Consider two Einstein solids in thermal contact. Solid A contains 5 atoms while solid B has 2 atoms. If the system has a total energy of 10ϵ10ϵ, what is the total number of microstates available to the 6:4 macropartition? The total number of microstates available to the 6:4 macropartition is Choose one a) 126,502,423 b) 308,411 C) 5,784,693 D) 4,883, 760 E) 3,141,592

Consider two Einstein solids in thermal contact. Solid A contains 5 atoms while solid B has 2 atoms. If the system has a total energy of 10ϵ10ϵ, what is the total number of microstates available to the 6:4 macropartition? The total number of microstates available to the 6:4 macropartition is Choose one a) 126,502,423 b) 308,411 C) 5,784,693 D) 4,883, 760 E) 3,141,592

Similar questions

The image shows the example of finding the number of vacancies in 1 cubic meter of copper (Cu) at 1000 degrees celcius (1273 k) considering the image data. Replicating the problem in the image, calculate the number of vacancies but at room temperature.Explain why there is such a difference in the number of vacancies at both temperatures.
Experiment 1. The student measures the volume of the gas in the cylinder, places a known mass mon top of the piston, and then increases the temperature of the gas at constant pressure to 273C. Experiment 2. After the gas is allowed to cool back to 0C at 1 atm pressure, the student locks the piston in place, and then increases the temperature of the gas to 273C. Experiment 3. After Experiment 2 is completed, the student unlocks the piston, and a computer-controlled heat source maintains the temperature at a constant 273C. After Experiment 2, how do the pressure and volume change (increase/decrease/remain the same)? After Experiment 3?
What is the average thermal velocity of a hydrogen molecule H at 27 \deg C? (Assume: Boltzmann constant = 1.38 x 10-23 J/K and the mass of H is m = 3.32 x 10-27 kg)
Interstellar space is quite different from the gaseous environments we commonly encounter on Earth. For instance, a typical density of the medium is about 1 atom cm−3 and that atom is typically H; the effective temperature due to stellar background radiation is about 10 kK. Estimate the diffusion coefficient and thermal conductivity of H under these conditions. Compare your answers with the values for gases under typical terrestrial conditions. Comment: Energy is in fact transferred much more effectively by radiation.
An SUV tire contains 0.037 m3 of air at a gauge pressure of 2.61 × 105 N/m2. The composition of air is about 78% nitrogen (N2) and 21% oxygen (O2), both diatomic molecules. How much more internal energy, in joules, does the air in the tire have than the same volume of air has at zero gauge pressure outside the tire? Einternal,2−Einternal,1 = ? Hints: -Assume not only equal volumes but also equal temperatures.-Since the temperature is constant, what must be changing in this process?-The heat capacity, and thus the internal energy, depends upon whether gas is monatomic or diatomic.