physics of the cosmos sections 37.4 – 37.5. reminders today: in-class quiz #6 addressing chapter...

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Physics of the Cosmos Sections 37.4 – 37.5

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Page 1: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Physics of the Cosmos

Sections 37.4 – 37.5

Page 2: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Reminders

• Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test.

• LAB B2-WNL: Wave Nature of Light due Friday @ 4pm.

• Weekly Reflection #13 will be sent out after class today; due Tuesday evening after fall break.

• The Mallard-based reading quiz due prior to class on Tuesday after fall break.

Page 3: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Review

• The time since the beginning of the universe is 1/H years or about 13.8 billion years.

• The Big Bang started off immensely hot!• Radiation dominated the early universe.• Matter dominance occurs after radiation

“cools” enough for matter to condense per the relationship E=mc2.

Page 4: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Matter Dominance (today)

• The universe is composed mostly of matter.• Most of the past 13.8 billion years has been

dominated by matter.• Our “horizon” is 13.8 billion light years away.• During this period, the rate of expansion has

been slowing (but for some recent findings!)• In the past, H was much higher.

Page 5: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Radiation Dominance (early)

• The nature of the radiation was that of a black body radiator at an extremely high temperature.

• The visible remnant of the early universe (radiation) is black body-like with a large red shift.

Page 6: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Wien’s Law

Page 7: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Stefan-Boltzmann Law

Page 8: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Expansion and Olber’s Paradox• Why is the night sky dark?• If the universe is infinite and

without boundary, every line of sight should intersect a star and the sky should be intensely bright.

• Consider the mathematics:– Apparent brightness is

proportional to 1/r2

– The volume of thin layers of space is proportional to r2

– These two effects offset one another!

Page 9: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Some Faulty Explanations

• The universe consists only of the Milky Way – a spinning Island Universe – but today we know that the Milky Way is only one of hundreds of billions of galaxies filling space.

• Absorption of starlight by dust between the clouds. But, no, these clouds would heat up if they absorbed all that radiation and would soon start glowing themselves.

Page 10: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Resolving Olber’s Paradox

• The paradox is resolved by the fact that the universe is expanding,

• distant objects are moving faster with increasing distance,

• and red shifts are greater with more distant objects.

• Ergo, the most distant objects are red shifted into longer wavelengths that we cannot see.

Page 11: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Echo of the Big Bang

• Work of Arno Penzias and Robert Wilson detecting cosmic microwave background radiation.

• Colleagues at Princeton University made an earlier prediction that microwave “echo” should exist as a consequence of the Big Bang.

Page 12: Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Cosmic Background Radiation

• Black body radiator at T = 2.725K and the work of COBE – a perfect match!

• During the earliest stages of the cosmos, the universe was radiation dominated.

• This radiation is just now reaching us from the “horizon” of the universe and is red shifted so it appears as a cold black body radiator.