修正重力模型和虫洞解决方案

IF 1.5 4区 物理与天体物理 Q3 PHYSICS, PARTICLES & FIELDS Advances in High Energy Physics Pub Date : 2024-03-12 DOI:10.1155/2024/3717418
S. Davood Sadatian, S. Mohamad Reza Hosseini
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We show that there is no need to define a wormhole from exotic matter and analyze the equations with numerical analysis to establish weak energy conditions. In the numerical analysis, we found that the appropriate values of the parameters can maintain the weak energy conditions without the need for exotic matter. Adjusting the parameters of the model can increase or decrease the rate of positive energy density or radial and tangential pressures. According to the numerical analysis conducted in this paper, the weak energy conditions are established in the whole space if <span><svg height=\"8.98582pt\" style=\"vertical-align:-0.6370001pt\" version=\"1.1\" viewbox=\"-0.0498162 -8.34882 18.648 8.98582\" width=\"18.648pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,11.017,0)\"></path></g></svg><span></span><svg height=\"8.98582pt\" style=\"vertical-align:-0.6370001pt\" version=\"1.1\" viewbox=\"22.230183800000002 -8.34882 6.418 8.98582\" width=\"6.418pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,22.28,0)\"></path></g></svg></span> and <span><svg height=\"12.7178pt\" style=\"vertical-align:-3.42947pt\" version=\"1.1\" viewbox=\"-0.0498162 -9.28833 39.187 12.7178\" width=\"39.187pt\" xmlns=\"http://www.w3.org/2000/svg\" 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xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,65.268,0)\"><use xlink:href=\"#g113-51\"></use></g><g transform=\"matrix(.013,0,0,-0.013,71.508,0)\"><use xlink:href=\"#g113-54\"></use></g><g transform=\"matrix(.013,0,0,-0.013,77.748,0)\"><use xlink:href=\"#g113-47\"></use></g><g transform=\"matrix(.013,0,0,-0.013,80.712,0)\"><use xlink:href=\"#g113-50\"></use></g><g transform=\"matrix(.013,0,0,-0.013,86.952,0)\"><use xlink:href=\"#g113-51\"></use></g></svg></span> or <span><svg height=\"8.98582pt\" style=\"vertical-align:-0.6370001pt\" version=\"1.1\" viewbox=\"-0.0498162 -8.34882 18.648 8.98582\" width=\"18.648pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"><use xlink:href=\"#g113-223\"></use></g><g transform=\"matrix(.013,0,0,-0.013,11.017,0)\"></path></g></svg><span></span><svg height=\"8.98582pt\" style=\"vertical-align:-0.6370001pt\" version=\"1.1\" viewbox=\"22.230183800000002 -8.34882 6.418 8.98582\" width=\"6.418pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,22.28,0)\"><use xlink:href=\"#g113-49\"></use></g></svg></span> and <span><svg height=\"12.7178pt\" style=\"vertical-align:-3.42947pt\" version=\"1.1\" viewbox=\"-0.0498162 -9.28833 18.817 12.7178\" width=\"18.817pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"><use xlink:href=\"#g113-224\"></use></g><g transform=\"matrix(.013,0,0,-0.013,11.186,0)\"><use xlink:href=\"#g117-92\"></use></g></svg><span></span><span><svg height=\"12.7178pt\" style=\"vertical-align:-3.42947pt\" version=\"1.1\" viewbox=\"22.399183800000003 -9.28833 28.184 12.7178\" width=\"28.184pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g 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We show that there is no need to define a wormhole from exotic matter and analyze the equations with numerical analysis to establish weak energy conditions. In the numerical analysis, we found that the appropriate values of the parameters can maintain the weak energy conditions without the need for exotic matter. Adjusting the parameters of the model can increase or decrease the rate of positive energy density or radial and tangential pressures. According to the numerical analysis conducted in this paper, the weak energy conditions are established in the whole space if <span><svg height=\\\"8.98582pt\\\" style=\\\"vertical-align:-0.6370001pt\\\" version=\\\"1.1\\\" viewbox=\\\"-0.0498162 -8.34882 18.648 8.98582\\\" width=\\\"18.648pt\\\" xmlns=\\\"http://www.w3.org/2000/svg\\\" xmlns:xlink=\\\"http://www.w3.org/1999/xlink\\\"><g transform=\\\"matrix(.013,0,0,-0.013,0,0)\\\"></path></g><g transform=\\\"matrix(.013,0,0,-0.013,11.017,0)\\\"></path></g></svg><span></span><svg height=\\\"8.98582pt\\\" style=\\\"vertical-align:-0.6370001pt\\\" version=\\\"1.1\\\" viewbox=\\\"22.230183800000002 -8.34882 6.418 8.98582\\\" width=\\\"6.418pt\\\" xmlns=\\\"http://www.w3.org/2000/svg\\\" xmlns:xlink=\\\"http://www.w3.org/1999/xlink\\\"><g transform=\\\"matrix(.013,0,0,-0.013,22.28,0)\\\"></path></g></svg></span> and <span><svg height=\\\"12.7178pt\\\" style=\\\"vertical-align:-3.42947pt\\\" version=\\\"1.1\\\" viewbox=\\\"-0.0498162 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引用次数: 0

摘要

我们利用带粘性的修正引力模型研究虫洞解决方案,目的是在不违反能量条件的情况下从数学上找到虫洞存在的解决方案。我们证明无需从奇异物质中定义虫洞,并通过数值分析方程建立弱能量条件。在数值分析中,我们发现适当的参数值可以维持弱能量条件,而不需要外来物质。调整模型参数可以增加或减少正能量密度或径向和切向压强的速率。根据本文的数值分析,如果 和 或 和 ,则整个空间的弱能量条件成立。分析还表明,虫洞的支撑物质接近于正常物质,这表明带粘性的广义模型具有可接受的参数空间来描述虫洞,而不需要奇异物质。
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Modified Gravity Model and Wormhole Solution
We investigate wormhole solutions using the modified gravity model with viscosity and aim to find a solution for the existence of wormholes mathematically without violating the energy conditions. We show that there is no need to define a wormhole from exotic matter and analyze the equations with numerical analysis to establish weak energy conditions. In the numerical analysis, we found that the appropriate values of the parameters can maintain the weak energy conditions without the need for exotic matter. Adjusting the parameters of the model can increase or decrease the rate of positive energy density or radial and tangential pressures. According to the numerical analysis conducted in this paper, the weak energy conditions are established in the whole space if and or and . The analysis also showed that the supporting matter of the wormhole is near normal matter, indicating that the generalized model with viscosity has an acceptable parameter space to describe a wormhole without the need for exotic matter.
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来源期刊
Advances in High Energy Physics
Advances in High Energy Physics PHYSICS, PARTICLES & FIELDS-
CiteScore
3.40
自引率
5.90%
发文量
55
审稿时长
6-12 weeks
期刊介绍: Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.
期刊最新文献
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