Browse By Unit
Daniella Garcia-Loos
Saarah Hasan
Daniella Garcia-Loos
Saarah Hasan
We've all heard of Einstein's famous equation, E=(Δm)c^2. In this lesson, we'll be going over how it can be used to calculate the mass equivalent for a given amount of energy transfer or an energy equivalent for a given amount of mass change.
Binding energy is the energy required to separate the particles in a system from each other. It is a measure of the strength of the forces that hold the particles together.
Here are some key points about binding energy:
Since atoms are so, so small, we need small units. We use the atomic mass unit (amu/u), which is defined as 1/12 the mass of a carbon-12 nucleus. 1u=1.6605∗10−^22^7 kg7kg. m_p=1.00728u
m_n=1.00867u
Let’s look at the helium-4 nucleus; it contains 2 protons and 2 neutrons-the predicted would be 4.0330 u. But the experimental mass of the helium-4 nucleus is 4.0026 u: this difference of 0.0304 u is called the mass defect and is proportional to the binding energy of the nucleus (E=mc^2).
Einstein’s special theory of relativity tells us that the mass can be converted to energy; the energy equivalent of 1 u=931.5 MeV. The binding energy of any nucleus is therefore determined by the relationship: BE(MeV) = Mass Defect * 931.5 MeV/uBE(MeV)=MassDefect∗931.5MeV/u Avg BE= BE/A AvgBE=BE/A where AA = the mass number of the element
The greater the average binding energy, the greater the stability of the nucleus.
Some information on fission and fusion:
Here are some key points about fission and fusion:
(A) I only (B) III only (C) I and II only (D) II and III only (E) I, II, and III
Answer:
<< Hide Menu
Daniella Garcia-Loos
Saarah Hasan
Daniella Garcia-Loos
Saarah Hasan
We've all heard of Einstein's famous equation, E=(Δm)c^2. In this lesson, we'll be going over how it can be used to calculate the mass equivalent for a given amount of energy transfer or an energy equivalent for a given amount of mass change.
Binding energy is the energy required to separate the particles in a system from each other. It is a measure of the strength of the forces that hold the particles together.
Here are some key points about binding energy:
Since atoms are so, so small, we need small units. We use the atomic mass unit (amu/u), which is defined as 1/12 the mass of a carbon-12 nucleus. 1u=1.6605∗10−^22^7 kg7kg. m_p=1.00728u
m_n=1.00867u
Let’s look at the helium-4 nucleus; it contains 2 protons and 2 neutrons-the predicted would be 4.0330 u. But the experimental mass of the helium-4 nucleus is 4.0026 u: this difference of 0.0304 u is called the mass defect and is proportional to the binding energy of the nucleus (E=mc^2).
Einstein’s special theory of relativity tells us that the mass can be converted to energy; the energy equivalent of 1 u=931.5 MeV. The binding energy of any nucleus is therefore determined by the relationship: BE(MeV) = Mass Defect * 931.5 MeV/uBE(MeV)=MassDefect∗931.5MeV/u Avg BE= BE/A AvgBE=BE/A where AA = the mass number of the element
The greater the average binding energy, the greater the stability of the nucleus.
Some information on fission and fusion:
Here are some key points about fission and fusion:
(A) I only (B) III only (C) I and II only (D) II and III only (E) I, II, and III
Answer:
© 2024 Fiveable Inc. All rights reserved.