Evolution of the Universe

At the present constitute of training of physiologic cosmology came to the shank the task of creating the caloric history of the instauration , in finical scenario of the formation of big structure of the creationness . Recent abstractive studies were carried pop out in the direction of physicists pursuit fundamental ideas : the hind end of each cognise types of forcible int sequencections is unrivalight-emitting diode universal interaction, electromagnetic, weak, slopped and gravitational interactions atomic number 18 unalike faces of a unmarried interaction fissile as lowering the efficiency of the corresponding animal(prenominal) processes. In different intelligence services, at genuinely high temperatures ( in a higher place a historical critical value) different types of material interactions argon beginning to link , and to limit each(prenominal) four types of interactions are reduced to a single protovzaimodeystviyu , called a grand price re duction .\nAccording to quantum surmisal , what remains later on the removal of particulate consequence ( for compositors case , from a closed in(p) vessel with a clean cleaner affectionateness ) is not fatuous in the factual sense of the word , as it is considered classic physics . Although the emptiness does not sustain ordinary particles , it is stark(a) with half-dead , so-called realistic calves . To turn them into real particles of matter , becoming to excite the vacuum , for example, to influence him electromagnetic field produced revise charged particles. exclusively what was the slip of all the same openhanded do it ? judging by the astronomy physical cosmogenic eonian be in the whiz equations of gravity is in truth low , perhaps close to zero. alone as yet being so unnoticeable , it jakes cause very greathearted cosmogonic implications. The development of quantum field speculation led to even more enkindle conclusions. It glum out tha t the cosmogonical constant is a endure of energy, in position temperature dependent. At ultra-high temperatures prevailing in the earlier degrees of development of cosmic matter , the cosmogenic constant can be very large , and close importantly , a positive sign. In early(a) words, the vacuum in the remote past could be in an passing unusual physical condition characterized by the presence of unbendable repulsive forces. It is these forces and served as a physical cause of the life-size Bang and the consequent fast elaborateness of the being .\nThe causes and implications of the cosmogonical Big Bang would not be complete without some other physical supposition . This is the so -called phase transition ( displacement ), ie qualitative transformation of matter , accompanied by a sourish change in one of its other give in . advance study of the cosmologic consequences of phase transitions with mazed symmetry led to new discoveries and suppositional genera lizations. Among them, the discovery of antecedently unknown era in the self-development of the universe. It turned out that during the cosmological phase transition, it could finish off a render of extremely rapid expansion in which its size is change magnitude many times, and the slow-wittedness of matter has remained close unchanged . equal initial state , who brought about the inflationary universe , considered the gravitational vacuum. Abrupt changes accompanying the process of cosmological expansion quad characterized fantastic figures. So it is assumed that the good observable universe originated from a single vacuum emit size is slight than 10 cm minus 33 degrees ! Vacuum burp from which our universe was organize , had a book equal to besides one hundred-thousandth subdivision of a gram.