Lecture 33 Flashcards

1
Q

What is happening to spacetime?

A

It is expanding as the fabric of space between galaxies is stretching and carrying galaxies away from one another. It is not an explosion of galaxies through space from a centre.

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2
Q

How is the universe’s expansion affected by velocity and acceleration?

A
  • the size of the universe can grow with no acceleration (constant velocity expansion)
  • when the initial velocity is positive the universe can expand while decelerating
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3
Q

What could change the expansion rate of the universe?

A
  • attractive force (gravity) = deceleration (Hubble constant gets smaller)
  • repulsive force (spacetime pushed apart) = acceleration ( Hubble constant gets larger)
  • balanced forces = no acceleration= coasting
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4
Q

Why would it be expected for the expansion of the universe to slow?

A

As gravity is an attractive force would act to slow the initial expansion of the universe

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5
Q

How does the Hubble constant show expansion?

A

The rate of expansion is represented by the Hubble constant, which is the slope of the Hubble diagram- a big Ho = fast expansion

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6
Q

What can be used as standard candles when measuring universe expansion?

A

White dwarf supernova- z~1 (a=0.5)

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7
Q

What is the process of observing the difference in the expansion theories of the early universe?

A

Compare redshift distance with luminosity distance. In doing this, it can be seen that the farther away the object, the bigger the difference between the different models.

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8
Q

What did the 1998 measurements show about the expansion of the universe?

A

The measurements showed that the universe was actually expanding. The observation of type 1a SN appeared fainter than expected for their redshifts, therefore further away than expected. This indicated that the universe was accelerating.

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9
Q

What is thought to be pushing spacetime apart?

A

Dark energy

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10
Q

What are some of the reasons people thought the universe could not be accelerating?

A
  • mistakes in observations/calculations
  • dust in distant galaxies made the SN brighter
  • ancient SN could have behaved differently to modern SN.
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11
Q

Around what time did the universe stop decelerating in expansion?

A

About 5 billion years ago (around redshift 0.5)

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12
Q

What is the theorised purpose and effect of dark energy?

A

It is proposed to be a counter the effects of gravity and causes the acceleration of the universe

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13
Q

What proportion of the universe is dark energy?

A

It is the primary constituent of the universe accounting for around 70% of its makeup.

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14
Q

What is dark energy?

A

The leading hypothesis is that dark energy is a cosmological constant- it is negative pressure of space

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15
Q

What is the density of dark energy in the universe?

A

The amount of dark energy in the universe remains constant even though the universe expands meaning that the relative density of dark energy compared to matter increases over time.

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16
Q

What did the Sloan survey show?

A

It used distant galaxies to show that expansion was faster in the past

17
Q

What will happen as the expansion of the universe speeds up?

A
  • there will be less and less galaxies visible in the sky a more distant sources move outside the visible horizon
  • fewer new galaxies and stars will be formed because the expansion will lower the density of intergalactic gas
  • gravitationally bound structures (galaxies and dark matter halos) will be left unaffected
18
Q

What is a spacetime diagram?

A
  • a graph of time vs space
  • light travels on world lines at angles greater than or equal to 45 degrees
  • nothing travels faster than the speed of light so all world lines must be equal to or steeper than 45 degrees
19
Q

What are the effects of the spacetime diagram?

A

We can only receive and transmit information to spacetime locations (events) inside our light cone

20
Q

What happens to the light cone as we move forward in time?

A

The light cone is expands and is larger at future times

21
Q

What does the horizon show us?

A
  • the horizon depends on when and where we are
  • the age of the universe sets the maximum distance we can see
  • the actual universe may be larger or infinite but we cannot tell
22
Q
A
23
Q
A