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The Snowmass Process is a particle physics community planning exercise sponsored by the Division of Particles and Fields of the American Physical Society. [1] During this process, scientists develop a collective vision for the next seven to ten years for particle physics research in the US.
This is a documentation subpage for Template:Physical cosmology. It may contain usage information, categories and other content that is not part of the original template page. Part of a series on
In modern physical cosmology, the cosmological principle is the notion that the spatial distribution of matter in the universe is uniformly isotropic and homogeneous when viewed on a large enough scale, since the forces are expected to act equally throughout the universe on a large scale, and should, therefore, produce no observable inequalities in the large-scale structuring over the course ...
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A cosmological phase transition is an overall change in the state of matter across the whole universe. The success of the Big Bang model led researchers to conjecture possible cosmological phase transitions taking place in the very early universe, at a time when it was much hotter and denser than today.
Change the Isaac Newton coat of arms from a obvious fake vector image to an image of the one on that was set in stone at the Woolsthorpe Manor, a much more creditable source 216.100.89.25 18:52, 25 January 2021 (UTC) Not done: this is the talk page for discussing improvements to the template {{Physical cosmology}}. Please make your request at ...
Meteorites are often studied as part of cosmochemistry. Cosmochemistry (from Ancient Greek κόσμος (kósmos) 'universe' and χημεία (khēmeía) 'chemistry') or chemical cosmology is the study of the chemical composition of matter in the universe and the processes that led to those compositions. [1]
This List of Cosmological Computation Software catalogs the tools and programs used by scientists in cosmological research.. In the past few decades, the accelerating technological evolution has profoundly enhanced astronomical instrumentation, enabling more precise observations and expanding the breadth and depth of data collection by several orders of magnitude.