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Acta Physica Sinica (abbreviation: Acta. Phys. Sin., or also APS) is a peer-reviewed scientific journal in the fields of physics published by the Chinese Physical Society. Established in 1933 as Chinese Journal of Physics , the journal was published in English, French and German at first.
The journal was established in 1992 as Acta Physica Sinica (Overseas Edition), publishing papers different from those of "Acta Physica Sinica" (in Chinese) in both language and content. The journal title was changed to Chinese Physics in 2000, and changed to Chinese Physics B in 2008.
Acta Physica may refer to several scientific journals of physics: Acta Physica Hungarica; Acta Physica Polonica;
Acta Physica Polonica was established by the Polish Physical Society in 1920. In 1970 it was split into Acta Physica Polonica A (published by the Institute of Physics of the Polish Academy of Sciences), whose scope includes general physics, atomic and molecular physics, condensed matter physics, optics and quantum optics, biophysics, quantum information, and applied physics, and Acta Physica ...
The weak mixing angle or Weinberg angle [2] is a parameter in the Weinberg–Salam theory of the electroweak interaction, part of the Standard Model of particle physics, and is usually denoted as θ W. It is the angle by which spontaneous symmetry breaking rotates the original W 0 and B 0 vector boson plane, producing as a result the Z 0
' Annals of Chemistry and Physics ') is a scientific journal founded in Paris, France, in 1789 under the title Annales de chimie. One of the early editors was the French chemist Antoine Lavoisier . Lavoisier, an aristocrat, was guillotined in May 1794, ostensibly for tax fraud: and the journal was not published from 1794 to 1796 while the Reign ...
Acta Mathematica Sinica (English series) is a peer-reviewed mathematics journal published quarterly by Springer.Founded in 1936 and split into a Chinese series and an English series in 1985, the journal publishes articles on all areas of mathematics, and allows submissions from researchers of all nationalities.
TOI-4603 b is a gas giant exoplanet orbiting HD 245134, a F-type subgiant star located 731 light-years away, in the constellation of Taurus. [ 3 ] [ note 1 ] It orbits its host star at a distance of 0.0888 astronomical units (13,280,000 km), completing one orbit every 7 days around it. [ 2 ]