Dark matter collisions with Xe on earth

This is a very small number, indicating that the chances of detecting dark matter particles in this scenario are very low. In summary, assuming a density of 0.3 GeV/cm3, a dark matter particle mass of 100 GeV, and a velocity of 200 km/s, with a cross section of 10^-44 cm^2, we can expect to see approximately 0.00001578 collisions per year in a cubic meter of Xenon at room temperature.
  • #1
j-lee00
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original question

Assume that the density of dark matter near the Earth is 0.3 GeV / cm3 and that the dark matter particle has a mass of 100 GeV and a velocity of 200 km/s. If the dark matter-nucleon cross section is 10^-44cm2 calculate how many events you would expect to see every year in a metre cubed volume of Xenon at room temperature.

I have worked out that

1) density of dark matter particles near Earth is 3 particles per m^3
2) the flux of the dark matter 6 * 10^5 m^-2 s^-1 passing through a m^3 of Xe
3) that there are 1.668 *10^25 particles in a m^3 of xenon

if the the cross section of dark matter 10^-44 cm^2

How do i work out the number of collisions per second?
 
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  • #2


To calculate the number of collisions per second, we can use the following formula:

Number of collisions per second = density of dark matter particles * flux * number of particles in a cubic meter * cross section

Plugging in the values we have calculated, we get:

Number of collisions per second = 3 particles/m^3 * 6 * 10^5 m^-2 s^-1 * 1.668 * 10^25 particles/m^3 * 10^-44 cm^2

= 3 * 6 * 10^5 * 1.668 * 10^25 * 10^-44 collisions/s

= 3 * 10^6 * 1.668 * 10^-19 collisions/s

= 5.004 * 10^-13 collisions/s

Therefore, we can expect to see approximately 5.004 * 10^-13 collisions per second in a cubic meter of Xenon at room temperature. To calculate the number of collisions per year, we can multiply this value by the number of seconds in a year (3.154 * 10^7):

Number of collisions per year = 5.004 * 10^-13 collisions/s * 3.154 * 10^7 s/year

= 1.578 * 10^-5 collisions/year

Therefore, we can expect to see approximately 0.00001578 collisions per year in a cubic meter of Xenon at room temperature.
 

1. What is dark matter?

Dark matter is a type of matter that does not interact with light, making it invisible to telescopes and other traditional means of detection. Its existence is inferred from its gravitational effects on visible matter.

2. How do dark matter collisions with Xe occur on earth?

Dark matter collisions with Xe on earth may occur when dark matter particles, which make up a significant portion of the universe, pass through the Earth and interact with xenon atoms in underground detectors.

3. Why is Xe used in detecting dark matter collisions on earth?

Xe, or xenon, is used in detecting dark matter collisions on earth because it is a heavy, inert gas that is sensitive to the energy released during a collision. It is also readily available and has a low natural radioactivity, making it a suitable material for use in underground detectors.

4. What can we learn from dark matter collisions with Xe on earth?

Studying dark matter collisions with Xe on earth can provide insight into the properties and behavior of dark matter particles, such as their mass and interaction strength. It can also help us understand the distribution of dark matter in our galaxy and the universe.

5. Are dark matter collisions with Xe on earth dangerous?

No, dark matter collisions with Xe on earth are not dangerous. The energy released in these collisions is extremely small and poses no threat to human health. The underground detectors used to study these collisions are also designed to prevent any harmful effects on the surrounding environment.

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