{"title":"N =2超重力宇宙学对Calabi-Yau流形拓扑的意义","authors":"S. Salem, Moataz H Emam, H. Salah","doi":"10.21608/absb.2022.121518.1172","DOIUrl":null,"url":null,"abstract":"When N = 1 D = 11 supergravity is compactified on CY threefold to N = 2 D = 5 supergravity the action of the last is given in terms of the geometery of the CY manifold space, namely, in terms of the hypermultiplets. There are z i ( i = 1 , ..., h 2 , 1 ) complex structure moduli in the moduli space of the CY manifold which’s a special K¨ahler manifold with a metric G i ¯ j . We solve the field equations of the complex structure moduli with the solution of the Einstein field equations to the moduli velocity norm G i ¯ j z i z ¯ j in case of a 3- brane filled with radiation, dust and energy embedded in the bulk of D = 5 supergravity. We get the time dependence of the moduli and the metric. Then we can further deduce the geometry of the moduli space by getting the K¨ahler potential which directly relates to the volume of the CY manifold.","PeriodicalId":7687,"journal":{"name":"Al-Azhar Bulletin of Science","volume":"23 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2022-03-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"The Implications of N =2 Supergravity Cosmology On the Topology of the Calabi-Yau Manifold\",\"authors\":\"S. Salem, Moataz H Emam, H. Salah\",\"doi\":\"10.21608/absb.2022.121518.1172\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"When N = 1 D = 11 supergravity is compactified on CY threefold to N = 2 D = 5 supergravity the action of the last is given in terms of the geometery of the CY manifold space, namely, in terms of the hypermultiplets. There are z i ( i = 1 , ..., h 2 , 1 ) complex structure moduli in the moduli space of the CY manifold which’s a special K¨ahler manifold with a metric G i ¯ j . We solve the field equations of the complex structure moduli with the solution of the Einstein field equations to the moduli velocity norm G i ¯ j z i z ¯ j in case of a 3- brane filled with radiation, dust and energy embedded in the bulk of D = 5 supergravity. We get the time dependence of the moduli and the metric. Then we can further deduce the geometry of the moduli space by getting the K¨ahler potential which directly relates to the volume of the CY manifold.\",\"PeriodicalId\":7687,\"journal\":{\"name\":\"Al-Azhar Bulletin of Science\",\"volume\":\"23 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-03-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Al-Azhar Bulletin of Science\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.21608/absb.2022.121518.1172\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Al-Azhar Bulletin of Science","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.21608/absb.2022.121518.1172","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
摘要
当N = 1 D = 11的超引力在CY上三倍紧化到N = 2 D = 5的超引力时,最后一个的作用用CY流形空间的几何形式,即用超多重态给出。有zi (i = 1,…)(h²,1)复结构模在CY流形的模空间中,CY流形是一个特殊的K´ahler流形,度量是gi¯j。我们用爱因斯坦场方程对模速度范数G i¯j z i z¯j的解来求解复杂结构模的场方程,在D = 5超重力体中嵌入了一个充满辐射、尘埃和能量的3膜。我们得到模和度规的时间依赖性。然后,我们可以通过得到与CY流形体积直接相关的K¨ahler势进一步推导出模空间的几何形状。
The Implications of N =2 Supergravity Cosmology On the Topology of the Calabi-Yau Manifold
When N = 1 D = 11 supergravity is compactified on CY threefold to N = 2 D = 5 supergravity the action of the last is given in terms of the geometery of the CY manifold space, namely, in terms of the hypermultiplets. There are z i ( i = 1 , ..., h 2 , 1 ) complex structure moduli in the moduli space of the CY manifold which’s a special K¨ahler manifold with a metric G i ¯ j . We solve the field equations of the complex structure moduli with the solution of the Einstein field equations to the moduli velocity norm G i ¯ j z i z ¯ j in case of a 3- brane filled with radiation, dust and energy embedded in the bulk of D = 5 supergravity. We get the time dependence of the moduli and the metric. Then we can further deduce the geometry of the moduli space by getting the K¨ahler potential which directly relates to the volume of the CY manifold.