Published March 24, 2014
| Version v1
Journal article
Dynamical interaction between astrophysical systems and dark substructure
- 1. Instituto de Ciencias Nucleares, UNAM, Apartado Postal 70-543, 04510, Ciudad Universitaria, D.F. (Mexico)
- 2. Instituto de Astronomia, UNAM, Apartado Postal 70-264, 04510, Ciudad Universitaria, D.F. (Mexico)
- 3. Instituto de Astronomia, UNAM, Apartado Postal 877, 22860 Ensenada, B.C. (Mexico)
Description
We explore the possibility to constrain the dark matter (DM) sub–structure properties, mass and distribution, at sub–galactic scales, by considering the dynamics of some astrophysical system under the dynamical influence of such sub–structure. We present preliminary results discussing the sensitivity of the Solar System dynamics, and dSphs wide binaries abundance, to the small scale DM distribution
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/485/1/012021Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 485
- Journal Issue
- 1
- Journal Page Range
- [6 p.]
- ISSN
- 1742-6596
Conference
- Title
- 18. international symposium on particles strings and cosmology
- Acronym
- PASCOS 2012
- Dates
- 3-8 Jun 2012
- Place
- Merida (Mexico)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 46073588
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; BINARY STARS; MASS; NONLUMINOUS MATTER; SENSITIVITY; SOLAR SYSTEM
- Descriptors DEC
- MATTER; PHYSICS; STARS