Lorem ipsum adipiscing elit, sed diam nonummy nibh euismod tincidunt ut laoreet dolore magna aliquam erat volutpat. Nulla lacinia; sapien in volutpat mattis, eros arcu rhoncus erat, iaculis sodales ante massa lobortis arcu. Etiam ullamcorper, libero sed rhoncus adipiscing, ante arcu dignissim urna, quis iaculis quam sapien eu velit. Praesent ut pulvinar lectus.
Donec enim enim, venenatis nec posuere in; dictum id lacus. Quisque vestibulum luctus tortor at vulputate. Maecenas mi augue, vehicula et consectetur ac, vulputate a risus. Pellentesque in feugiat elit. Curabitur sed diam enim. Sed varius faucibus lectus, a scelerisque massa posuere ac. Quisque dapibus, est ac rhoncus tempus, nisl purus posuere urna, accumsan lobortis metus mauris at nibh. Duis ullamcorper adipiscing quam in dapibus. Nulla facilisi. Praesent sagittis commodo lorem, vitae euismod justo venenatis at. Suspendisse et ante dui. Etiam id enim at sem rhoncus sodales commodo et nulla. Donec sed erat dolor, vitae auctor mauris. Suspendisse feugiat mollis ante vitae blandit. Cum sociis natoque penatibus et magnis dis parturient montes, nascetur ridiculus mus. Duis elementum, massa eget sollicitudin egestas, risus diam posuere elit; quis luctus eros velit eget odio. Maecenas at mauris sit amet orci scelerisque adipiscing. Sed tincidunt sollicitudin suscipit. Fusce lobortis sagittis arcu eu volutpat! Ut vitae facilisis nisi. Quisque sodales auctor sem in mollis! Phasellus mi urna, vehicula quis congue et, pellentesque non nisi. Suspendisse pellentesque sollicitudin orci ac condimentum? Sed mollis tempor enim, eu eleifend est molestie vitae. Duis magna dolor, iaculis sed pharetra nec, venenatis vitae dui. Sed eros quam, venenatis a hendrerit nec, vehicula ut diam.
Etiam diam magna; porta sed gravida vel, molestie non lacus. Donec laoreet est vitae enim hendrerit egestas. Vivamus ultricies elementum nisl, in consectetur eros laoreet ut! Donec porttitor venenatis rhoncus. Nunc pretium erat at dui laoreet egestas. Sed sed diam ante! Duis nisi felis, rhoncus id tempor at, fermentum ac metus. Aenean ante tellus, congue volutpat molestie nec, tempor quis purus. Aliquam sollicitudin porttitor ipsum; eu consectetur metus dictum porta. Maecenas imperdiet ornare urna, sed hendrerit odio pharetra a. Curabitur quam mi, pulvinar nec gravida eget, rhoncus vel elit. Maecenas lacinia nulla sit amet eros mollis eu pulvinar magna varius. Praesent sagittis; arcu sed facilisis pharetra, ante urna posuere nulla, at ultrices nisl diam ac dolor. Fusce eu diam turpis. Donec feugiat libero ut lectus consectetur ac consectetur velit eleifend. Curabitur elit nibh, viverra sed tempor eget, commodo eget elit? Aenean odio neque; blandit nec sodales non, consectetur blandit sem.</p><p> Sed tempor eleifend diam, eget vestibulum lectus imperdiet a. Nam interdum nisl a quam aliquet sed molestie nulla ullamcorper! Integer tincidunt dictum nisl, ut congue metus rhoncus fermentum. Cras tempus vestibulum lorem quis sollicitudin. Vestibulum non est vel magna vestibulum gravida a eu arcu. Aliquam sagittis, sapien eget ullamcorper eleifend, tortor arcu luctus elit, eget convallis dui arcu sed purus. Proin a mauris justo. Mauris tortor nisl, tincidunt eu tincidunt nec, interdum eu massa.
They are generally known as WIMPs (for weakly interacting huge particles), and in the
event that they exist, these particles have lots tens or a whole lot of occasions higher than that of a proton but work together so weakly with atypical matter that they are difficult to detect.
Using this method, astronomers have confirmed that galactic clusters certainly have excessive plenty exceeding these measured
by luminous matter and, as a result, have provided extra proof of darkish matter.
Is it an exotic, undiscovered type of matter, or is it peculiar matter that now we have issue observing?
As astronomers gathered clues in regards to the existence - and staggering amount - of darkish matter,
they turned to the computer to create models of how the strange stuff may be organized.
If distant galaxies typically lie inside a shroud of darkish matter, then the Milky Way
may, too. The objective of LHC experiments isn't
to produce WIMPs instantly, however to supply different particles that
might decay into darkish matter. The researchers disagreed,
nevertheless, on the density of the dark matter across Abell 383.
One staff calculated that the dark matter increased toward the center of the cluster, while the other measured
much less dark matter at the center.