Dark energy may have a completely unknown aspect of physics acting as an accomplice in its efforts to defy gravity, suppressing the growth of large-scale structures like galaxy superclusters.

Just saying it's consistent to the Lambda-CDM, that's not enough in itself. It has to be consistent with Lambda-CDM and give you the same parameters for the basic properties of that model." ...

This “cold dark matter” model is the CDM in our Lambda-CDM model of cosmology, and it’s been pretty successful in explaining how the tiny density fluctuations in the cosmic microwave ...

The Lambda-CDM model puts tight restrictions on the upper limit of neutrino masses. That could change if dark energy turns out to be varying rather than constant: the upper boundary would increase ...

In the Lambda-CDM model, it’s the accelerating expansion of the universe that gives photons their extra redshift in later times.

Dark energy, the mysterious force driving the accelerated expansion of the universe, has puzzled scientists since its ...

The prevailing model of cosmology, called the lambda-CDM model (lambda for the cosmological constant; CDM for cold dark matter—more on this in a moment), imposes an upper boundary for the age of ...

Plugging these into the Lambda-CDM model spat out a Hubble constant of roughly 46,200 mph per million light-years, or roughly 67 kilometers per second per megaparsec.

Right now, the leading theory, or standard model, of cosmology is called "Lambda CDM.' Lambda denotes the cosmological constant describing dark energy, and CDM stands for cold dark matter.

Largest Map of Mass Distribution The standard model of cosmology, called Lambda-CDM, includes two key ingredients.