towards the black hole little by little, means that the intensity of the black hole is first felt after coming to the area where the object changes its position and moves towards the black hole is called Ergosphere. When an object moves into the Ergosphere, it can return to its previous position. Of course it will require extra energy for the object. However, if this event occurs in the polar region of the black hole, then the object will not be able to return in any way because the Ergosphere in the polar region merges perfectly with the Event Horizon. Again, if this happens in the equatorial region, then the least energy must be applied to the object because the expansion of the Ergosphere is the greatest in this region, that is, the distance from the black hole to the edge of the Ergosphere is the greatest here.

                    There is another small region after this Ergosphere and this is the last outer area of the black hole. This part is called the Innermost Stable Circular Orbit or ISCB. In this region, an object can move around the black hole in a steady manner. Its location depends on the nature of the black hole. However, current scientists are still quite skeptical about the structure of the black hole. Einstein himself expressed doubts about this.

                    We cannot see the formation of the black hole. There are basically two reasons for this. First, the attraction of the black hole stops the time because there is a direct relationship between the velocity of light and time. If it is possible for us to observe the events inside the black hole, we would see that everything there was moving at a very slow pace. Again, if it is possible to observe the rest of the universe from inside the black hole, we would see everything moving very fast. This phenomenon is called Gravitational Time Dilation. Nothing can be observed for this infinite delay. Second, since light is absorbed by the black hole, we will see that the light will begin to fade after the star collapse and eventually disappear into the black hole. No information will reach us from there.

                    The black hole is a very mysterious unknown world to us because it is a place where the laws or formulas of physics do not work, so all the events inside it are still incomprehensible to us today. Scientists say that all the measurable information inside the black hole is lost forever. This phenomenon is called Information Loss Paradox. However, from the position around the black hole, scientists speculate that if the black hole is formed after stabilization, three types of features may occur in it. These are firstly, the mass-centered property secondly, the electric-centered property and finally, the angular-momentum-related property. (Angular-momentum: A special feature of physics produced by the rotation of a rotating object) Of course, this assumption is subject to extensive research.

                    There are several things that can be said to be obtained by observing the black hole. On 10th April 2019, a blurry picture of the black hole was first published in front of the people of the world. This was done through a worldwide network of radio telescopes called Event Horizon Telescopes. This black hole is the black hole at the center of the M-87 galaxy or Virgo galaxy, 55,000,000 light-years from Earth, whose mass is 650 crore times the mass of the sun. Here the existence of the black hole is understood due to the curvature of the lines of light near the event horizon of the black hole. Using this same technology, the magnetic field was discovered outside the event horizon of the Sagittarius A* black hole at the center of our galaxy, 25,640 light-years from Earth in 2015. In addition, the gravitational waves that were generated when the two black holes merged on 14th September of that year were observed for the first time. The mass of the two black holes that merged here is 36 times and 29 times the mass of the sun respectively. This is the greatest proof of the presence of a black hole.

                    As for the black hole in the center of our galaxy, the mass of this Sagittarius A* black hole is equal to 4.3 X 106 times the mass of our sun and a little less than 0.02 light-years in diameter. This type of super massive black hole is present in the centre of all galaxies. However, if the mass is taken into account in per unit area, then it can be seen that the mass of the stellar black hole is always greater than that of this type of black hole.

                    In 1974, the famous British scientist Sir Stephen Hawking said that the black hole is not completely dark but emits even a small amount of heat radiation which we call Hawking Radiation which is still widely studied by many scientists around the world. In other words, the energy required for this light and heat radiation is provided by the black hole itself. According to Einstein's mass-energy equation (E=mc2), mass and energy are interrelated, so energy loss means that the mass of the black hole decreases little by little. In this way, the black hole will disappear into space. The temperature we are talking about here is called Hawking Temperature. This temperature is 62 nano Kelvin or -273.15 degree Celsius in the case of black hole like the Sun. This temperature is inversely proportional to the mass of the black hole and proportional to the surface gravity, i.e. the smaller black hole radiates more than the larger one. If this theory is proven, then it can be said that the black hole is gradually evaporating as it compresses with increasing heat radiation. However, the radiation level in the black hole is so low that it is virtually impossible to detect them from earth. However, through mathematical analysis, scientists speculate that an explosion with gamma ray may happen at the end of this process, which may help in the future. In this context, the Fermi Gamma Ray Space Telescope has launched in 2008 for further observation and research.

                    If the light of all the stars in the sky could be obscured in any way, then a glimmer of bright red light could be seen spread all over the sky. This ray of light is the last radiant ray produced after the Big Bang, called Cosmic Microwave Background Radiation. The temperature of this radiation is 2.7 Kelvin or -270.45 degree Celsius. If the radiated temperature of the black hole would be higher than this, it would take 1064 years for the black hole equal to the sun to completely evaporate. In the case of a huge black hole, it will take more time. Although not proven, no second radiation other than Hawking radiation has yet been reported, so indirect observation is more relevant than direct observation for black hole observation.

                    However, it is not yet possible to say exactly what happens after that. A group of that White Holes, Warm Holes may be created through black holes. Another group of scientists says that it will be possible to reach another universe by Time-Travel through the black hole, that is, Multi-verse Theory or Parallel-Universe Hypothesis may be clearly and accurately established in near or far future through the black hole. With the help of modern technology, we may inform our existence in future to new universe through black hole. Another group of scientists claimed that when black hole will come to an end, its mass and material will also facilitate the scientists say birth of new stars. However, there is no doubt that the subject is complex enough and researchable. The only answer lies within the hand of highly advanced technology and research of the future.


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