AbstractWe present new fast numerical simulations of cosmic microwave background and large scale structure in the case in which the cosmological dark matter is made entirely or partly made of mirror matter. We consider scalar adiabatic primordial perturbations at linear scales in a flat Universe. The speed of the simulations allows us for the first time to use Markov Chain Monte Carlo analyses to constrain the mirror parameters. A Universe with pure mirror matter can fit very well the observations, equivalently to the case of an admixture with cold dark matter. In both cases, the cosmological models estimate the presence of a consistent amount of mirror dark matter, 0.06≲Ωmirrorh2≲0.12
AbstractMirror world, a parallel hidden sector with microphysics identical to ordinary particle phys...
We study a two-parameter extension of the cosmological standard model ΛCDM in which cold dark matter...
A new and inexpensive technique for detecting self interacting dark matter in the form of small grai...
We present new fast numerical simulations of cosmic microwave background and large scale structure i...
AbstractWe present new fast numerical simulations of cosmic microwave background and large scale str...
AbstractMirror dark matter interacting with ordinary matter via photon-mirror photon kinetic mixing ...
AbstractMirror dark matter provides a simple framework for which to explain the DAMA/LIBRA annual mo...
Mirror matter is predicted to exist if parity is an unbroken symmetry of nature. Currently, there is...
In the mirror world hypothesis the mirror baryonic component emerges as a possible dark matter candi...
Parity and time reversal are obvious and plausible candidates for fundamental symmetries of nature. ...
About 80% of the mass of the present Universe is made up of the unknown (dark matter), while the res...
Mirror matter is an entirely new form of matter predicted to exist if mirror symmetry is a fundament...
Recently, the CDMS/Si experiment has observed a low energy excess of events in their dark matter sea...
Mirror world, a parallel hidden sector with microphysics identical to ordinary particle physics, can...
AbstractRecently, the CDMS/Si experiment has observed a low energy excess of events in their dark ma...
AbstractMirror world, a parallel hidden sector with microphysics identical to ordinary particle phys...
We study a two-parameter extension of the cosmological standard model ΛCDM in which cold dark matter...
A new and inexpensive technique for detecting self interacting dark matter in the form of small grai...
We present new fast numerical simulations of cosmic microwave background and large scale structure i...
AbstractWe present new fast numerical simulations of cosmic microwave background and large scale str...
AbstractMirror dark matter interacting with ordinary matter via photon-mirror photon kinetic mixing ...
AbstractMirror dark matter provides a simple framework for which to explain the DAMA/LIBRA annual mo...
Mirror matter is predicted to exist if parity is an unbroken symmetry of nature. Currently, there is...
In the mirror world hypothesis the mirror baryonic component emerges as a possible dark matter candi...
Parity and time reversal are obvious and plausible candidates for fundamental symmetries of nature. ...
About 80% of the mass of the present Universe is made up of the unknown (dark matter), while the res...
Mirror matter is an entirely new form of matter predicted to exist if mirror symmetry is a fundament...
Recently, the CDMS/Si experiment has observed a low energy excess of events in their dark matter sea...
Mirror world, a parallel hidden sector with microphysics identical to ordinary particle physics, can...
AbstractRecently, the CDMS/Si experiment has observed a low energy excess of events in their dark ma...
AbstractMirror world, a parallel hidden sector with microphysics identical to ordinary particle phys...
We study a two-parameter extension of the cosmological standard model ΛCDM in which cold dark matter...
A new and inexpensive technique for detecting self interacting dark matter in the form of small grai...