Wormholes and Teleporters

Igor Nikitin

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Wormholes and Teleporters

Igor Nikitin

General Physics · Submitted 2 Mar 2021

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Using analytical and numerical methods, as well as visualization, we will construct an example of an opening and closing wormhole with the dimensions of the central black hole in the Milky Way galaxy.

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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,471 input tokens.

What the abstract itself states, as probabilities: claims first 0.06 · states limitation 0.21 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.12 · compares with prior results 0.82 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; show every role.

In general relativity, there is a class of solutions that currently do not have observed analogues, but on which the theory is shaped, giving an understanding what is fundamentally possible within its framework. Such solutions include wormholes, tunnels that connect distant regions in spacetime. Although not a single wormhole has yet been discovered, there is a large number of works devoted to their study, thanks to which wormholes as a class of solutions become firmly established in modern science. In this paper, we consider two topologically nontrivial types of solutions related to wormholes. First: wormholes that can open and close. In this relation, we will discuss topological censorship theorems, which under certain conditions prohibit changing topology. We will also discuss known ways to circumvent these theorems. Using analytical and numerical methods, as well as visualization, we will construct an example of an opening and closing wormhole with the dimensions of the central black hole in the Milky Way galaxy. Our construction continues the work by Kardashev, Novikov and Shatskiy, in which a static wormhole with the same parameters was considered. The second type is a modification of Visser's dihedral wormhole solution for a dynamic case, which can be considered as a model of a teleportation event.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	In general relativity, there is a class of solutions that currently do not have observed analogues, but on which the theory is shaped, giving an understanding what is fundamentally possible within its framework.	background 1.00	0.03	0.03	asserted 0.99
s1	Such solutions include wormholes, tunnels that connect distant regions in spacetime.	background 1.00	0.04	0.02	asserted 1.00
s2	Although not a single wormhole has yet been discovered, there is a large number of works devoted to their study, thanks to which wormholes as a class of solutions become firmly established in modern science.	background 1.00	0.03	0.03	asserted 1.00
s3	In this paper, we consider two topologically nontrivial types of solutions related to wormholes.	contribution 0.97	0.42	0.04	asserted 0.95
s4	First: wormholes that can open and close.	contribution 0.93	0.12	0.04	asserted 0.87
s5	In this relation, we will discuss topological censorship theorems, which under certain conditions prohibit changing topology.	background 0.75	0.10	0.04	asserted 0.95
s6	We will also discuss known ways to circumvent these theorems.	contribution 0.81	0.21	0.03	asserted 0.84
s7	Using analytical and numerical methods, as well as visualization, we will construct an example of an opening and closing wormhole with the dimensions of the central black hole in the Milky Way galaxy.	contribution 0.80	0.94	0.17	asserted 0.96
s8	Our construction continues the work by Kardashev, Novikov and Shatskiy, in which a static wormhole with the same parameters was considered.	background 0.68	0.38	0.04	asserted 1.00
s9	The second type is a modification of Visser's dihedral wormhole solution for a dynamic case, which can be considered as a model of a teleportation event.	contribution 0.97	0.53	0.08	hedged possibility 0.57

What kind of paper the classifier reports this is: theoretical result 0.91 · evidence from proof or derivation 0.56.

What was examined, and what was not

sources read

arXiv listing abstract v1

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

In general relativity, there is a class of solutions that currently do not have observed analogues, but on which the theory is shaped, giving an understanding what is fundamentally possible within its framework. Such solutions include wormholes, tunnels that connect distant regions in spacetime. Although not a single wormhole has yet been discovered, there is a large number of works devoted to their study, thanks to which wormholes as a class of solutions become firmly established in modern science. In this paper, we consider two topologically nontrivial types of solutions related to wormholes. First: wormholes that can open and close. In this relation, we will discuss topological censorship theorems, which under certain conditions prohibit changing topology. We will also discuss known ways to circumvent these theorems. Using analytical and numerical methods, as well as visualization, we will construct an example of an opening and closing wormhole with the dimensions of the central black hole in the Milky Way galaxy. Our construction continues the work by Kardashev, Novikov and Shatskiy, in which a static wormhole with the same parameters was considered. The second type is a modification of Visser's dihedral wormhole solution for a dynamic case, which can be considered as a model of a teleportation event.

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What this paper does with the arXiv papers it cites

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

What it cites · 39 sentences without a confident label

Uses the method or tool of 2 papers

The solution is found numerically, by integration procedure [ref] .

Static spherically symmetric solutions of Einstein field equations with radial dark matter · Opening wormholes · 1.00
Then the metric ([ref]) will be [equation] Using the coordinate transformation [ref] , the metric is simplified to [equation] coincident with the flat Minkowski plane, covered twice by the transformation $(x,y)→(u,v)$.

Complex actions in two-dimensional topology change · Opening wormholes, details of construction · 0.85

Uses data or values from 1 paper

Since the NRDM solution differs from the Schwarzschild one, the setting of the starting point at a large radius in weak fields should use a slightly different nominal value $r_s, nom = 1.32 ·10^10$m, to be compatible with the observed value $r_s = 1.2 ·10^10$m by Ghez et al. [ref] , in strong fields.

Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits · Opening wormholes · 0.99

Compares with 7 papers

After the application of the algorithm Einstein to the metric ([ref]), we obtain [equation] this result can be also cross-checked against the formulas in [ref] and [ref] .

From the Flamm-Einstein-Rosen bridge to the modern renaissance of traversable wormholes · Topology change · 0.99
The same result was also obtained by [ref] using other types of regularization.

Complex actions in two-dimensional topology change · Stargates and teleporters, details of construction · 0.91
The same result was also obtained by [ref] using other types of regularization.

On the Distributional Nature of the Energy Momentum Tensor of a Black Hole or What Curves the Schwarzschild Geometry ? · Stargates and teleporters, details of construction · 0.91

Cites as background 8 papers

This question was examined in detail in [ref] Chap.6.5, based on the original works [ref] .

Topology Change in Classical General Relativity · Topology change · 0.97
The progress has been described in the book [ref] , the recent developments were reported in [ref] .

From the Flamm-Einstein-Rosen bridge to the modern renaissance of traversable wormholes · Introduction · 1.00
The works [ref] have considered QG-corrections to Friedmann cosmological model with a scalar field.

Quantum Nature of the Big Bang: An Analytical and Numerical Investigation · Topology change · 0.87

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