Richard 2.3 Flashcards

(33 cards)

1
Q

What is gravity according to Einstein’s General Relativity?

A

Mass curves space-time; gravity is curved space-time, not a force

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2
Q

What is the “magic carpet” analogy?

A

Space-time is like a flexible carpet that bends with mass.

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3
Q

When was General Relativity developed?

A

1915, during WWI.

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4
Q

What were the 3 classical tests of General Relativity?

A

Mercury’s perihelion precession, gravitational time dilation, bending of starlight.

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5
Q

How does General Relativity explain Mercury’s orbit?

A

Precession of 43 arcseconds/century explained by curved spacetime.

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6
Q

What is gravitational time dilation?

A

Clocks in stronger gravitational fields tick slower than those in weaker fields

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7
Q

How does light behave near a massive object?

A

Light bends as it follows straight lines in curved space-time

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8
Q

What experiment confirmed light bending?

A

1919 solar eclipse: starlight bent 1.8 arcseconds near the Sun

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9
Q

What major objects and phenomena does General Relativity predict?

A

Black holes and gravitational waves.

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10
Q

What did the cosmological principle state?

A

Universe is homogeneous and isotropic on large scales

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11
Q

Who predicted an expanding universe in the 1920s?

A

Alexander Friedmann and Georges Lemaître.

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12
Q

What is the Big Bang in General Relativity?

A

Space itself expands; there is no central point or edge.

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13
Q

Can parts of the universe expand faster than light?

A

Yes, due to space expansion.

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14
Q

How large is the observable universe?

A

About 40 billion light-years across (due to expansion).

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15
Q

What does Hubble’s Constant (HC) measure?

A

The expansion rate of the universe (km/s per Mpc)

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16
Q

Why was Hubble’s original HC wrong?

A

Misidentified Cepheid variable stars.

17
Q

What is today’s debated range of HC values?

A

Mid-60s to early 70s km/s/Mpc.

18
Q

Why does Hubble’s Constant change over time?

A

Universe’s gravity affects expansion rate
- universe expansion was decelerating, now accelerating

19
Q

What is critical density?

A

The density needed to halt expansion and cause collapse.

20
Q

What is the current matter density relative to critical?

A

About 30% of critical density → underdense universe.

21
Q

What is accelerated expansion?

A

Universe expansion speeding up rather than slowing.

22
Q

What causes accelerated expansion?

A

Dark energy (consistent with cosmological constant).

23
Q

What is dark energy?

A

Unknown form of energy with negative pressure, constant density across space.

24
Q

How does dark energy behave as universe expands?

A

Density stays constant, unlike matter which thins out.

25
When did universe transition from decelerating to accelerating?
About 4 billion years ago.
26
What fraction of the universe is dark matter?
About 25%.
27
What happens to Hubble’s Constant in the future?
Will slowly approach a fixed value.
28
Will the universe expand forever?
Yes, dark energy dominance causes eternal expansion.
29
What is the coincidence problem?
Why do we live at the time when dark energy starts to dominate?
30
What happens to distant galaxies in the future?
They will move beyond our observable horizon.
31
Could Hubble’s Constant reach zero?
Only if universe were to collapse (current data says it won’t).
32
What is phantom energy?
Hypothetical energy that increases with expansion (likely sci-fi).
33
What does current data suggest about dark energy?
Consistent with cosmological constant (Einstein’s "blunder").