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An alpha particle (\(m = 6.64 \times 10^{-27} kg\)) emitted in the radioactive decay of uranium-238 has an energy of 4.20 MeV. What is its de Broglie wavelength?

Short Answer

Expert verified
The de Broglie wavelength is \(1.51 \times 10^{-15}\) m.

Step by step solution

01

Convert Energy Units

Convert the given energy from MeV to joules. The conversion factor is \(1 \text{ MeV} = 1.60218 \times 10^{-13} \text{ J}\). So, the energy in joules is \(4.20 \text{ MeV} \times 1.60218 \times 10^{-13} \text{ J/MeV} = 6.729156 \times 10^{-13} \text{ J}\).
02

Use the Energy-Momentum Relation

The relationship between energy and momentum for a non-relativistic particle is given by \(E = \frac{p^2}{2m}\). Rearrange to solve for momentum \(p\) as \(p = \sqrt{2mE}\). Substitute \(m = 6.64 \times 10^{-27} \text{ kg}\) and \(E = 6.729156 \times 10^{-13} \text{ J}\) to find \(p = \sqrt{2 \times 6.64 \times 10^{-27} \text{ kg} \times 6.729156 \times 10^{-13} \text{ J}}\). Upon simplifying, \(p = 4.375 \times 10^{-19} \text{ kg m/s}\).
03

Calculate the de Broglie Wavelength

Use the de Broglie wavelength formula \(\lambda = \frac{h}{p}\), where \(h = 6.626 \times 10^{-34} \text{ J s}\) is Planck's constant. Substitute \(p = 4.375 \times 10^{-19} \text{ kg m/s}\) to get \(\lambda = \frac{6.626 \times 10^{-34} \text{ J s}}{4.375 \times 10^{-19} \text{ kg m/s}}\). Calculate the wavelength as \(\lambda = 1.51 \times 10^{-15} \text{ m}\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Radioactive Decay
Radioactive decay is a natural process where unstable atomic nuclei lose energy by emitting radiation. This process can result in the transformation of one element into another. Radioactive decay occurs because the nucleus of an atom is unstable due to the imbalance of forces within it.
The three main types of radioactive decay are alpha decay, beta decay, and gamma decay. In alpha decay, the nucleus emits an alpha particle, reducing the atomic number by two and the mass number by four. The time it takes for a substance to decay to half its original amount is called its half-life. This concept is crucial in fields such as nuclear physics and medicine, as it helps scientists predict how long a radioactive substance will be active.
Alpha Particle
An alpha particle is a type of radiation composed of two protons and two neutrons. This makes it identical to a helium-4 nucleus. Alpha particles are quite hefty compared to other forms of radiation like beta particles and gamma rays. Due to their size, they have a low penetration ability but are highly effective at ionizing other atoms.
Alpha particles are commonly emitted during alpha decay, a type of radioactive decay. When an alpha particle is emitted, it carries away a significant amount of energy from the nucleus, which can result in changes to the identity of the atom. For instance, uranium-238 becomes thorium-234 upon emitting an alpha particle.
In the context of the exercise, the alpha particle emitted from the decay of uranium-238 is precisely what gives rise to the de Broglie wavelength calculations.
Energy Conversion
Energy conversion is essential in understanding physical processes, especially when dealing with units like MeV and joules. MeV, or mega electron volts, is a unit of energy commonly used in nuclear and particle physics. It measures the energy of subatomic particles, like the alpha particle in the exercise.
To make calculations manageable, we often convert MeV to joules. One electron volt (eV) is the energy gained by an electron when it is accelerated through a potential difference of one volt. One MeV equals one million eVs, and since 1 eV is equal to \(1.60218 \times 10^{-19} \text{ J}\), this allows for straightforward conversion to joules.
In this exercise, the energy of the alpha particle is given as 4.20 MeV, which, when converted using the factor \(1.60218 \times 10^{-13} \text{ J/MeV}\), becomes \(6.729156 \times 10^{-13} J\). This conversion is a crucial step in solving problems involving energy calculations.
Momentum Calculation
Momentum is a key concept in physics, often calculated as the product of an object's mass and velocity. In particle physics, momentum helps us understand how particles move and interact at the smallest scales.
In the exercise, the goal is to determine the de Broglie wavelength of an alpha particle. A critical step is calculating the particle’s momentum using its energy. This is done through the formula relating energy and momentum: \(E = \frac{p^2}{2m}\), where \(E\) is energy, \(m\) is mass, and \(p\) is momentum.
Rearrange the formula to find \(p\):
  • \(p = \sqrt{2mE}\)
By substituting the mass \(6.64 \times 10^{-27} \text{ kg}\) and energy \(6.729156 \times 10^{-13} \text{ J}\), we compute the momentum: \(p = 4.375 \times 10^{-19} \text{ kg m/s}\).
Understanding momentum calculations is vital for determining the de Broglie wavelength, as demonstrated in this exercise.

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Most popular questions from this chapter

A scientist has devised a new method of isolating individual particles. He claims that this method enables him to detect simultaneously the position of a particle along an axis with a standard deviation of 0.12 nm and its momentum component along this axis with a standard deviation of 3.0 \(\times\) 10\(^{-25}\) kg \(\bullet\) m/s. Use the Heisenberg uncertainty principle to evaluate the validity of this claim.

A 4.78-MeV alpha particle from a \(^{226}\)Ra decay makes a head-on collision with a uranium nucleus. A uranium nucleus has 92 protons. (a) What is the distance of closest approach of the alpha particle to the center of the nucleus? Assume that the uranium nucleus remains at rest and that the distance of closest approach is much greater than the radius of the uranium nucleus. (b) What is the force on the alpha particle at the instant when it is at the distance of closest approach?

Two stars, both of which behave like ideal blackbodies, radiate the same total energy per second. The cooler one has a surface temperature \(T\) and a diameter 3.0 times that of the hotter star. (a) What is the temperature of the hotter star in terms of \(T\) ? (b) What is the ratio of the peak-intensity wavelength of the hot star to the peak-intensity wavelength of the cool star?

Imagine another universe in which the value of Planck's constant is 0.0663 J \(\cdot\) s, but in which the physical laws and all other physical constants are the same as in our universe. In this universe, two physics students are playing catch. They are 12 m apart, and one throws a 0.25-kg ball directly toward the other with a speed of 6.0 m/s. (a) What is the uncertainty in the ball's horizontal momentum, in a direction perpendicular to that in which it is being thrown, if the student throwing the ball knows that it is located within a cube with volume 125 cm\(^3\) at the time she throws it? (b) By what horizontal distance could the ball miss the second student?

(a) For one-electron ions with nuclear charge Z, what is the speed of the electron in a Bohr-model orbit labeled with \(n\)? Give your answer in terms of \(v_1\), the orbital speed for the \(n\) = 1 Bohr orbit in hydrogen. (b) What is the largest value of Z for which the \(n\) = 1 orbital speed is less than 10\(\%\) of the speed of light in vacuum?

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