Abstract
We consider the three-dimensional stationary Vlasov-Poisson system of equations with respect to the distribution function of the gravitating matter f = f(q)(r, u), the local density rho = rho(r) , and the Newtonian potential, U = U(r), where r: = vertical bar x vertical bar, u : vertical bar v vertical bar ((x, v) is an element of R-3 x R-3 are the space-velocity coordinates), and f is a function q of the local energy E: = u(r) + u(2)/2. For a given function p = p(r), we obtain sufficient conditions for p to be "extendable." This means that there exists a stationary spherically symmetric solution (f(q), rho, U) of the Vlasov-Poisson system depending on the local energy E such that rho=p.
Dokumententyp: | Zeitschriftenartikel |
---|---|
Fakultät: | Mathematik, Informatik und Statistik > Mathematik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 510 Mathematik |
ISSN: | 1064-5624 |
Sprache: | Englisch |
Dokumenten ID: | 88955 |
Datum der Veröffentlichung auf Open Access LMU: | 25. Jan. 2022, 09:28 |
Letzte Änderungen: | 13. Aug. 2024, 12:44 |