Controlled ensemble null tests of dynamical dark energy hints: single-probe recovery of \(\Lambda \)CDM with BAO, compressed-CMB, and SNe mocks

IF 4.9 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Seokcheon Lee
{"title":"Controlled ensemble null tests of dynamical dark energy hints: single-probe recovery of \\(\\Lambda \\)CDM with BAO, compressed-CMB, and SNe mocks","authors":"Seokcheon Lee","doi":"10.1140/epjc/s10052-026-16374-9","DOIUrl":null,"url":null,"abstract":"<div><p>Recent combined cosmological analyses have reported mild apparent departures from the cosmological-constant equation of state. Such departures are difficult to interpret because BAO, compressed CMB distance priors, and Type Ia supernovae constrain different projections of the expansion history and carry different calibration degeneracies. We perform controlled ensemble null tests using observable-level Gaussian BAO-like, CMB-like, and supernova-like mock datasets generated from a common fiducial flat <span>\\(\\Lambda \\)</span>CDM cosmology. The aim is to determine whether each constituent single-probe likelihood block can produce an apparent DDE-like marginalized-posterior displacement, or spuriously exclude the fiducial model, through its own degeneracy structure and calibration freedom. The analysis adopts probe-adapted parameterizations for the BAO scale, the CMB physical matter density, and the supernova normalization degeneracy. With explicit convergence diagnostics, percentile-based posterior coverage tests, and realization-level pull statistics, none of the three single-probe analyses spuriously excludes the fiducial input at the 95% level. All completed BAO and SNe chains enter their final ensembles after adaptive extension of the originally rejected runs; for compressed CMB, a mock-data-space audit finds no detectable selection dependence within the sensitivity of the 208-mock ensemble. The compressed CMB-only likelihood nevertheless exhibits stable displaced marginalized medians together with broad late-time posterior intervals, illustrating that posterior location and model exclusion are distinct diagnostics. These results show that a displaced marginalized posterior in a single realization is not, by itself, evidence for dynamical dark energy. Such shifts must be interpreted through mock-ensemble recovery, convergence diagnostics, and the probe-dependent geometry of the likelihood.\n</p></div>","PeriodicalId":788,"journal":{"name":"The European Physical Journal C","volume":"86 10","pages":""},"PeriodicalIF":4.9000,"publicationDate":"2026-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjc/s10052-026-16374-9.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The European Physical Journal C","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1140/epjc/s10052-026-16374-9","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0

Abstract

Recent combined cosmological analyses have reported mild apparent departures from the cosmological-constant equation of state. Such departures are difficult to interpret because BAO, compressed CMB distance priors, and Type Ia supernovae constrain different projections of the expansion history and carry different calibration degeneracies. We perform controlled ensemble null tests using observable-level Gaussian BAO-like, CMB-like, and supernova-like mock datasets generated from a common fiducial flat \(\Lambda \)CDM cosmology. The aim is to determine whether each constituent single-probe likelihood block can produce an apparent DDE-like marginalized-posterior displacement, or spuriously exclude the fiducial model, through its own degeneracy structure and calibration freedom. The analysis adopts probe-adapted parameterizations for the BAO scale, the CMB physical matter density, and the supernova normalization degeneracy. With explicit convergence diagnostics, percentile-based posterior coverage tests, and realization-level pull statistics, none of the three single-probe analyses spuriously excludes the fiducial input at the 95% level. All completed BAO and SNe chains enter their final ensembles after adaptive extension of the originally rejected runs; for compressed CMB, a mock-data-space audit finds no detectable selection dependence within the sensitivity of the 208-mock ensemble. The compressed CMB-only likelihood nevertheless exhibits stable displaced marginalized medians together with broad late-time posterior intervals, illustrating that posterior location and model exclusion are distinct diagnostics. These results show that a displaced marginalized posterior in a single realization is not, by itself, evidence for dynamical dark energy. Such shifts must be interpreted through mock-ensemble recovery, convergence diagnostics, and the probe-dependent geometry of the likelihood.

动态暗能量提示的受控系综无效检验:利用BAO、压缩cmb和SNe模拟单探针恢复\(\Lambda \) CDM
最近的综合宇宙学分析报告了轻微的明显偏离宇宙常数状态方程。这种偏离很难解释,因为BAO、压缩的CMB距离先验和Ia型超新星约束了膨胀历史的不同投影,并携带了不同的校准简并。我们使用可观测水平的高斯类bao、类cmb和类超新星模拟数据集进行了受控的集合零检验,这些模拟数据集来自一个共同的基准平面\(\Lambda \) CDM宇宙学。目的是确定每个组成单探针似然块是否可以通过其自身的简并结构和校准自由度产生明显的dde样的边缘化后验位移,或者虚假地排除基准模型。对BAO尺度、CMB物理物质密度和超新星归一化简并度采用探针适应的参数化分析。通过明确的收敛诊断,基于百分位数的后验覆盖率测试和实现水平的拉统计,三个单探针分析都没有虚假地排除95的基准输入% level. All completed BAO and SNe chains enter their final ensembles after adaptive extension of the originally rejected runs; for compressed CMB, a mock-data-space audit finds no detectable selection dependence within the sensitivity of the 208-mock ensemble. The compressed CMB-only likelihood nevertheless exhibits stable displaced marginalized medians together with broad late-time posterior intervals, illustrating that posterior location and model exclusion are distinct diagnostics. These results show that a displaced marginalized posterior in a single realization is not, by itself, evidence for dynamical dark energy. Such shifts must be interpreted through mock-ensemble recovery, convergence diagnostics, and the probe-dependent geometry of the likelihood.
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
The European Physical Journal C
The European Physical Journal C 物理-物理:粒子与场物理
CiteScore
8.10
自引率
15.90%
发文量
1008
审稿时长
2-4 weeks
期刊介绍: Experimental Physics I: Accelerator Based High-Energy Physics Hadron and lepton collider physics Lepton-nucleon scattering High-energy nuclear reactions Standard model precision tests Search for new physics beyond the standard model Heavy flavour physics Neutrino properties Particle detector developments Computational methods and analysis tools Experimental Physics II: Astroparticle Physics Dark matter searches High-energy cosmic rays Double beta decay Long baseline neutrino experiments Neutrino astronomy Axions and other weakly interacting light particles Gravitational waves and observational cosmology Particle detector developments Computational methods and analysis tools Theoretical Physics I: Phenomenology of the Standard Model and Beyond Electroweak interactions Quantum chromo dynamics Heavy quark physics and quark flavour mixing Neutrino physics Phenomenology of astro- and cosmoparticle physics Meson spectroscopy and non-perturbative QCD Low-energy effective field theories Lattice field theory High temperature QCD and heavy ion physics Phenomenology of supersymmetric extensions of the SM Phenomenology of non-supersymmetric extensions of the SM Model building and alternative models of electroweak symmetry breaking Flavour physics beyond the SM Computational algorithms and tools...etc.
×
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:604180095
Book学术官方微信
小红书