Mathematics
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cemec..24..407b&link_type=abstract
Celestial Mechanics, vol. 24, Aug. 1981, p. 407-429.
Mathematics
10
Binary Stars, Stellar Evolution, Stellar Mass Ejection, Two Body Problem, Differential Equations, Symmetry, Transformations (Mathematics), Variational Principles
Scientific paper
The classical non-stationary two-body Gylden-Mescerskii (Gylden 1889, Mescerskii 1893) problem for describing double-star evolution with secular mass loss due to photon and corpuscular activity is investigated using differential equation transformation methods. The possible mass variation laws for reducing the equation to an autonomous form by transformation are given. Symmetry properties are also investigated and integrable cases from the group point of view are reviewed. Finite transformation groups permitting the division of the problem of intergrating the equation into noncrossing classes in accordance with mass variation laws are constructed. Finally, it is intended that the use of the mass variation laws should allow a physically realizable picture of the motion.
No associations
LandOfFree
Gylden-Mescerskii problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gylden-Mescerskii problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gylden-Mescerskii problem will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1745278