Special Issue on Dark Matter and Dark Energy
In cosmology, dark matter is something that can’t be directly detected,
that is, it does not interact with electromagnetic force. It may be a major
component of the universe, but it does not belong to any known substance of
visible celestial bodies. The most powerful evidence for the existence of dark
matter is two points: one is the problem of Galaxy rotation, the other is the
gravitational lensing effect. In short, dark energy comes from the fact that
the universe accelerates expansion. The influence of dark matter is expressed
in individual galaxies, while dark energy acts only on the entire cosmic scale.
The theory of dark matter has been widely recognized by astronomy and
cosmology, but the study of dark energy is still in its infancy. The study of
dark matter and dark energy has opened up a new world for physics and
astronomy.
In this special issue, we intend to invite front-line
researchers and authors to submit original researches and review articles on
exploring Dark Matter and Dark Energy.
Potential topics include, but are not limited to:
-
Big tear theory
-
Origin of dark
matter and dark energy
-
Formation of
dark matter and dark energy
-
Detection of
dark matter and dark energy
-
Dark energy
model
-
Material
movement and space-time structure
-
The future evolution
of the universe
-
The composition
of dark matter and dark energy
Authors should read over the journal’s For Authors carefully before submission. Prospective
authors should submit an electronic copy of their complete manuscript through
the journal’s Paper Submission System.
Please kindly notice that the “Special Issue”
under your manuscript title is supposed to be specified and the research field
“Special Issue – Dark Matter and Dark
Energy” should be chosen during your submission.
According to the
following timetable:
Submission Deadline
|
September 13th, 2018
|
Publication Date
|
November 2018
|
Guest Editor:
For
further questions or inquiries
Please
contact Editorial Assistant at
jmp@scirp.org