Cosmology and Big Bang Flashcards

1
Q

studying universe methods

A

observations - deep survery of galaxies (100s of millions mapped), background radiation, and element abundances.

simplified theoretical models - examples include homogeneity, isotropy, etc.

computer simulations

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2
Q

observational facts on recession of galaxies

A

fact 1: except for some near ones, light from all galaxies is redshifted.

fact 2: redshift is proportional to distance.

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3
Q

recession of galaxies (hubbles law of 1929)

A

from hubble plots of recession speed vs. distance we get [v = H x D].

everything is moving away from everything else, everything looks like the center but there is no center.

distance is stretching because universe expansion happening at 70 km/s/Mps = 700 km/year/ly.

tracing back universe, it must have started from a point (big bang).

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4
Q

evidence for big bang

A

expanding universe (hubble law)

cosmic microwave background radiation

abundance of elements (big bang nucleosynthess)

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5
Q

big bang is twofold

A

first part if the initial creation event: point from which universe began to expand, Gamow (1940s) proposed universe began in an explosive event giving birth to matter space time, etc. 13.8 billion years ago.

second part is the entire physical model/scenarios of universe’s evolution from t=0 onward; expansion, cooling, nuclear reactions, radiations, etc.

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6
Q

big bang theory beginning

A

very dense very hot beginning, first energy produces particles, then protons fuse to make helium (plus a little lithum and berilium) during first 3 minutes of universe

380,000 years later hydrogen forms; matter.

full model traced evolution of universe in time.

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7
Q

future of the universe

A

depending on matter/energy/density:

eternal expansion/big rip, collapse/big crunch, equilibrium

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8
Q

big rip

A

universe expands infinitely, expansion accelerates overtime until everything tears apart.

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9
Q

big crunch

A

gravity slows and expansion reverses, universe contracts back to a hot/dense state, possible reversal of big bang.

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10
Q

equilibrium

A

universe stabilizes, balances forces prevent expansion or collapse, stability is long-term

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