PHYS 3022 Lecture 12 (Wise)

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Pressure Integral

26 Terms

1
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What does hydrostatic equilibrium describe?

Gravity is balanced by pressure.

2
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What does mass conservation track in a star?

How enclosed mass changes with radius.

3
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What does an equation of state relate?

Pressure to the physical state and properties of gas.

4
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What is gas pressure microscopically caused by?

Particles transferring momentum through collisions.

5
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What is the pressure integral used for?

Calculating pressure from a particle momentum distribution.

6
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What does particle number density mean?

Number of particles per unit volume.

7
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What distribution is used to derive ideal gas pressure for massive particles?

The Maxwell–Boltzmann velocity distribution.

8
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What is the ideal gas law's conceptual message?

Gas pressure depends on particle density and temperature.

9
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What is mean molecular weight (μ)?

Average mass per gas particle, measured relative to hydrogen mass.

10
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What influences a gas's mean molecular weight?

Its chemical composition and ionization state.

11
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How is a completely neutral gas's particle count characterized?

Atoms contribute particles; there are no free electrons from ionization.

12
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Why does ionization change mean molecular weight?

Free electrons increase the total number of particles.

13
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For an ionized atom, what particles are counted?

Its nucleus/ion and its free electrons.

14
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What is a mass fraction?

The fraction of total gas mass contributed by a species.

15
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What do X, Y, and Z represent in stellar composition?

Mass fractions of hydrogen, helium, and metals, respectively.

16
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What does the metal fraction Z mean in stellar astrophysics?

The mass fraction in elements heavier than helium.

17
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What does the weighted metal-composition average account for?

The relative abundances and atomic weights of metals.

18
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How does ionization generally affect particle number per unit mass?

It increases the number of particles per unit mass.

19
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What is the typical young-star composition used in lecture?

Hydrogen 0.70, helium 0.28, metals 0.02 by mass.

20
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For that young-star example, how do neutral and ionized μ compare?

Neutral μ ≈ 1.3; ionized μ ≈ 0.62.

21
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What is the average kinetic energy per particle in a Maxwellian gas?

It increases in proportion to absolute temperature.

22
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What is radiation pressure associated with?

Momentum carried by photons.

23
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What sets radiation energy density in thermal equilibrium?

Temperature; it scales as the fourth power of temperature.

24
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What are the two contributions to total pressure in the lecture?

Gas pressure and radiation pressure.

25
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Which pressure dominates in the Sun's core example?

Gas pressure; radiation pressure is only about 0.065% of gas pressure.

26
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Why is radiation pressure small in the cited solar-core example?

Its calculated value is much smaller than gas pressure.