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 33 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
YES! Correct, THANKS for helping me on my review


cpetit11

  • Member
  • Posts: 321
Reply 3 on: Yesterday
Thanks for the timely response, appreciate it

 

Did you know?

Your heart beats over 36 million times a year.

Did you know?

Cyanide works by making the human body unable to use oxygen.

Did you know?

Fatal fungal infections may be able to resist newer antifungal drugs. Globally, fungal infections are often fatal due to the lack of access to multiple antifungals, which may be required to be utilized in combination. Single antifungals may not be enough to stop a fungal infection from causing the death of a patient.

Did you know?

The top five reasons that children stay home from school are as follows: colds, stomach flu (gastroenteritis), ear infection (otitis media), pink eye (conjunctivitis), and sore throat.

Did you know?

Coca-Cola originally used coca leaves and caffeine from the African kola nut. It was advertised as a therapeutic agent and "pickerupper." Eventually, its formulation was changed, and the coca leaves were removed because of the effects of regulation on cocaine-related products.

For a complete list of videos, visit our video library