Dark energy and matter interacting scenario to relieve H 0 and S 8 tensions* * Supported by the National SKA Program of China (2022SKA0110200, 2022SKA0110203), and the National Natural Science Foundation of China (11975072, 11875102, 11835009)

IF 3.6 2区物理与天体物理 Q1 PHYSICS, NUCLEAR

中国物理C Pub Date : 2024-05-01 DOI:10.1088/1674-1137/ad2b52

Li-Yang Gao, She-Sheng Xue, Xin Zhang

{"title":"Dark energy and matter interacting scenario to relieve H 0 and S 8 tensions* * Supported by the National SKA Program of China (2022SKA0110200, 2022SKA0110203), and the National Natural Science Foundation of China (11975072, 11875102, 11835009)","authors":"Li-Yang Gao, She-Sheng Xue, Xin Zhang","doi":"10.1088/1674-1137/ad2b52","DOIUrl":null,"url":null,"abstract":"We consider a new cosmological model (called <inline-formula>\n<tex-math><?CDATA $ \\tilde\\Lambda $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M1.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>CDM), in which the vacuum energy interacts with matter and radiation, and test this model using the current cosmological observations. Using the CMB+BAO+SN (CBS) dataset to constrain the model, we find that <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M2.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> and <inline-formula>\n<tex-math><?CDATA $ S_8 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M3.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> tensions are relieved to <inline-formula>\n<tex-math><?CDATA $ 2.87\\sigma $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M4.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> and <inline-formula>\n<tex-math><?CDATA $ 2.77\\sigma $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M5.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>, respectively. However, in this case, the <inline-formula>\n<tex-math><?CDATA $ \\tilde\\Lambda $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M6.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>CDM model is not favored by the data, compared with ΛCDM. We find that when the <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M7.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> and <inline-formula>\n<tex-math><?CDATA $ S_8 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M8.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> data are added to the data combination, the situation is significantly improved. In the CBS+<inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M9.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> case, the model relieves the <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M10.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> tension to <inline-formula>\n<tex-math><?CDATA $ 0.47\\sigma $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M11.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>, and the model is favored over ΛCDM. In the CBS+<inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M12.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>+<inline-formula>\n<tex-math><?CDATA $ S_8 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M13.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> case, we obtain a synthetically best situation, in which the <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M14.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> and <inline-formula>\n<tex-math><?CDATA $ S_8 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M15.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> tensions are relieved to <inline-formula>\n<tex-math><?CDATA $ 0.72\\sigma $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M16.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> and <inline-formula>\n<tex-math><?CDATA $ 2.11\\sigma $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M17.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>, respectively. In this case, the model is most favored by the data. Therefore, this cosmological model can greatly relieve the <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M18.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> tension and simultaneously effectively alleviate the <inline-formula>\n<tex-math><?CDATA $ S_8 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_5_051001_M19.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> tension.","PeriodicalId":10250,"journal":{"name":"中国物理C","volume":"52 1","pages":""},"PeriodicalIF":3.6000,"publicationDate":"2024-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"中国物理C","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1674-1137/ad2b52","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, NUCLEAR","Score":null,"Total":0}

引用次数: 0

Abstract

We consider a new cosmological model (called

CDM), in which the vacuum energy interacts with matter and radiation, and test this model using the current cosmological observations. Using the CMB+BAO+SN (CBS) dataset to constrain the model, we find that

and

tensions are relieved to

and

, respectively. However, in this case, the

CDM model is not favored by the data, compared with ΛCDM. We find that when the

and

data are added to the data combination, the situation is significantly improved. In the CBS+

case, the model relieves the

tension to

, and the model is favored over ΛCDM. In the CBS+

case, we obtain a synthetically best situation, in which the

and

tensions are relieved to

and

, respectively. In this case, the model is most favored by the data. Therefore, this cosmological model can greatly relieve the

tension and simultaneously effectively alleviate the

tension.

查看原文本刊更多论文

暗能量和物质相互作用情景缓解 H 0 和 S 8 张力* * 国家 SKA 计划（2022SKA0110200, 2022SKA0110203）和国家自然科学基金（11975072, 11875102, 11835009）资助

我们考虑了一个新的宇宙学模型（称为 CDM），在这个模型中，真空能量与物质和辐射相互作用，并利用当前的宇宙学观测数据对这个模型进行了检验。利用 CMB+BAO+SN （CBS）数据集对该模型进行约束，我们发现和的张力分别缓解了和。然而，在这种情况下，与ΛCDM相比，数据并不支持CDM模型。我们发现，当数据组合中加入和数据时，情况会得到明显改善。在 CBS+ 情形下，模型缓解了与 ΛCDM 的紧张关系，模型比 ΛCDM 更受青睐。在 CBS++ 情况下，我们得到了一个合成上的最佳情况，即张力和张力分别缓解到和。在这种情况下，该模型最受数据青睐。因此，这个宇宙学模型可以极大地缓解张力，同时有效地缓解张力。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

中国物理C 物理-物理：核物理

CiteScore

6.50

自引率

8.30%

发文量

8976

审稿时长

1.3 months

期刊介绍： Chinese Physics C covers the latest developments and achievements in the theory, experiment and applications of: Particle physics; Nuclear physics; Particle and nuclear astrophysics; Cosmology; Accelerator physics. The journal publishes original research papers, letters and reviews. The Letters section covers short reports on the latest important scientific results, published as quickly as possible. Such breakthrough research articles are a high priority for publication. The Editorial Board is composed of about fifty distinguished physicists, who are responsible for the review of submitted papers and who ensure the scientific quality of the journal. The journal has been awarded the Chinese Academy of Sciences ‘Excellent Journal’ award multiple times, and is recognized as one of China''s top one hundred key scientific periodicals by the General Administration of News and Publications.