PHYSICS OCR B MATTER, Exercises of Physics

MATTER TOPIC PHYSICS OCR B A LEVEL

Typology: Exercises

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Matter starting to ‘come apart’
The energy per particle in matter at temperature T is typically of the order of magnitude kT, where k is the
Boltzmann constant 1.38 x 10–23 J K–1. A few particles will have energies quite a lot greater than average.
In these questions you will see examples of processes which happen at an appreciable rate, when the
energy required is in the range roughly 10 to 30 times kT. Electron charge = 1.6 x 10-19C, NA = 6.03 x 1023.
1. Energy 40 kJ mol–1 is required to evaporate water molecules from the liquid. Convert this to joules
per particle.
2. Water evaporates at a noticeable rate at 300 K, even though it only boils (at atmospheric pressure)
at 373 K. Calculate the value of kT at 300 K. What is the ratio /kT, where is the energy needed to
evaporate one molecule?
3. Electrons ‘evaporate’ from heated metals. This ‘thermionic emission’ is used to obtain the electron
beam in a television set. The energy required to remove an electron from platinum is 5.4 eV. Express this
energy in joules per electron.
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Matter starting to ‘come apart’

The energy per particle in matter at temperature T is typically of the order of magnitude kT, where k is the Boltzmann constant 1.38 x 10–23^ J K–1. A few particles will have energies quite a lot greater than average. In these questions you will see examples of processes which happen at an appreciable rate, when the energy required is in the range roughly 10 to 30 times kT. Electron charge = 1.6 x 10-19C, NA = 6.03 x 10^23.

  1. Energy 40 kJ mol–1^ is required to evaporate water molecules from the liquid. Convert this to joules per particle.
  2. Water evaporates at a noticeable rate at 300 K, even though it only boils (at atmospheric pressure) at 373 K. Calculate the value of kT at 300 K. What is the ratio /kT, where  is the energy needed to evaporate one molecule?
  3. Electrons ‘evaporate’ from heated metals. This ‘thermionic emission’ is used to obtain the electron beam in a television set. The energy required to remove an electron from platinum is 5.4 eV. Express this energy in joules per electron.
  1. At room temperature, the emission of electrons from platinum is negligible. However, at 2000 K, an appreciable thermionic current can be detected. Calculate the value of kT at 2000 K. What is the ratio /kT, where  is the energy needed to ‘evaporate’ one electron from platinum?
  2. What would you predict about thermionic emission from thorium-coated tungsten, for which the energy needed to remove an electron is 2.6 eV?
  3. The surface of the Sun is at a temperature of about 6000 K. ‘Typical’ photons from a hot object at temperature T have energy of approximately 3kT. Calculate energy 3kT and the wavelength of a ‘typical’ photon from the Sun. h = 6.6 x 10–34^ J Hz–1^ and c = 3 x 10^8 m s–1. In what part of the electromagnetic spectrum does it fall?
  4. Sunlight does contain a small proportion of ultraviolet radiation. As evidence, you get sunburn in direct sunlight. The wavelength of the ultraviolet radiation may go down to as short as 100 nm. How many times larger than the ‘typical’ energy 3kT of a photon is the energy of these ultraviolet photons?

Grease can just about be washed off dirty dinner plates using hot water. Greases often stick together by hydrogen bonds, with energy  of the order 20 kJ mol–1.

  1. Estimate the ratio /kT for doing the washing up, pulling apart a few hydrogen bonds to move a grease molecule. Solid carbon dioxide, often called dry ice, slowly evaporates (sublimes) at the low temperature of –78ºC, or 195 K.
  2. Calculate the energy kT, in units of kJ mol–1, at 195 K.
  3. The energy  to evaporate solid carbon dioxide is 27 kJ mol–1. What is the ratio /kT at 195 K?