Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model
In this current study, we explore the modified homogeneous cosmological model in the background of LRS Bianchi type-<i>I</i> space−time. For this purpose, we employ the Homotopy Perturbation Method (HPM). HPM is an analytical-based method. Further, we calculated the main field...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-03-01
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| Series: | Symmetry |
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| Online Access: | https://www.mdpi.com/2073-8994/12/3/403 |
| _version_ | 1811307062215311360 |
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| author | Yihu Feng Lei Hou |
| author_facet | Yihu Feng Lei Hou |
| author_sort | Yihu Feng |
| collection | DOAJ |
| description | In this current study, we explore the modified homogeneous cosmological model in the background of LRS Bianchi type-<i>I</i> space−time. For this purpose, we employ the Homotopy Perturbation Method (HPM). HPM is an analytical-based method. Further, we calculated the main field equations of the cosmological model LRS Bianchi type-<i>I</i> space−time. Furthermore, we discuss the necessary calculations of HPM. Therefore, we investigate the analytical solution of our problem by adopting HPM. In this response, we discuss five different values of parameter n. We also give a brief discussion about solutions. The main purpose of this study is to apply the application of HPM in the cosmological field. |
| first_indexed | 2024-04-13T08:57:40Z |
| format | Article |
| id | doaj.art-9b4eb00254ef4880937fcf444764d530 |
| institution | Directory Open Access Journal |
| issn | 2073-8994 |
| language | English |
| last_indexed | 2024-04-13T08:57:40Z |
| publishDate | 2020-03-01 |
| publisher | MDPI AG |
| record_format | Article |
| series | Symmetry |
| spelling | doaj.art-9b4eb00254ef4880937fcf444764d5302022-12-22T02:53:14ZengMDPI AGSymmetry2073-89942020-03-0112340310.3390/sym12030403sym12030403Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological ModelYihu Feng0Lei Hou1Department of Mathematics, Shanghai University, Shanghai 200444, ChinaDepartment of Mathematics, Shanghai University, Shanghai 200444, ChinaIn this current study, we explore the modified homogeneous cosmological model in the background of LRS Bianchi type-<i>I</i> space−time. For this purpose, we employ the Homotopy Perturbation Method (HPM). HPM is an analytical-based method. Further, we calculated the main field equations of the cosmological model LRS Bianchi type-<i>I</i> space−time. Furthermore, we discuss the necessary calculations of HPM. Therefore, we investigate the analytical solution of our problem by adopting HPM. In this response, we discuss five different values of parameter n. We also give a brief discussion about solutions. The main purpose of this study is to apply the application of HPM in the cosmological field.https://www.mdpi.com/2073-8994/12/3/403lrs bianchi type-<i>i</i> space–timehpmcosmological model |
| spellingShingle | Yihu Feng Lei Hou Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model Symmetry lrs bianchi type-<i>i</i> space–time hpm cosmological model |
| title | Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model |
| title_full | Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model |
| title_fullStr | Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model |
| title_full_unstemmed | Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model |
| title_short | Approximate Solutions of the LRS Bianchi Type-<i>I</i> Cosmological Model |
| title_sort | approximate solutions of the lrs bianchi type i i i cosmological model |
| topic | lrs bianchi type-<i>i</i> space–time hpm cosmological model |
| url | https://www.mdpi.com/2073-8994/12/3/403 |
| work_keys_str_mv | AT yihufeng approximatesolutionsofthelrsbianchitypeiiicosmologicalmodel AT leihou approximatesolutionsofthelrsbianchitypeiiicosmologicalmodel |