This topic contains a solution. Click here to go to the answer

Author Question: How did dark matter behave differently from normal matter during the early stages of the big bang, ... (Read 72 times)

ericka1

  • Hero Member
  • *****
  • Posts: 544
How did dark matter behave differently from normal matter during the early stages of the big bang, and how is this important for the formation of stars and galaxies?
 
  What will be an ideal response?

Question 2

How is the Sun's rotation different than that of Earth's?
 
  What will be an ideal response?



Related Topics

Need homework help now?

Ask unlimited questions for free

Ask a Question
Marked as best answer by a Subject Expert

Jayson

  • Sr. Member
  • ****
  • Posts: 350
Answer to Question 1

As long as radiation dominated the early Universe, normal baryonic matter could not contract to form galaxies and stars. Dark, non-baryonic matter does not interact with electromagnetic radiation, and was not affected by the intense radiation.

Tiny fluctuations in the texture of the big bang were caused by quantum mechanical effects. As the Universe expanded, these tiny fluctuations would have been stretched to very large, but subtle, variations in the gravitational field of the Universe. Since dark matter was not affected by radiation, it began to clump around areas of higher gravitational field.

At the time of recombination, baryonic matter was smoothly spread through the Universe, but dark matter was already clumped in filaments. After recombination, ordinary matter quickly gravitated to regions of high dark-matter density.

Dark matter clumping allowed normal matter to clump and begin producing stars and galaxies much faster than normal matter could have done on its own.

Answer to Question 2

Earth is a solid body and rotates equally at all latitudes. The Sun does not rotate as a rigid body; this is possible because the Sun is entirely gas. For example, the equatorial region of the photosphere rotates faster than do regions at higher latitudes. At the equator, the photosphere rotates once every 24.5 days, but at latitude 45 degrees, one rotation takes 27.8 days. This phenomenon is called differential rotation. Helioseismology maps of rotation in the Sun's interior reveal that the gas at different levels also rotates with different periods, another type of differential rotation. Both types of differential rotation seem to be involved in the Sun's magnetic cycle.




ericka1

  • Member
  • Posts: 544
Reply 2 on: Jul 27, 2018
Thanks for the timely response, appreciate it


mohan

  • Member
  • Posts: 362
Reply 3 on: Yesterday
Wow, this really help

 

Did you know?

There are over 65,000 known species of protozoa. About 10,000 species are parasitic.

Did you know?

Approximately 25% of all reported medication errors result from some kind of name confusion.

Did you know?

Patients who have undergone chemotherapy for the treatment of cancer often complain of a lack of mental focus; memory loss; and a general diminution in abilities such as multitasking, attention span, and general mental agility.

Did you know?

The effects of organophosphate poisoning are referred to by using the abbreviations “SLUD” or “SLUDGE,” It stands for: salivation, lacrimation, urination, defecation, GI upset, and emesis.

Did you know?

Only one in 10 cancer deaths is caused by the primary tumor. The vast majority of cancer mortality is caused by cells breaking away from the main tumor and metastasizing to other parts of the body, such as the brain, bones, or liver.

For a complete list of videos, visit our video library