The weak turbulence methods in the problem of galaxy mass distribution function
The analogy between the turbulent Kolmogorov type spectra and the distribution of galaxies on masses is discussed. Due to nonlocality [1] of galaxy mass spectrum formed by merging the additional approximate conservation law affects its intermediate asymptotics power index, which proves to be interve...
Gespeichert in:
| Veröffentlicht in: | Вопросы атомной науки и техники |
|---|---|
| Datum: | 2000 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
2000
|
| Schlagworte: | |
| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/78551 |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | The weak turbulence methods in the problem of galaxy mass distribution function / V.M. Kontorovich // Вопросы атомной науки и техники. — 2000. — № 6. — С. 84-87. — Бібліогр.: 18 назв. — англ. |
Institution
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-78551 |
|---|---|
| record_format |
dspace |
| spelling |
Kontorovich, V.M. 2015-03-18T19:01:44Z 2015-03-18T19:01:44Z 2000 The weak turbulence methods in the problem of galaxy mass distribution function / V.M. Kontorovich // Вопросы атомной науки и техники. — 2000. — № 6. — С. 84-87. — Бібліогр.: 18 назв. — англ. 1562-6016 https://nasplib.isofts.kiev.ua/handle/123456789/78551 533.9 The analogy between the turbulent Kolmogorov type spectra and the distribution of galaxies on masses is discussed. Due to nonlocality [1] of galaxy mass spectrum formed by merging the additional approximate conservation law affects its intermediate asymptotics power index, which proves to be intervening between the constant mass flux and this of the number of massive galaxies. Analytical description of this asymptotics, which essentially uses the Smoluchowsky kinetic equation symmetry transformation, is presented. The result is compared with the recently discovered steepness of galaxy luminosity function on its faint edge. The problem of the main part of barionic mass in the Universe is shortly discussed in this context. en Національний науковий центр «Харківський фізико-технічний інститут» НАН України Вопросы атомной науки и техники Plasma dynamics and plasma-wall interaction The weak turbulence methods in the problem of galaxy mass distribution function Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
The weak turbulence methods in the problem of galaxy mass distribution function |
| spellingShingle |
The weak turbulence methods in the problem of galaxy mass distribution function Kontorovich, V.M. Plasma dynamics and plasma-wall interaction |
| title_short |
The weak turbulence methods in the problem of galaxy mass distribution function |
| title_full |
The weak turbulence methods in the problem of galaxy mass distribution function |
| title_fullStr |
The weak turbulence methods in the problem of galaxy mass distribution function |
| title_full_unstemmed |
The weak turbulence methods in the problem of galaxy mass distribution function |
| title_sort |
weak turbulence methods in the problem of galaxy mass distribution function |
| author |
Kontorovich, V.M. |
| author_facet |
Kontorovich, V.M. |
| topic |
Plasma dynamics and plasma-wall interaction |
| topic_facet |
Plasma dynamics and plasma-wall interaction |
| publishDate |
2000 |
| language |
English |
| container_title |
Вопросы атомной науки и техники |
| publisher |
Національний науковий центр «Харківський фізико-технічний інститут» НАН України |
| format |
Article |
| description |
The analogy between the turbulent Kolmogorov type spectra and the distribution of galaxies on masses is discussed. Due to nonlocality [1] of galaxy mass spectrum formed by merging the additional approximate conservation law affects its intermediate asymptotics power index, which proves to be intervening between the constant mass flux and this of the number of massive galaxies. Analytical description of this asymptotics, which essentially uses the Smoluchowsky kinetic equation symmetry transformation, is presented. The result is compared with the recently discovered steepness of galaxy luminosity function on its faint edge. The problem of the main part of barionic mass in the Universe is shortly discussed in this context.
|
| issn |
1562-6016 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/78551 |
| citation_txt |
The weak turbulence methods in the problem of galaxy mass distribution function / V.M. Kontorovich // Вопросы атомной науки и техники. — 2000. — № 6. — С. 84-87. — Бібліогр.: 18 назв. — англ. |
| work_keys_str_mv |
AT kontorovichvm theweakturbulencemethodsintheproblemofgalaxymassdistributionfunction AT kontorovichvm weakturbulencemethodsintheproblemofgalaxymassdistributionfunction |
| first_indexed |
2025-12-07T20:04:27Z |
| last_indexed |
2025-12-07T20:04:27Z |
| _version_ |
1850881204181532672 |