{"title":"JWST 再电离危机所隐含的宇宙时间线","authors":"F. Melia","doi":"10.1051/0004-6361/202450835","DOIUrl":null,"url":null,"abstract":"JWST's discovery of well-formed galaxies and supermassive black holes only a \n few hundred Myr after the big bang, and the identification of polycyclic aromatic\n hydrocarbons (PAHs) at $z=6.71$, seriously challenge the timeline predicted by Lambda CDM. \n Moreover, the implied bright UV-irradiation of the early Universe suggests a reionization \n history much too short to comply with the observed evolution of the hydrogen ionization \n fraction, $x_ HII (z)$. A recent analysis of reionization after JWST by Munoz:2024 has concluded\n that the Lambda CDM timeline simply cannot accommodate the combined JWST- Planck observations even if exotic fixes are introduced to modify the standard reionization model.\n In this paper, we argue that this so-called `photon budget crisis' is more likely\n due to flaws in the cosmological model itself. We aim to re-analyze the data in the context\n of established astrophysics with $R_ h =ct$ as the background cosmology, an approach\n that has already been shown to mitigate the tension created by the too-early appearance \n of galaxies, quasars and PAHs. We employ the standard reionization model using the JWST-measured UV luminosity\n function in the early Universe and the timeline and physical conditions in both \n Lambda CDM and $R_ h =ct$. The former has already been fully probed and discussed \n by Munoz:2024 and we here merely redo the calculation to ensure consistency with \n their pioneering work. We then contrast the predicted reionization histories in these two \n scenarios and compare them with the data. We confirm that the reionization history predicted by Lambda CDM is in significant tension\n with the observations, and demonstrate that the latter are instead in excellent agreement with \n the $R_ h =ct$ timeline. Together, the four anomalies uncovered by JWST, including the newly discovered reionization\n `crisis' discussed in this paper, provide strong evidence against the timeline \n predicted by Lambda CDM and in favor of the evolutionary history in $R_ h =ct$.","PeriodicalId":505693,"journal":{"name":"Astronomy & Astrophysics","volume":"72 7","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-06-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The Cosmic Timeline Implied by the JWST Reionization Crisis\",\"authors\":\"F. 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We aim to re-analyze the data in the context\\n of established astrophysics with $R_ h =ct$ as the background cosmology, an approach\\n that has already been shown to mitigate the tension created by the too-early appearance \\n of galaxies, quasars and PAHs. We employ the standard reionization model using the JWST-measured UV luminosity\\n function in the early Universe and the timeline and physical conditions in both \\n Lambda CDM and $R_ h =ct$. The former has already been fully probed and discussed \\n by Munoz:2024 and we here merely redo the calculation to ensure consistency with \\n their pioneering work. We then contrast the predicted reionization histories in these two \\n scenarios and compare them with the data. We confirm that the reionization history predicted by Lambda CDM is in significant tension\\n with the observations, and demonstrate that the latter are instead in excellent agreement with \\n the $R_ h =ct$ timeline. 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引用次数: 0
摘要
JWST 在大爆炸后仅几百 Myr 就发现了形态良好的星系和超大质量黑洞,并在 $z=6.71$ 发现了多环芳烃(PAHs),这严重挑战了 Lambda CDM 预测的时间轴。 此外,早期宇宙中隐含的明亮紫外线辐照表明其再电离历史太短,不符合观测到的氢离子化分数($x_ HII (z)$)的演变。穆诺兹(Munoz:2024)最近对JWST之后的再电离现象进行了分析,得出结论认为,即使引入奇异的修正来修改标准再电离模型,Lambda CDM时间轴也根本无法适应JWST-普朗克的联合观测结果。在本文中,我们认为这种所谓的 "光子预算危机 "更可能是由于宇宙学模型本身的缺陷造成的。我们的目的是在以$R_ h =ct$ 为背景宇宙学的既定天体物理学背景下重新分析数据,这种方法已经被证明可以缓解星系、类星体和多环芳香烃过早出现所造成的紧张局势。我们采用标准再电离模型,利用 JWST 测得的早期宇宙紫外线光度函数以及 Lambda CDM 和 $R_ h =ct$ 的时间轴和物理条件。前者已经由Munoz:2024进行了充分的探测和讨论,我们在这里只是重新做了计算,以确保与他们的开创性工作保持一致。然后,我们对比这两种情况下预测的再电离历史,并与数据进行比较。我们证实,Lambda CDM 预测的再电离历史与观测结果有很大的矛盾,并证明后者与 $R_ h =ct$ 时间线非常吻合。JWST发现的四个异常现象,包括本文讨论的新发现的再电离 "危机",共同提供了强有力的证据,反驳了Lambda CDM预测的时间线,支持R_ h =ct$的演化历史。
The Cosmic Timeline Implied by the JWST Reionization Crisis
JWST's discovery of well-formed galaxies and supermassive black holes only a
few hundred Myr after the big bang, and the identification of polycyclic aromatic
hydrocarbons (PAHs) at $z=6.71$, seriously challenge the timeline predicted by Lambda CDM.
Moreover, the implied bright UV-irradiation of the early Universe suggests a reionization
history much too short to comply with the observed evolution of the hydrogen ionization
fraction, $x_ HII (z)$. A recent analysis of reionization after JWST by Munoz:2024 has concluded
that the Lambda CDM timeline simply cannot accommodate the combined JWST- Planck observations even if exotic fixes are introduced to modify the standard reionization model.
In this paper, we argue that this so-called `photon budget crisis' is more likely
due to flaws in the cosmological model itself. We aim to re-analyze the data in the context
of established astrophysics with $R_ h =ct$ as the background cosmology, an approach
that has already been shown to mitigate the tension created by the too-early appearance
of galaxies, quasars and PAHs. We employ the standard reionization model using the JWST-measured UV luminosity
function in the early Universe and the timeline and physical conditions in both
Lambda CDM and $R_ h =ct$. The former has already been fully probed and discussed
by Munoz:2024 and we here merely redo the calculation to ensure consistency with
their pioneering work. We then contrast the predicted reionization histories in these two
scenarios and compare them with the data. We confirm that the reionization history predicted by Lambda CDM is in significant tension
with the observations, and demonstrate that the latter are instead in excellent agreement with
the $R_ h =ct$ timeline. Together, the four anomalies uncovered by JWST, including the newly discovered reionization
`crisis' discussed in this paper, provide strong evidence against the timeline
predicted by Lambda CDM and in favor of the evolutionary history in $R_ h =ct$.