The flux density at a point in space is given by B = 4xaₓ + 2kya + 8a Wb/m² . The value of constant k must be equal to
- A-2
- B-0.5
- C+0.5
- D+2
Solution & Step-by-step Explanation
Magnetic Flux Density Field Analysis
The question asks us to find the value of a constant, k, within a given magnetic flux density vector field. The magnetic flux density, denoted by , describes the strength and direction of a magnetic field. A fundamental property of all magnetic fields in physics is that they are solenoidal. This means that the magnetic field lines do not start or end at any point; they always form closed loops.
Understanding the Solenoidal Property
Mathematically, the solenoidal property is expressed using the divergence theorem. For any magnetic flux density field , its divergence must be zero:
This equation is one of Maxwell's equations and is crucial for solving problems involving magnetic fields. We will use this principle to find the value of k.
Step 1: Identify the Components of B
The given magnetic flux density vector is:
From this vector equation, we can identify the components of the magnetic flux density field:
- The x-component is
- The y-component is
- The z-component is
Step 2: Calculate the Divergence of B
The divergence of a vector field in Cartesian coordinates is given by:
Applying this formula to our magnetic flux density field :
Step 3: Compute the Partial Derivatives
Now, we compute the partial derivative of each component with respect to its corresponding coordinate:
- Derivative of with respect to x:
- Derivative of with respect to y:
- Derivative of with respect to z: (The derivative of a constant is zero)
Step 4: Solve for the Constant k
Substitute the computed partial derivatives back into the divergence equation and set it equal to zero, based on the solenoidal property ():
Now, we solve this equation for k:
Conclusion
Therefore, the value of the constant k that satisfies the condition for a magnetic flux density field is -2.
The question asks us to find the value of a constant, k, within a given magnetic flux density vector field. The magnetic flux density, denoted by , describes the strength and direction of a magnetic field. A fundamental property of all magnetic fields in physics is that they are solenoidal. This means that the magnetic field lines do not start or end at any point; they always form closed loops.
Understanding the Solenoidal Property
Mathematically, the solenoidal property is expressed using the divergence theorem. For any magnetic flux density field , its divergence must be zero:
This equation is one of Maxwell's equations and is crucial for solving problems involving magnetic fields. We will use this principle to find the value of k.
Step 1: Identify the Components of B
The given magnetic flux density vector is:
From this vector equation, we can identify the components of the magnetic flux density field:
- The x-component is
- The y-component is
- The z-component is
Step 2: Calculate the Divergence of B
The divergence of a vector field in Cartesian coordinates is given by:
Applying this formula to our magnetic flux density field :
Step 3: Compute the Partial Derivatives
Now, we compute the partial derivative of each component with respect to its corresponding coordinate:
- Derivative of with respect to x:
- Derivative of with respect to y:
- Derivative of with respect to z: (The derivative of a constant is zero)
Step 4: Solve for the Constant k
Substitute the computed partial derivatives back into the divergence equation and set it equal to zero, based on the solenoidal property ():
Now, we solve this equation for k:
Conclusion
Therefore, the value of the constant k that satisfies the condition for a magnetic flux density field is -2.