Time and Date Stamps (logged): 17:12:20 06-10-2020 °¶Ÿ°±Ÿ±¯¯µŸ°¯Ÿ±¯±¯ Physics II

General College Physics (Phy 202) Test 4


Completely document your work and your reasoning.

You will be graded on your documentation, your reasoning, and the correctness of your conclusions.

** Write clearly in dark pencil or ink, on one side of the paper only. **


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Instructions:

Directions for Student:

Test Problems:

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Constants

Constants:

k = 9*10^9 N m^2 / C^2 qE = 1.6 * 10^-19 C h = 6.63 * 10^-34 J s
energy of n=1 orbital in hydrogen atom:  -13.6 eV k '  = 9 * 10^-7 T m / amp atomic mass unit:  1.66 * 10^-27 kg
electron mass:  9.11 * 10^-31 kg speed of light:  3 * 10^8 m/s Avogadro's Number: 6.023 * 10^-23 particles/mole
Gas Constant:  R = 8.31 J / (mole K) proton mass:  1.6726 * 10^-27 kg neutron mass:  1.6749 * 10^-27 kg

 

 

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Problem Number 1

What is the deBroglie wavelength of an electron moving at 7.2 * 10^6 m/s?

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Problem Number 2

A certain hypothetical atom contains 77 protons and 110 neutrons in its nucleus and has an atomic mass of 186.2 atomic mass units, or amu (an amu is approximately 1.66 * 10^-27 kg). How many protons and how many neutrons will it end up with if it undergoes an alpha decay? How many if it undergoes a beta decay? How many if it undergoes a gamma decay?

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Problem Number 3

How much energy will an electron in orbit about a hydrogen atom lose in a transition from orbit # 2 to orbit # 3, where orbits are counted from the closest outward? If this lost energy is carried away by a photon, what will be its wavelength?

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Problem Number 4

A photon of 115.5458 nm electromagnetic radiation encounters an electron in the n = 2 orbital of a hydrogen atom, and causes it to 'jump' to the n = 3 orbital. What will be the wavelength of a photon which carries away any excess energy from the collision?

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Problem Number 5

A spacecraft moving at constant velocity .89 * c relative to a nonaccelerating observer keeps time by reflecting a light pulse back and forth between two mirrors oriented at a right angle to the direction of motion. The mirrors are 100 meters apart (big spaceship) and are mounted within a sealed vertical vacuum tube (vertical being perpendicular to the direction of motion) so that the light pulse will travel at its vaccuum speed.

If we assume that the laws of physics are the same in the reference frame of the spaceship as in the frame of the observer, it follows that the speed of light in a vacuum will be identical in both reference frames.

Under this assumption:

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Problem Number 6

The intensity of light with a mean wavelength of 585 nm falling on a solar sail is 310 watts/m^2.  The sail is oriented perpendicular to the direction of the incoming light, in order to intercept as much light as possible.

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Problem Number 7

Find the velocity an electron in a circular orbit would require at a distance of 2.544 Angstroms from a proton.  Find the deBroglie wavelength of this electron.   Determine the potential and kinetic energies of an orbit at this distance.   Could this orbit exist?  [ The mass of an electron is 9.11 * 10^-31 kg; the proton has a much greater mass; Planck's Constant is 6.62 * 10^-34 J s; k = 9 * 10^9 N m^2 / C^s ]

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Problem Number 8

A hypothetical atom with negligible kinetic energy has a mass of 205 amu. It undergoes a beta decay. The remaining atom has atomic mass 204.5 amu. What is the kinetic energy and/or wavelength (whichever is more appropriate) of the emitted particle, assuming that the kinetic energy of the remaining atom is negligible? How much energy would be released by the decay of a mole of these atoms? Note that the mass of a helium nucleus is about 4.001 amu and the mass of an electron about .00055 amu, where an amu is approximately 1.66 * 10^-27 kg?