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新研究将宇宙年龄加倍至 267 亿年

新研究将宇宙年龄加倍至 267 亿年

一项新的研究表明,宇宙的年龄可能有 267 亿年,几乎是广泛接受的 137 亿年年龄的两倍。 新模型结合了兹威基的疲倦光理论和不断演变的狄拉克耦合常数,可以解释大爆炸后仅 3 亿年形成的年轻成熟星系的存在,并提出对宇宙学常数的修订解释。

一项新的研究表明,宇宙可能有 267 亿年的历史,挑战了基于 Lambda-CDM 一致性模型的广泛接受的 137 亿年的估计。

一项新的研究挑战了现行的宇宙学模型,并为所谓的“不可能的早期星系问题”提供了新的线索,根据这项研究,我们的宇宙可能比目前估计的年龄要老一倍。

作者、渥太华大学理学院物理学副教授拉金德拉·古普塔 (Rajendra Gupta) 说道。

拉金德拉·古普塔

“我们新设计的模型将星系的形成时间延长了数十亿年,使宇宙的年龄达到了 267 亿岁,而不是之前估计的 13.7 岁。” Rajendra Gupta – 渥太华大学理学院物理学助理教授。 图片来源:渥太华大学

多年来,天文学家和物理学家一直通过测量自诞生以来所经过的时间来计算宇宙的年龄。[{” attribute=””>Big Bang and by studying the oldest stars based on the redshift of light coming from distant galaxies. In 2021, thanks to new techniques and advances in technology, the age of our universe was thus estimated at 13.797 billion years using the Lambda-CDM concordance model.

However, many scientists have been puzzled by the existence of stars like the Methuselah that appear to be older than the estimated age of our universe and by the discovery of early galaxies in an advanced state of evolution made possible by the James Webb Space Telescope. These galaxies, existing a mere 300 million years or so after the Big Bang, appear to have a level of maturity and mass typically associated with billions of years of cosmic evolution. Furthermore, they’re surprisingly small in size, adding another layer of mystery to the equation.

Zwicky’s tired light theory proposes that the redshift of light from distant galaxies is due to the gradual loss of energy by photons over vast cosmic distances. However, it was seen to conflict with observations. Yet Gupta found that “by allowing this theory to coexist with the expanding universe, it becomes possible to reinterpret the redshift as a hybrid phenomenon, rather than purely due to expansion.”

“Our newly-devised model stretches the galaxy formation time by several billion years, making the universe 26.7 billion years old, and not 13.7 as previously estimated.”

Rajendra Gupta, Adjunct professor of physics in the Faculty of Science at the University of Ottawa

In addition to Zwicky’s tired light theory, Gupta introduces the idea of evolving “coupling constants,” as hypothesized by Paul Dirac. Coupling constants are fundamental physical constants that govern the interactions between particles. According to Dirac, these constants might have varied over time. By allowing them to evolve, the timeframe for the formation of early galaxies observed by the Webb telescope at high redshifts can be extended from a few hundred million years to several billion years. This provides a more feasible explanation for the advanced level of development and mass observed in these ancient galaxies.

Moreover, Gupta suggests that the traditional interpretation of the “cosmological constant,” which represents dark energy responsible for the accelerating expansion of the universe, needs revision. Instead, he proposes a constant that accounts for the evolution of the coupling constants. This modification in the cosmological model helps address the puzzle of small galaxy sizes observed in the early universe, allowing for more accurate observations.

On July 7, 2023, the study, “JWST early Universe observations and 𝚲CDM cosmology,” was published in the Monthly Notices of the Royal Astronomical Society (MNRAS) by Oxford University Press.

Reference: “JWST early Universe observations and ΛCDM cosmology” by R Gupta, 7 July 2023, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stad2032

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