Issues

 / 

2020

 / 

June

  

Methodological notes


Generalization of the k coefficient method in relativity to an arbitrary angle between the velocity of an observer (source) and the direction of the light ray from (to) a faraway source (observer) at rest


Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation

The $k$ coefficient method proposed by H Bondi is extended to a general case when the angle $\alpha$ between the velocity of a signal from a distant source at rest and the velocity of an observer does not coincide with 0 or $\pi$, as considered by Bondi, but takes an arbitrary value in the interval $0\le \alpha \le \pi$, and to the opposite case, when the source is moving and the observer is at rest, while the angle $\alpha$ between the source velocity and the direction of the signal to the observer takes any value between 0 and $\pi $. Functions $k_*(\beta,\alpha)$ and $k_+(\beta,\alpha)$ of the angle and relative velocity are introduced for the ratio $\omega /\omega^{'}$ of proper frequencies of the source and observer. Their explicit expressions are obtained from the condition of the invariance of the ray beam coherence in passing from the source frame to that of the observer without using the Lorentz transform. Owing to the analyticity of these functions in $\alpha$, the ratio of frequencies in the cases mentioned is given by the formulas $\omega /\omega ^{'}=k_*(\beta,\alpha)$ and $\omega /\omega^{'}=k_+(\beta,\pi -\alpha )\equiv 1/k_*(\beta,\alpha)$, which coincide with those for the Doppler effect, in which the angle $\alpha$, velocity $\beta$, and one of the frequencies are measured in a rest reference frame. A ray emitted by the source at angle $\alpha$ to the observer velocity in the source frame is directed at the angle $\alpha^{'}$ to the same velocity in the observer frame. Owing to light aberration, the angles $\alpha$ and $\alpha^{'}$ are functionally related through $k_*(\beta,\alpha)=k_+(\beta,\alpha^{'})$. The functions $\alpha^{'}(\alpha,\beta)$ and $\alpha (\alpha ^{'},\beta)$ are expressed as antiderivatives of the functions $k_*(\beta,\alpha)$ and $k_*(\beta,\pi -\alpha ^{'})$. The analyticity of functions $k_*(\beta, z)$ and $k_+(\beta, z)$ in $z\equiv \alpha$ in the interval $0\le z\le \pi $ is continued into the entire plane of complex $z$, where $k_*$ has poles at $z^\pm _n=2\pi n\mp \rm i \ln \cos \alpha _1$ (see (17)), and $k_+$ has zeros in the same points shifted by $\pi$. The spatiotemporal asymmetry of the Doppler and light aberration effects is explained by the closeness of these singularities to the real axis.

Typically, an English fulltext is available in about 3 months from the date of publication of the original article.

Keywords: special relativity theory, invariance of coherence, invariance of phase, Doppler effect, aberration of light, analyticity in angle, conjugate poles and aberration scale
PACS: 03.30.+p, 42.15.Fr (all)
DOI: 10.3367/UFNe.2019.12.038703
URL: https://ufn.ru/en/articles/2020/6/e/
Citation: Ritus V I "Generalization of the k coefficient method in relativity to an arbitrary angle between the velocity of an observer (source) and the direction of the light ray from (to) a faraway source (observer) at rest" Phys. Usp. 63 601–610 (2020)
BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks

Received: 1st, July 2019, revised: 30th, October 2019, 3rd, December 2019

Оригинал: Ритус В И «Обобщение метода коэффициента k в теории относительности на произвольный угол между скоростью наблюдателя (источника) и направлением луча света от далёкого неподвижного источника (к далёкому неподвижному наблюдателю)» УФН 190 648–657 (2020); DOI: 10.3367/UFNr.2019.12.038703

© 1918–2020 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions