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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.
Chinese Physics B is devoted to rapid publication of original research papers, rapid communications, and reviews on the latest developments and achievements in all branches of physics worldwide except nuclear physics, as well as the physics of elementary particles and fields.
Acta Physica may refer to several scientific journals of physics: Acta Physica Hungarica; Acta Physica Polonica; See also. Helvetica Physica Acta
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 ...
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.
Acta Mathematicae Applicatae Sinica (English series) is a peer-reviewed mathematics journal published quarterly by Springer. Established in 1984 by the Chinese Mathematical Society, the journal publishes articles on applied mathematics. According to the Journal Citation Reports, the journal had a 2020 impact factor of 1.102. [1]
Weinberg angle θ W, and relation between couplings g, g ′, and e = g sin θ W. Adapted from Lee (1981). [1] The pattern of weak isospin, T 3, and weak hypercharge, Y W, of the known elementary particles, showing electric charge, Q, [a] along the Weinberg angle. The neutral Higgs field (upper left, circled) breaks the electroweak symmetry and ...
Tau Ceti, Latinized from τ Ceti, is a single star in the constellation Cetus that is spectrally similar to the Sun, although it has only about 78% of the Sun's mass.At a distance of just under 12 light-years (3.7 parsecs) from the Solar System, it is a relatively nearby star and the closest solitary G-class star.