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Keywords = gas of null strings

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8 pages, 216 KB  
Proceeding Paper
The Evolution of Dark Energy in a Model of a Gas of Thin Tubes of a Massless Scalar Field
by Alexander Lelyakov and Stepan Lelyakov
Phys. Sci. Forum 2026, 14(1), 12; https://doi.org/10.3390/psf2026014012 - 29 Jul 2026
Viewed by 115
Abstract
We have shown the possibility of realizing the phase of phantom dark energy in a gas of thin tubes of a massless scalar field, and we have also shown that in the process of evolution, the phantom component of dark energy in such [...] Read more.
We have shown the possibility of realizing the phase of phantom dark energy in a gas of thin tubes of a massless scalar field, and we have also shown that in the process of evolution, the phantom component of dark energy in such a gas can become equal to zero. In this case, starting from a certain point in time, the total value of the parameter of the equation of state for a gas of thin tubes of a massless scalar field will satisfy the inequality w > 1 . Full article
(This article belongs to the Proceedings of The 3rd International Online Conference on Universe)
9 pages, 770 KB  
Proceeding Paper
“Null String” Gas Cosmology: 1st Steps
by Alexander Lelyakov
Phys. Sci. Forum 2021, 2(1), 14; https://doi.org/10.3390/ECU2021-09330 - 23 Feb 2021
Viewed by 4673
Abstract
This work is devoted to the study of the asymptotics of the gravitational field of primary particles with nonzero rest mass. These particles are structurally composed of two closed “null strings” (thin closed tubes of a massless scalar field) in the shape of [...] Read more.
This work is devoted to the study of the asymptotics of the gravitational field of primary particles with nonzero rest mass. These particles are structurally composed of two closed “null strings” (thin closed tubes of a massless scalar field) in the shape of a circle, and they are formed in a gas of null strings as a result of gravitational interaction. It is shown that on time scales much larger than the time of one complete cycle of oscillation of the null strings forming a particle, or at distances much larger than the dimensions of the region within which the oscillations of interacting null strings occur, the gravitational field of such a particle is described by the Minkowski metric. It is noted that with decreasing observation time or on distance scales that are commensurate with the size of primary particles, significant deviations of the gravitational field from the flat Minkowski space-time should appear in the gas of null strings. Full article
(This article belongs to the Proceedings of The 1st Electronic Conference on Universe)
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17 pages, 577 KB  
Article
Gravitational Interaction in a Null String Gas and Its Possible Consequences
by Alexander Lelyakov
Universe 2020, 6(9), 142; https://doi.org/10.3390/universe6090142 - 2 Sep 2020
Cited by 7 | Viewed by 5878
Abstract
In this paper, we investigated the possible consequences of gravitational interaction in a gas of null strings. The structural elements of this gas are closed null strings in the form of a circle (thin closed tubes of massless scalar field). A possibility to [...] Read more.
In this paper, we investigated the possible consequences of gravitational interaction in a gas of null strings. The structural elements of this gas are closed null strings in the form of a circle (thin closed tubes of massless scalar field). A possibility to qualitatively take into account the mutual influence on motion for gravitationally interacting null strings is proposed. It is shown that the result of gravitational interaction is the self-consistent motion of two null strings inside a space-limited region. Such systems of gravitationally interacting null strings can be considered as primary particles in a gas of null strings with an effective nonzero rest mass. It is noted that the “lifetime” of such particles should depend on external conditions. Long-term existence (“lifetime”) of primary particles is possible if they are combined into more complex structures. The possibility of such a union depends on the motion direction of the null strings forming the particles. The most interesting is the possibility of combining primary particles into spherically symmetric formations—“macro” objects. A feature of such “macro” formations in a gas of null strings is the fundamental impossibility to have finally formed structure. In a gas of null strings, processes leading to a random (dynamic) change in the number of null strings gravitationally belonging to a “macro” object are inevitable. By averaging over time the various spatial distributions of the “macro” formations, the concepts of “substance” and “interaction field” can be introduced in a gas of null strings. Full article
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