Unfortunately, a lot of the field theory surrounding CDM is speculative at the moment. One of the possibilities is that the dark matter particle is the lightest supersymmetric particle, so reading up on supersymmetry may be helpful for seeing one possible theory that might potentially include the dark matter particle. Just bear in mind that there are many other possibilities. Hopefully future dark matter searches or the LHC will provide further insight (the LHC is unlikely to detect the dark matter particle itself, but it may detect other high-energy particles that could give us a hint in what theory is correct at higher energies, which would tell us what framework we should use to try to understand dark matter).xn_axe said:Hi Guys,
Can anyone provide links, books which explain the mathematical background of the field theory that explains the current accepted ^CDM model of the universe?
Thanks
Adarsh
Cold dark matter (CDM) is a type of hypothetical matter that is believed to make up a large portion of the total matter in the universe. It is called "cold" because it moves at relatively slow speeds and "dark" because it does not emit or absorb light, making it difficult to detect directly.
Mathematical analysis is crucial in understanding the properties and behavior of CDM. It allows scientists to develop models and simulations that can help explain the distribution and dynamics of CDM in the universe. It also helps in predicting and interpreting observations of CDM in astrophysical systems.
Some of the most widely accepted theories and models for CDM include the Cold Dark Matter (CDM) model, the Warm Dark Matter (WDM) model, and the Self-Interacting Dark Matter (SIDM) model. These models differ in their assumptions about the nature and properties of CDM, and have been tested against observations from various astrophysical systems.
CDM is thought to play a major role in the formation of structures in the universe, such as galaxies, galaxy clusters, and large-scale structures. This is because CDM is believed to interact mainly through gravitational forces, which can cause it to clump together and form the basis for the growth of structures over time.
One major challenge in studying CDM using mathematical analysis is the lack of direct detection of CDM particles. This makes it difficult to confirm the validity of different models and theories. Additionally, there is still much to be understood about the properties and behavior of CDM, which can make it challenging to accurately model and simulate its effects on the universe.