创造场宇宙学中的五维球形对称宇宙

Q4 Physics and Astronomy
U. K. Panigrahi, R. Patra, M. Sharma
{"title":"创造场宇宙学中的五维球形对称宇宙","authors":"U. K. Panigrahi, R. Patra, M. Sharma","doi":"10.9790/4861-06511418","DOIUrl":null,"url":null,"abstract":"The phenomenon of expanding universe, primordial nucleon-synthesis and the observed isotropy of cosmic microwave background radiation (CMBR) are the three very important observations in astronomy. These were successfully explained by big-bang cosmology based on Einstein’s field equations. Smoot et al. [2] revealed that the earlier prediction of the FriedmanRobertson-Walker type of models do not always exactly match with our expectations. Some puzzling results regarding the red shifts from the extra galactic objects continue to contradict the theoretical explanations given by the big-bang type model. Also, CMBR discovery did not prove it to be outcome of a big-bang theory. In fact, Narlikar et al. [3] have proved the possibility of non-relic interpretation of CMBR. To explain such phenomenon, many alternative theories have been proposed from time to time. Hoyle [4], Bondi and Gold [5] proposed steady state theory in which the universe does neither have singular beginning nor an end on the cosmic time scale. To overcome this difficulty Hoyle and Narlikar [6] adopted a field theoretic approach by introducing a mass-less and charge-less scalar field C in the Einstein-Hilbert action to account for the matter creation. In the Cfield theory introduced by Hoyle and Narlikar, there is no big-bang type of singularity as in the steady state theory of Bondi and Gold [5]. A solution of Einstein’s field equations admitting radiation with negative energy mass less scalar creation field C was obtained by Narlikar and Padmanabhan [1]. The study of Hoyle and Narlikar theory [6-8] of space-times with higher dimensions ____________________ mitasharma08@gmail.com was carried out by Chaterjee and Banarjee [9]. RajBali and Tikekar [10] studied C field Cosmology with variable G in the flat FriedmanRobertson-Walker model and with non flat FRW space time by Raj Bali and Kumawat [11]. The solutions of Einstien’s field equations in the presence of creation field have been obtained for different Binachi type universes by Singh and Chaubey [12]. In the present work, we have studied the Hoyle and Narlikar C-field cosmology in spherical symmetric space time. We have assumed that , = , that is, the creation field C is a function of time‘t’ only.","PeriodicalId":7403,"journal":{"name":"African Review of Physics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2015-01-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"FIVE DIMENSIONAL SPHERICAL SYMMETRIC UNIVERSE IN CREATION FIELD COSMOLOGY\",\"authors\":\"U. K. Panigrahi, R. Patra, M. Sharma\",\"doi\":\"10.9790/4861-06511418\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The phenomenon of expanding universe, primordial nucleon-synthesis and the observed isotropy of cosmic microwave background radiation (CMBR) are the three very important observations in astronomy. These were successfully explained by big-bang cosmology based on Einstein’s field equations. Smoot et al. [2] revealed that the earlier prediction of the FriedmanRobertson-Walker type of models do not always exactly match with our expectations. Some puzzling results regarding the red shifts from the extra galactic objects continue to contradict the theoretical explanations given by the big-bang type model. Also, CMBR discovery did not prove it to be outcome of a big-bang theory. In fact, Narlikar et al. [3] have proved the possibility of non-relic interpretation of CMBR. To explain such phenomenon, many alternative theories have been proposed from time to time. Hoyle [4], Bondi and Gold [5] proposed steady state theory in which the universe does neither have singular beginning nor an end on the cosmic time scale. To overcome this difficulty Hoyle and Narlikar [6] adopted a field theoretic approach by introducing a mass-less and charge-less scalar field C in the Einstein-Hilbert action to account for the matter creation. In the Cfield theory introduced by Hoyle and Narlikar, there is no big-bang type of singularity as in the steady state theory of Bondi and Gold [5]. A solution of Einstein’s field equations admitting radiation with negative energy mass less scalar creation field C was obtained by Narlikar and Padmanabhan [1]. The study of Hoyle and Narlikar theory [6-8] of space-times with higher dimensions ____________________ mitasharma08@gmail.com was carried out by Chaterjee and Banarjee [9]. RajBali and Tikekar [10] studied C field Cosmology with variable G in the flat FriedmanRobertson-Walker model and with non flat FRW space time by Raj Bali and Kumawat [11]. The solutions of Einstien’s field equations in the presence of creation field have been obtained for different Binachi type universes by Singh and Chaubey [12]. In the present work, we have studied the Hoyle and Narlikar C-field cosmology in spherical symmetric space time. We have assumed that , = , that is, the creation field C is a function of time‘t’ only.\",\"PeriodicalId\":7403,\"journal\":{\"name\":\"African Review of Physics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-01-30\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"African Review of Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.9790/4861-06511418\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"African Review of Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.9790/4861-06511418","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 1

摘要

宇宙膨胀现象、原始核子合成和宇宙微波背景辐射各向同性的观测是天文学中非常重要的三个观测结果。这些都被基于爱因斯坦场方程的大爆炸宇宙论成功地解释了。Smoot等人[2]揭示了friedman - robertson - walker类型模型的早期预测并不总是与我们的期望完全匹配。关于星系外天体的红移,一些令人困惑的结果继续与大爆炸模型给出的理论解释相矛盾。此外,CMBR的发现并不能证明它是大爆炸理论的结果。事实上,Narlikar等人[3]已经证明了CMBR非遗迹解释的可能性。为了解释这一现象,人们不时提出许多不同的理论。Hoyle[4]、Bondi和Gold[5]提出了稳态理论,在该理论中,宇宙在宇宙时间尺度上既没有单一的开始也没有单一的结束。为了克服这一困难,Hoyle和Narlikar[6]采用了场论方法,在爱因斯坦-希尔伯特作用中引入了一个无质量和无电荷的标量场C来解释物质的产生。在Hoyle和Narlikar引入的Cfield理论中,不存在像Bondi和Gold的稳态理论[5]那样的大爆炸型奇点。Narlikar和Padmanabhan[1]得到了爱因斯坦场方程的一个解,该解允许具有负能量质量的无标量产生场C的辐射。Chaterjee和Banarjee[9]对高维时空____________________ mitasharma08@gmail.com的Hoyle和Narlikar理论[6-8]进行了研究。RajBali和Tikekar[10]在平坦的friedman - robertson - walker模型中研究了变量G的C场宇宙学,RajBali和Kumawat[11]研究了非平坦的FRW时空。Singh和Chaubey[12]已经得到了不同Binachi型宇宙存在创造场时的爱因斯坦场方程的解。在本工作中,我们研究了球对称时空中的Hoyle和Narlikar c场宇宙学。我们假设,=,即创建域C不仅是时间的函数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
FIVE DIMENSIONAL SPHERICAL SYMMETRIC UNIVERSE IN CREATION FIELD COSMOLOGY
The phenomenon of expanding universe, primordial nucleon-synthesis and the observed isotropy of cosmic microwave background radiation (CMBR) are the three very important observations in astronomy. These were successfully explained by big-bang cosmology based on Einstein’s field equations. Smoot et al. [2] revealed that the earlier prediction of the FriedmanRobertson-Walker type of models do not always exactly match with our expectations. Some puzzling results regarding the red shifts from the extra galactic objects continue to contradict the theoretical explanations given by the big-bang type model. Also, CMBR discovery did not prove it to be outcome of a big-bang theory. In fact, Narlikar et al. [3] have proved the possibility of non-relic interpretation of CMBR. To explain such phenomenon, many alternative theories have been proposed from time to time. Hoyle [4], Bondi and Gold [5] proposed steady state theory in which the universe does neither have singular beginning nor an end on the cosmic time scale. To overcome this difficulty Hoyle and Narlikar [6] adopted a field theoretic approach by introducing a mass-less and charge-less scalar field C in the Einstein-Hilbert action to account for the matter creation. In the Cfield theory introduced by Hoyle and Narlikar, there is no big-bang type of singularity as in the steady state theory of Bondi and Gold [5]. A solution of Einstein’s field equations admitting radiation with negative energy mass less scalar creation field C was obtained by Narlikar and Padmanabhan [1]. The study of Hoyle and Narlikar theory [6-8] of space-times with higher dimensions ____________________ mitasharma08@gmail.com was carried out by Chaterjee and Banarjee [9]. RajBali and Tikekar [10] studied C field Cosmology with variable G in the flat FriedmanRobertson-Walker model and with non flat FRW space time by Raj Bali and Kumawat [11]. The solutions of Einstien’s field equations in the presence of creation field have been obtained for different Binachi type universes by Singh and Chaubey [12]. In the present work, we have studied the Hoyle and Narlikar C-field cosmology in spherical symmetric space time. We have assumed that , = , that is, the creation field C is a function of time‘t’ only.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
African Review of Physics
African Review of Physics PHYSICS, MULTIDISCIPLINARY-
自引率
0.00%
发文量
1
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信