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The network of cosmological tests is tight enough now to show that the relativistic Big Bang cosmology is a good approximation to what happened as the universe expanded and cooled through light element production and evolved to the present.…

宇宙学与河外天体物理 · 物理学 2017-03-29 P. J. E. Peebles

The expansion of our universe, when followed backward in time, implies that it emerged from a phase of huge density, the big bang. These stages are so extreme that classical general relativity combined with matter theories is not able to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Martin Bojowald

This article relates two topics of central importance in modern astronomy - the discovery some fifteen years ago of the first planets around other stars (exoplanets), and the centuries-old problem of understanding the origin of our own…

地球与行星天体物理 · 物理学 2011-11-08 Michael Perryman

We venture that the long evolution of science may be viewed as unfolding over three blurred epochs. The first epoch spans the slow, haphazard, error-ridden realization of scientific truths along with foundational scientific methods. The…

物理与社会 · 物理学 2025-11-04 Peter Sheridan Dodds

We review our current understanding of how the first galaxies formed at the end of the cosmic dark ages, a few 100 million years after the Big Bang. Modern large telescopes discovered galaxies at redshifts greater than seven, whereas…

宇宙学与河外天体物理 · 物理学 2015-05-27 Volker Bromm , Naoki Yoshida

The early phase of cosmic evolution is still a great topic of interest to the cosmologist community. Especially the mechanism behind the origin of the Universe is yet to be resolved. Most people believe in the Big Bang models (singular…

广义相对论与量子宇宙学 · 物理学 2023-08-17 Subhayan Maity , Sujayita Bakra

The elegance of inflationary cosmology and cosmological perturbation theory ends with the formation of the first stars and galaxies, the initial sources of light that launched the phenomenologically rich process of cosmic reionization. Here…

星系天体物理 · 物理学 2016-01-27 Milos Milosavljevic , Chalence Safranek-Shrader

In popular cosmological scenarios, some time beyond a redshift of 10, stars within protogalaxies created the first heavy elements; these systems, together perhaps with an early population of quasars, generated the ultraviolet radiation and…

天体物理学 · 物理学 2009-10-31 Piero Madau

Modern cosmological simulations predict that the first generation of stars formed with a mass scale around 100 solar masses about 300-400 million years after the Big Bang. When the first stars reached the end of their lives, many of them…

高能天体物理现象 · 物理学 2014-07-30 Ke-Jung Chen

The Dark Age is the period between the time when the cosmic microwave background was emitted and the time when the evolution of structure in the universe led to the gravitational collapse of objects in which the first stars were formed. The…

天体物理学 · 物理学 2009-11-10 Jordi Miralda-Escude

Since the beginning of the 20th century, a continuous evolution and perfection of what we today call the standard cosmological model has been produced, although some authors like to distinguish separate periods within this evolution. A…

物理学史与哲学 · 物理学 2023-08-02 Martin Lopez-Corredoira

Large telescopes have allowed astronomers to observe galaxies that formed as early as 850 million years after the Big Bang. We predict when the first star that astronomers can observe formed in the universe, accounting for the first time…

天体物理学 · 物理学 2009-11-11 Smadar Naoz , Shay Noter , Rennan Barkana

The `Little Bangs' made in particle collider experiments reproduce the conditions in the Big Bang when the age of the Universe was a fraction of a second. It is thought that matter was generated, the structures in the Universe were formed…

天体物理学 · 物理学 2009-09-11 John Ellis

While the generally recognized symmetries of cosmos are preserved, conservation laws for gravitational system are reconsidered and the Lagrangian density of pure gravitational field is revised. From these considerations, some of the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Fang-Pei Chen

Cosmology is nowadays going through a true revolution in the quantity and quality of observations that are capable of providing crucial information about the origin and evolution of the universe. In the first years of the next millenium we…

天体物理学 · 物理学 2015-06-24 Juan Garcia-Bellido

Stars and planets are the fundamental objects of the Universe. Their formation processes, though related, may differ in important ways. Stars almost certainly form from gravitational collapse and probably have formed this way since the…

地球与行星天体物理 · 物理学 2009-04-02 Alwyn Wootten , Bryan Butler , Antonio Hales , Stuartt Corder , Robert Brown , David Wilner

Gravity plays an important part in the experiments and discoveries of the modern world. But how was it discovered? Surely Newton and Einstein were not the only people to observe it and account for it. It had been a long path before the full…

科普物理 · 物理学 2020-12-01 Arshia Anjum , Sriman Srisa Saran Mishra

In order to account for the observable Universe, any comprehensive theory or model of cosmology must draw from many disciplines of physics, including gauge theories of strong and weak interactions, the hydrodynamics and microphysics of…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Peter Anninos

An impressive bulk of multiple astronomical observations indicates that there are plenty of objects in the universe with the age which cannot be explained by the conventional theory. A model is considered which successfully describes all…

宇宙学与河外天体物理 · 物理学 2014-10-28 A. D. Dolgov

These notes are intended as an introductory course for experimental particle physicists interested in the recent developments in astrophysics and cosmology. I will describe the standard Big Bang theory of the evolution of the universe, with…

高能物理 - 唯象学 · 物理学 2007-05-23 Juan Garcia-Bellido