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Все науки. №7, 2024. Международный научный журнал. Ибратжон Хатамович АлиевЧитать онлайн книгу.

Все науки. №7, 2024. Международный научный журнал - Ибратжон Хатамович Алиев


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A «WALL—I», Marco B «Eve», Tianwen-1, Zhuron, Psyche, Hera, Europa Clipper and others [13—14; 15].

      These include the probes of the Mars satellite, as well as other satellites and even asteroids – Dawn, Galileo, who visited asteroids 951 Gaspra, 243 Ida, Clementine, who visited 1620 Geographos, among others. Separately, there are probes of the largest planet – Jupiter in the person of Pioneer 10, Pioneer 11, Cassini, Ulysses, New Horizons, Galileo, Juno, SOC, and its satellites, in particular Ganymede. Also, Saturn – Voyager 1, Voyager 2, Cassini, and its moon Titan – Huygens [7—8; 14—15]. And even the most distant planets of the Solar System – Uranus, Neptune, which Voyager 1 was able to reach, and even the dwarf planet Pluto, which the New Horizons probe was able to reach, which continued its journey and was able to reach the Kuiper belt to the space object 486958 Arrokot, located at a distance of 43.4 astronomical units from the Sun [1—8; 9]!

      Based on the particular list of space objects of artificial and research origin available in space, it becomes obvious that the most important scientific research data on a wide variety of objects in and outside the Solar System must be transmitted at the highest possible speeds. At the moment, taking into account the available technologies, at a distance of 43.4 astronomical units, taking into account the distance to Earth of 42.4 astronomical units from the farthest probe New Horizons, the signal reaches in 21,157.8 seconds or 5 hours 52 minutes and 37.8 seconds.

      In order to be able to transmit a signal over a distance using tunneling technology, it is necessary to initially present the information in the form of a group of charges, a beam, to which additional energy is transmitted. It can be transmitted by means of an electric field in a small portable accelerator, where, upon reaching the required defect, the particle will tunnel at a speed several times higher than the speed of light, according to the nature of the phenomenon of quantum tunneling to Earth at a specified point with a certain error and degree of loss.

      But for a better consideration of the issue, it is necessary to proceed to the formulation of the appropriate task.

      Setting the task

      Initially, it is known that the phenomenon is described by the Schrodinger equation in the dynamic representation (1)

      The equation involves a potential barrier U (x, t), which is a variable function and depends on multiple parameters – objects that are located between the source and the receiver, which must be overcome by the guided particle. Most often, vacuum prevails in outer space, but there are also quite a few obstacles, for the initial idea, we define the value of the potential barrier as the amount of energy of the mass of all matter located on the communication channel, with an average density of matter in the Solar system. Thus, the communication channel is an imaginary cylinder with a radius equal to the radius of a beam of 10 microns, 42.4 astronomical units long, from which the corresponding volume and mass are calculated, taking into account the average density of matter in the solar system of 0.931*10—26 kg/m3 (2).

      And also, based on the height of the potential barrier, it is possible to determine the boundary and initial conditions for the state function of the quantum mechanical system in (3).

      The boundary conditions are formed from several statements. For use, such a system is necessary in which the probability of finding the beam after sending it in the radiator should be zero, at the specified target – on the Ground, should be equal to 100 percent. Despite the fact that with classical propagation at a time, taking into account such distance measurement, it is necessary that after 21,157,80283 seconds-meters, the probability of finding the beam on Earth was 100% and zero when reaching the Sun at 21,656,80762 seconds-meters. Based on the obtained indicators with respect to one dimension and time, equation (1) can be solved with the specified boundary conditions (3).

      To do this, the Fourier variable separation method will be used, with respect to solving an equation of the form (4), the form of the function (5) will be adopted, where, after substitution, the form (6) is formed, from which 2 separate ordinary differential equations are derived.

      The equation is solved in time to the state of the general form, according to (7), but due to the presence of initial conditions in (3), the present form can be solved by means of representation in the form of a system (8), taking into account the finding of the formula-dependence on the independent variables of the general form of the function (9), where after solving the formed equation after substituting the formula of the independent variable, the form of the introduced constant (10) in (6) is formed.

      The value of the constant makes it possible to determine the value of the first and, accordingly, the opposite of the second independent constant (11), which, after substituting into the general form of the time function (7), gives its private emerging form (12) and (Fig. 1).

      Fig. 1. Graph of the function

      To continue the study, after establishing the actual form of the function in time, it is necessary to solve the formed ordinary differential equation with respect to the coordinate, which was obtained in the ratio (6). Since the value for the constant was also obtained in (10), after substitution, a final form of an ordinary differential equation in coordinate is formed, for which there is a constant from the characteristic of the form (13), and then the general form of the function (14).

      When forming the problem, boundary conditions were also indicated, the substitution of which allows us to operate from the conclusions of the expression for the third and also opposite, as can be seen from the boundary conditions, independent constant, which in this case has a large-scale appearance, for which a replacement is introduced (15).

      Substituting the resulting replacement allows you to ultimately form a simplified view of the function at the coordinate (16).

      The result of the study is the assembled form of the function of the quantum mechanical state of the tunneling system. However, in this case, the desired function is initially a probability distribution function, for which only the square of its module has physical meaning. Based on this, it is possible to form the form of the square of the module of the function, as for the boundary conditions to be set, for the reason that initially the problem required complete preservation of information and in the case of data transition to an imaginary space, the boundary conditions were set to the original form of the function, for which the square of the module is represented in (17—18).

      Thus, a full-fledged pattern was derived that predicts the probability distribution of finding a response signal for a given case at the maximum distance from the Earth for the probe.

      Results

      According to the results of the study, a function depending on 2 variables was obtained, which can be constructed and according to the initial projection, the first graph of the function is formed without an additional power factor. After applying the appropriate processing (18), the function remains the same, but its parameters describe the actual picture (Fig. 2).

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