Chapter 18: Problem 2471
A nucleus of \({ }^{210}{ }_{84}\) Po originally at rest emits \(\alpha\) -particle with speed \(\mathrm{v}\) what will be the recoil speed of the daughter nucleus (A) \([\mathrm{v} /(214)]\) (B) \([(4 \mathrm{v}) /(214)]\) (C) \([(4 \mathrm{v}) /(206)]\) (D) \([\mathrm{v} /(206)]\)
Short Answer
Expert verified
The recoil speed of the daughter nucleus is (C) \([(4 \mathrm{v}) /(206)]\).
Step by step solution
01
Identify the given information
Given information:
1. The initial nucleus is Po-210: It has 210 nucleons and 84 protons (mass number A = 210; atomic number Z = 84)
2. An α-particle is emitted: An α-particle consists of 2 protons and 2 neutrons (mass number A = 4; atomic number Z = 2)
3. The speed of the emitted α-particle is v
02
Calculate the mass of the daughter nucleus
Since the α-particle has a mass number of 4, the mass number of the daughter nucleus is the difference between the parent nucleus and the α-particle:
A_daughter = A_parent - A_alpha = 210 - 4 = 206
The daughter nucleus has 206 nucleons and 82 protons (mass number A = 206; atomic number Z = 82)
03
Apply the conservation of momentum principle
Before the α-particle emission, the system is at rest, and its total linear momentum is zero. After the emission, the sum of the linear momentum of the α-particle and daughter nucleus should still be zero.
Let v_daughter be the recoil speed of the daughter nucleus. Then, applying the conservation of momentum principle:
\(mass_{daughter} \cdot v_{daughter} = mass_{alpha} \cdot v_{alpha}\)
Since the masses of the α-particle and daughter nucleus are proportional to their mass numbers, we can rewrite the equation as:
\(A_{daughter} \cdot v_{daughter} = A_{alpha} \cdot v_{alpha}\)
04
Solve for the recoil speed of the daughter nucleus
Now we can solve for v_daughter:
\(v_{daughter} = (A_{alpha} \cdot v_{alpha}) / A_{daughter}\)
Substitute the values we found earlier:
\(v_{daughter} = (4 \cdot v) / 206\)
Comparing this to the given answer choices, we find that the correct answer is:
(C) \([(4 \mathrm{v}) /(206)]\)
Unlock Step-by-Step Solutions & Ace Your Exams!
-
Full Textbook Solutions
Get detailed explanations and key concepts
-
Unlimited Al creation
Al flashcards, explanations, exams and more...
-
Ads-free access
To over 500 millions flashcards
-
Money-back guarantee
We refund you if you fail your exam.
Over 30 million students worldwide already upgrade their learning with Vaia!
Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Momentum Conservation
In physics, the principle of momentum conservation is fundamental when analyzing collisions and decays, including nuclear decays. In a closed system with no external forces, the total momentum before an event is equal to the total momentum after the event. This principle helps to determine unknown velocities after interactions, such as the emission of particles during nuclear decay.
For example, in the decay of a nucleus where an alpha particle is emitted, the system initially is at rest, meaning its total momentum is zero. When the alpha particle is emitted, it gains momentum. To conserve the total momentum of the system, the remaining daughter nucleus must also have an equal and opposite momentum. This ensures momentum conservation overall, balancing the initial state where no motion or external forces were present.
Understanding this principle helps predict the resulting speed and direction of nuclei or particles involved in nuclear reactions and can be calculated by equating the momentum of the emitted particle to the momentum of the recoiling nucleus.
For example, in the decay of a nucleus where an alpha particle is emitted, the system initially is at rest, meaning its total momentum is zero. When the alpha particle is emitted, it gains momentum. To conserve the total momentum of the system, the remaining daughter nucleus must also have an equal and opposite momentum. This ensures momentum conservation overall, balancing the initial state where no motion or external forces were present.
Understanding this principle helps predict the resulting speed and direction of nuclei or particles involved in nuclear reactions and can be calculated by equating the momentum of the emitted particle to the momentum of the recoiling nucleus.
Alpha Particle Emission
Alpha particle emission is a type of nuclear decay where an unstable nucleus releases an alpha particle to become more stable. An alpha particle is essentially a helium nucleus, consisting of two protons and two neutrons, and carries a positive charge.
When a nucleus emits an alpha particle:
When a nucleus emits an alpha particle:
- It reduces its atomic mass by 4 units (since the alpha particle itself has a mass number of 4).
- It reduces its atomic number by 2, changing the element to a different one in the periodic table.
- The original nucleus becomes the 'daughter nucleus' post-decay.
Daughter Nucleus
When a nucleus undergoes a process like alpha decay, the original nucleus transforms into a different nucleus known as the daughter nucleus.
- The mass number of the daughter nucleus is reduced from the original by 4, reflecting the mass of the alpha particle emitted.
- The atomic number decreases by 2 due to the loss of two protons as part of the alpha particle.
- In addition to the change in atomic composition, the daughter nucleus often gains additional stability and sits as a lower-energy state compared to its parent.
Recoil Speed Calculation
Calculating the recoil speed of a daughter nucleus is a vital step when analyzing nuclear decays, using the principle of conservation of momentum. Consider the scenario where a nucleus emits an alpha particle.
- Initially, the nucleus is at rest, so total momentum before the emission is zero.
- Upon emission, the alpha particle gains speed and momentum in one direction, requiring the daughter nucleus to move in the opposite direction to conserve total momentum.
- \(A_{\text{alpha}}\) is the mass number of the alpha particle.
- \(v_{\alpha}\) is the speed of the alpha particle.
- \(A_{\text{daughter}}\) is the mass number of the daughter nucleus after emission.