Astrophysics Flashcards

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1
Q

Properties of CMBR

A
  • Uniform intensity in all directions

- Structure in background intensity/ small ripples

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2
Q

How the standard model of the universe affects these properties (of CMBR)

A
  • Produced when matter and radiation decoupled
  • Originally gamma radiation
  • (gamma radiation) red-shifted to microwave / originally higher energy
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3
Q

Explain the significance of the properties (of CMBR) as evidence for the past evolution of the universe

A
  • Evidence that universe began with big bang

- Temperature corresponds to 2.7 K / 3K / that predicted by big bang model

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4
Q

Formation of Neutron Star/Black Hole

A
  • Hydrogen runs out in the star and stops burning
  • This lead to the onset of Helium fusion and expand to a Red Supergiant
  • Then there is a gravitational collapse of the core (as the radiation/gas pressure is now lesser than the gravitational pressure)
  • Supernovae explosion takes place
  • If Mass of the core is between the Chandrasekhar limit and 3 Solar Masses a Neutron Star is Formed if it is greater than 3 Solar Masses then a Black hole is formed
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5
Q

Cosmological Principle

A

Homogenous- mass is evenly distributed

Isotropic-looks the same in all directions

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6
Q

Why understanding of the earliest moments of universe are unreliable

A
  • No Experimental/Physical Evidence
  • States of Matter/laws of physics were unknown at the time
  • The energies/ temperatures are unreproducible
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7
Q

Hubble’s law

A

v=Hnougt*d

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8
Q

What is the big bang and how does it explain the origin of CMBR?

A

-Creation of the universe (from which space/time evolved)
-(At the start) the universe was hot / infinitely dense
Expansion of the universe led to cooling
-The (current) temperature of the universe is 2.7 K / 3 K
-The (wavelength of the) gamma radiation stretched to microwaves (by the expansion).
-(Cosmological principle is supported because) CMBR is isotropic

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9
Q

Evidences for the Big Bang

A

-star-light shows red shift
-galaxies receding from Earth
-recessional velocity proportional to distance
-cosmological microwave background radiation (CMBR)
-uniform intensity in all directions
small ripple (1)
-(black body temperature) of 2.7 K (3K)-
-High ratio of helium to hydrogen (1) Indicates very high temperatures existed (1) ratio too high to originate from stellar fusion (1)

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10
Q

How Edwin Hubble provided evidence for an expanding universe

A
  • red shift data for galaxies
  • Which can be used to calculate velocity from red shift 1
  • Which shows galaxies/ stars receding from Earth
  • Distance data for galaxies can be used to calculate velocity using Hubble’s Law
  • Hence, universe began at a single point
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11
Q

Formation of a Star such as sun and possible evolution

A
  1. (Interstellar dust and gas) cloud is drawn together by gravitational force / gravity in a gravitational collapse
  2. Loss in (gravitational) PE / KE increases / temperature increases
  3. Fusion (of protons / hydrogen nuclei) takes place
    Protons / hydrogen nuclei combine to make helium (nuclei)
  4. Energy is released in fusion reactions
  5. A stable star is formed when gravitational pressure is equal to internal / gas / radiation pressure
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12
Q

Charecteristics of a white dwarf

A
  • (extremely) dense / (very) hot / low luminosity
  • no fusion reactions occur
  • it is a remnant of a low-mass star
  • correct reference to Fermi pressure / electron degeneracy / Chandrasekhar’s limit
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13
Q

Why is the the star the brightest when its coolest

A
  • This occurs in a red giant

- (It is cooler but has) large surface area (and therefore radiates large amounts of energy)

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14
Q

Evolution of Universe

A
  1. (At the start it was) very hot / extremely dense / singularity
  2. All forces were unified
  3. Expansion led to cooling
  4. Quarks / leptons (soup)
  5. More matter than antimatter
  6. Quarks combine to form hadrons / protons / neutrons
  7. Imbalance of neutrons and protons / (primordial) helium produced
  8. Atoms formed
  9. Idea of gravitational force responsible for formation of stars / galaxies
  10. Temperature becomes 2.7 K / 3 K or (the universe is saturated with cosmic) microwave background radiation
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15
Q

Absorption Spectrum

A
  • Dark lines / bands

- against a background of continuous spectrum

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