Cosmology on small scales 2018

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985840%3A_____%2F18%3A00500747" target="_blank" >RIV/67985840:_____/18:00500747 - isvavai.cz</a>

Result on the web

—

DOI - Digital Object Identifier

—

Result language

angličtina

Original language name

Cosmology on small scales 2018

Original language description

In the early twenties of the last century, Alexander A. Friedmann (1888-1925) derived from the system of ten Einstein's equations applied to a perfectly symmetric universe, which is homogeneous and isotropic for every fixed time instant, a nonlinear differential equation for the expansion rate of the universe. The question is whether one can perform such excessive extrapolations, i.e. to apply Einstein's equations to galactic or cosmological scales. The current standard model of cosmology is based on the normalized Friedmann equation which contains, as major parameters, densities of dark matter and dark energy. So, it is timely to gather specialists from different disciplines, including galaxy evolution and planetology, to discuss the problem of existence of dark matter and dark energy at various scales, both from theoretical and observational points of view.

Czech name

—

Czech description

—

Type

M - Conference organization

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

—

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Event location

Prague

Event country

CZ - CZECH REPUBLIC

Event starting date

—

Event ending date

—

Total number of attendees

75

Foreign attendee count

50

Type of event by attendee nationality

WRD - Celosvětová akce