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Yet in order to explain the actual universe having "nebulae", it was thought that the matter density was neglible in comparison to vacuum density Λ/8π.
Luckily, theorists could still have a flat beautiful universe because the gap in the matter density was made up by the so-called dark energy that astronomers have recently discovered seems to be accelerating the expansion of the universe.
By that year, of course, the universe was known to be expanding; therefore, the only way to explain a constant (steady state) matter density was to postulate the continuous creation of matter to offset the attenuation caused by the cosmic expansion.
In resting-state MRI studies comparing interictal migraineurs to healthy control subjects, decreased grey matter density was observed in the left TP [10] and the left TP exhibited decreased connectivity with components of the default-mode network [11].
Using the voxel-based morphometric analysis of the structural T1-weighted MRI scans, a significant structural difference in grey matter density was found in patients with cluster headache when compared to healthy volunteers.
An alternative concept is that they formed closer to the Sun, where the matter density was higher, and then subsequently migrated to their current orbits after the removal of the gaseous protoplanetary disc.
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Therefore the uniformity of bale dry matter density is a determinant for the successful operation of any dryer.
Uncertainty of model forcing and soil properties (sand fraction, clay fraction and organic matter density) were considered in the ensemble predictions of the soil moisture profiles.
We know what the matter density is everywhere we look.
At its current precision, the experiment rules out only chameleons whose interaction with matter the thing that makes the field go away where the matter density is high is much stronger than gravity, Khoury says.
Thus a common task performed on cosmological simulation data sets is determining the distribution, sizes, and merger histories of dark matter halos, which are identified as regions in simulations where the dark matter density is higher than some prescribed threshold.
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Justyna Jupowicz-Kozak
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