{"title":"根据ACT数据的非最小耦合","authors":"Qing Gao , Yungui Gong , Zhu Yi , Fengge Zhang","doi":"10.1016/j.dark.2025.102106","DOIUrl":null,"url":null,"abstract":"<div><div>The latest ACT data release disfavors the attractor <span><math><mrow><msub><mrow><mi>n</mi></mrow><mrow><mi>s</mi></mrow></msub><mo>=</mo><mn>1</mn><mo>−</mo><mn>2</mn><mo>/</mo><mi>N</mi></mrow></math></span>. In inflationary models with nonminimal coupling, such attractors typically arise in the strong coupling limit. To align with observational constraints, we focus on nonminimal coupling models with small coupling constants. For the model with the coupling function <span><math><mrow><mi>Ω</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><mn>1</mn><mo>+</mo><mi>ξ</mi><mi>f</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow></mrow></math></span> and the potential <span><math><mrow><mi>V</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><msup><mrow><mi>λ</mi></mrow><mrow><mn>2</mn></mrow></msup><msup><mrow><mi>f</mi></mrow><mrow><mn>2</mn></mrow></msup><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow></mrow></math></span>, we find that observational data constrain the parameters as <span><math><mrow><mn>0</mn><mo>.</mo><mn>1</mn><mo>≲</mo><mi>ξ</mi><mo>≲</mo><mn>35</mn></mrow></math></span> and <span><math><mrow><mn>0</mn><mo>≲</mo><mi>k</mi><mo>≲</mo><mn>1</mn><mo>.</mo><mn>5</mn></mrow></math></span> for <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><msup><mrow><mi>ϕ</mi></mrow><mrow><mi>k</mi></mrow></msup></mrow></math></span> at the <span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> confidence level. With the help of the nonminimal coupling <span><math><mrow><mi>Ω</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><mn>1</mn><mo>+</mo><mi>ξ</mi><msup><mrow><mi>ϕ</mi></mrow><mrow><mn>2</mn></mrow></msup></mrow></math></span>, the hilltop inflation and power-law inflation models with power indices <span><math><mrow><mn>2</mn><mo>/</mo><mn>3</mn></mrow></math></span> and <span><math><mrow><mn>1</mn><mo>/</mo><mn>3</mn></mrow></math></span> can be consistent with observational data within the <span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> range. We also give the viable parameter regions of <span><math><mi>ξ</mi></math></span> for these three models.</div></div>","PeriodicalId":48774,"journal":{"name":"Physics of the Dark Universe","volume":"50 ","pages":"Article 102106"},"PeriodicalIF":6.4000,"publicationDate":"2025-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Nonminimal coupling in light of ACT data\",\"authors\":\"Qing Gao , Yungui Gong , Zhu Yi , Fengge Zhang\",\"doi\":\"10.1016/j.dark.2025.102106\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The latest ACT data release disfavors the attractor <span><math><mrow><msub><mrow><mi>n</mi></mrow><mrow><mi>s</mi></mrow></msub><mo>=</mo><mn>1</mn><mo>−</mo><mn>2</mn><mo>/</mo><mi>N</mi></mrow></math></span>. In inflationary models with nonminimal coupling, such attractors typically arise in the strong coupling limit. To align with observational constraints, we focus on nonminimal coupling models with small coupling constants. For the model with the coupling function <span><math><mrow><mi>Ω</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><mn>1</mn><mo>+</mo><mi>ξ</mi><mi>f</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow></mrow></math></span> and the potential <span><math><mrow><mi>V</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><msup><mrow><mi>λ</mi></mrow><mrow><mn>2</mn></mrow></msup><msup><mrow><mi>f</mi></mrow><mrow><mn>2</mn></mrow></msup><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow></mrow></math></span>, we find that observational data constrain the parameters as <span><math><mrow><mn>0</mn><mo>.</mo><mn>1</mn><mo>≲</mo><mi>ξ</mi><mo>≲</mo><mn>35</mn></mrow></math></span> and <span><math><mrow><mn>0</mn><mo>≲</mo><mi>k</mi><mo>≲</mo><mn>1</mn><mo>.</mo><mn>5</mn></mrow></math></span> for <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><msup><mrow><mi>ϕ</mi></mrow><mrow><mi>k</mi></mrow></msup></mrow></math></span> at the <span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> confidence level. With the help of the nonminimal coupling <span><math><mrow><mi>Ω</mi><mrow><mo>(</mo><mi>ϕ</mi><mo>)</mo></mrow><mo>=</mo><mn>1</mn><mo>+</mo><mi>ξ</mi><msup><mrow><mi>ϕ</mi></mrow><mrow><mn>2</mn></mrow></msup></mrow></math></span>, the hilltop inflation and power-law inflation models with power indices <span><math><mrow><mn>2</mn><mo>/</mo><mn>3</mn></mrow></math></span> and <span><math><mrow><mn>1</mn><mo>/</mo><mn>3</mn></mrow></math></span> can be consistent with observational data within the <span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> range. We also give the viable parameter regions of <span><math><mi>ξ</mi></math></span> for these three models.</div></div>\",\"PeriodicalId\":48774,\"journal\":{\"name\":\"Physics of the Dark Universe\",\"volume\":\"50 \",\"pages\":\"Article 102106\"},\"PeriodicalIF\":6.4000,\"publicationDate\":\"2025-09-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics of the Dark Universe\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S2212686425002997\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of the Dark Universe","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2212686425002997","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
The latest ACT data release disfavors the attractor . In inflationary models with nonminimal coupling, such attractors typically arise in the strong coupling limit. To align with observational constraints, we focus on nonminimal coupling models with small coupling constants. For the model with the coupling function and the potential , we find that observational data constrain the parameters as and for at the confidence level. With the help of the nonminimal coupling , the hilltop inflation and power-law inflation models with power indices and can be consistent with observational data within the range. We also give the viable parameter regions of for these three models.
期刊介绍:
Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact.
The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.