Give step-by-step solution with explanation and final answer:Question 4: (10 points) Let F(z,y,2) = (z arctan(y?), * In(a® + 1),4%2). Find the flux of F across the surface S, which is part of 2% + y + z = 2 that lies above the plane z = 1 and is oriented upward.
Question:
Give step-by-step solution with explanation and final answer:
Question 4: (10 points)
Let F(z,y,2) = (z arctan(y?), * In(a® + 1),4%2). Find the flux of F
across the surface S, which is part of 2% + y + z = 2 that lies above
the plane z = 1 and is oriented upward.
This is AI generated Response.
Asked by: gvr
Created at: 2025-06-12 04:37:14
Asked by: gvr
Created at: 2025-06-12 04:37:14
Final Answer:
Rendered
Raw Text
Did you like this answer?
Let's solve the problem step by step:
### **Step 1: Write the Problem Clearly**
Given:
\[
\mathbf{F}(x, y, z) = \left(z \arctan(y^2),\ z^3 \ln(x^2 + 1),\ x^2 z\right)
\]
Surface \( S \): Part of \( x^2 + y^2 + z = 2 \) **above** \( z = 1 \), oriented **upward**.
We are to find the **flux** of \( \mathbf{F} \) **across \( S \)**.
---
### **Step 2: Surface and Its Projection**
The surface \( S \) is given by:
\[
z = 2 - x^2 - y^2, \quad \text{with } z \geq 1
\]
So,
\[
2 - x^2 - y^2 \geq 1 \implies x^2 + y^2 \leq 1
\]
Thus, the projection \( D \) on the \( xy \)-plane is the disk \( x^2 + y^2 \leq 1 \).
---
### **Step 3: Find the Upward Unit Normal Vector**
For a surface \( z = f(x, y) \), the upward normal is:
\[
\mathbf{n} = \frac{(-f_x, -f_y, 1)}{\sqrt{f_x^2 + f_y^2 + 1}}
\]
But for flux, we use the surface integral:
\[
\iint_S \mathbf{F} \cdot d\mathbf{S} = \iint_D \mathbf{F}(x, y, f(x, y)) \cdot \mathbf{n} \, dA
\]
Or, equivalently,
\[
\iint_D \left[ \mathbf{F}(x, y, f(x, y)) \cdot (-f_x, -f_y, 1) \right] dA
\]
For \( z = 2 - x^2 - y^2 \):
\[
f_x = -2x,\quad f_y = -2y
\]
So, \( (-f_x, -f_y, 1) = (2x, 2y, 1) \).
---
### **Step 4: Substitute \( z \) and Compute the Dot Product**
Evaluate \( \mathbf{F}(x, y, z) \) at \( z = 2 - x^2 - y^2 \):
- \( z = 2 - x^2 - y^2 \)
- \( F_1 = z \arctan(y^2) \)
- \( F_2 = z^3 \ln(x^2 + 1) \)
- \( F_3 = x^2 z \)
So,
\[
\mathbf{F}(x, y, z) = \left((2 - x^2 - y^2)\arctan(y^2),\ (2 - x^2 - y^2)^3 \ln(x^2 + 1),\ x^2 (2 - x^2 - y^2)\right)
\]
Dot product with \( (2x, 2y, 1) \):
\[
\begin{align*}
&\mathbf{F} \cdot (2x, 2y, 1) \\
=& 2x (2 - x^2 - y^2)\arctan(y^2) + 2y (2 - x^2 - y^2)^3 \ln(x^2 + 1) + x^2(2 - x^2 - y^2)
\end{align*}
\]
---
### **Step 5: Write the Flux Integral**
\[
\iint_D \left[ 2x (2 - x^2 - y^2)\arctan(y^2) + 2y (2 - x^2 - y^2)^3 \ln(x^2 + 1) + x^2(2 - x^2 - y^2) \right] dA
\]
where \( D: x^2 + y^2 \leq 1 \).
---
### **Step 6: Change to Polar Coordinates**
Let \( x = r\cos\theta, y = r\sin\theta \), \( dA = r dr d\theta \), \( r \in [0, 1], \theta \in [0, 2\pi] \).
- \( x^2 + y^2 = r^2 \)
- \( x = r\cos\theta \)
- \( y = r\sin\theta \)
So, the terms become:
1. \( 2x (2 - x^2 - y^2) \arctan(y^2) = 2r\cos\theta (2 - r^2)\arctan(r^2\sin^2\theta) \)
2. \( 2y (2 - x^2 - y^2)^3 \ln(x^2 + 1) = 2r\sin\theta (2 - r^2)^3 \ln(r^2\cos^2\theta + 1) \)
3. \( x^2(2 - x^2 - y^2) = r^2\cos^2\theta (2 - r^2) \)
---
### **Step 7: Integrate Each Term**
#### **First Two Terms:**
Notice that integrating any function that is **odd** in \( x \) or \( y \) over a disk centered at the origin will yield **zero**.
- \( x \) and \( y \) are odd functions.
- The disk \( D \) is symmetric about the origin.
- The first and second terms are odd in \( x \) and \( y \), respectively.
So, the integrals of the first two terms over the disk are **zero**.
#### **Only Third Term Remains:**
\[
\iint_D x^2(2 - x^2 - y^2)\ dA
\]
In polar coordinates:
\[
\int_0^{2\pi} \int_0^1 r^2\cos^2\theta (2 - r^2) r dr d\theta
\]
---
### **Step 8: Compute the Remaining Integral**
\[
\int_0^{2\pi} \int_0^1 r^2\cos^2\theta (2 - r^2) r dr d\theta
= \int_0^{2\pi} \cos^2\theta\ d\theta \int_0^1 r^3 (2 - r^2) dr
\]
Compute the \( r \) integral:
\[
\int_0^1 r^3 (2 - r^2) dr = 2\int_0^1 r^3 dr - \int_0^1 r^5 dr = 2\left[\frac{r^4}{4}\right]_0^1 - \left[\frac{r^6}{6}\right]_0^1 = 2 \left(\frac{1}{4}\right) - \left(\frac{1}{6}\right) = \frac{1}{2} - \frac{1}{6} = \frac{1}{3}
\]
Now, the \( \theta \) integral:
\[
\int_0^{2\pi} \cos^2\theta\ d\theta = \int_0^{2\pi} \frac{1+\cos 2\theta}{2} d\theta = \frac{1}{2}\int_0^{2\pi} 1 d\theta + \frac{1}{2} \int_0^{2\pi} \cos 2\theta d\theta = \frac{1}{2}(2\pi) + 0 = \pi
\]
---
### **Step 9: Final Answer**
Multiply the two results:
\[
\text{Flux} = \pi \times \frac{1}{3} = \boxed{\frac{\pi}{3}}
\]
---
## **Final Answer**
\[
\boxed{\frac{\pi}{3}}
\]
Question:
i need detailed calculations along with the final Answer
This is AI generated Response.
Asked by: gvr
Created at: 2025-06-12 04:38:35
Asked by: gvr
Created at: 2025-06-12 04:38:35
Final Answer:
Rendered
Raw Text
Did you like this answer?
Let's carefully solve the problem step by step, including all detailed calculations.
---
### **Given Data:**
- Vector field:
\[
\mathbf{F}(x, y, z) = \left(z \arctan(y^2),\ z^3 \ln(x^2 + 1),\ x^2 z\right)
\]
- Surface \( S \): part of the paraboloid
\[
z = 2 - x^2 - y^2
\]
lying **above** the plane \( z = 1 \), with upward orientation.
---
### **Step 1: Describe the Surface and Its Projection**
The surface \( z = 2 - x^2 - y^2 \) is a downward-opening paraboloid.
- The portion above \( z=1 \):
\[
2 - x^2 - y^2 \geq 1 \Rightarrow x^2 + y^2 \leq 1
\]
So, the projection \( D \) in the \( xy \)-plane is the disk:
\[
x^2 + y^2 \leq 1
\]
---
### **Step 2: Surface Element and Normal Vector**
For a surface \( z = f(x, y) = 2 - x^2 - y^2 \),
- The upward normal vector is given by:
\[
\mathbf{n} = \frac{(-f_x, -f_y, 1)}{\sqrt{f_x^2 + f_y^2 + 1}}
\]
- The differential surface element:
\[
d\mathbf{S} = \mathbf{n} \, dA = \frac{(-f_x, -f_y, 1)}{\sqrt{f_x^2 + f_y^2 + 1}} \, dA
\]
However, for flux calculation, it's often easier to use the surface integral in the form:
\[
\iint_S \mathbf{F} \cdot d\mathbf{S} = \iint_D \mathbf{F}(x, y, f(x,y)) \cdot \mathbf{n} \, dA
\]
Or, directly:
\[
\iint_D \mathbf{F}(x, y, f(x,y)) \cdot (-f_x, -f_y, 1) \, dA
\]
since the normal points upward.
---
### **Step 3: Compute derivatives \(f_x\) and \(f_y\)**
\[
f_x = -2x, \quad f_y = -2y
\]
Thus, the upward normal vector components (without normalization) are:
\[
(-f_x, -f_y, 1) = (2x, 2y, 1)
\]
---
### **Step 4: Evaluate \( \mathbf{F} \) at \( z = f(x,y) \)**
\[
z = 2 - x^2 - y^2
\]
Compute each component:
- \(F_1 = z \arctan(y^2) = (2 - x^2 - y^2) \arctan(y^2)\)
- \(F_2 = z^3 \ln(x^2 + 1) = (2 - x^2 - y^2)^3 \ln(x^2 + 1)\)
- \(F_3 = x^2 z = x^2 (2 - x^2 - y^2)\)
---
### **Step 5: Set up the flux integral**
\[
\text{Flux} = \iint_D \left[ \mathbf{F} \cdot (2x, 2y, 1) \right] dA
\]
Explicitly:
\[
\text{Flux} = \iint_D \left[ F_1 \cdot 2x + F_2 \cdot 2y + F_3 \cdot 1 \right] dA
\]
Substitute:
\[
\begin{aligned}
\text{Flux} &= \iint_D \left[ (2 - x^2 - y^2) \arctan(y^2) \cdot 2x \right. \\
&\quad + \left. (2 - x^2 - y^2)^3 \ln(x^2 + 1) \cdot 2y + x^2 (2 - x^2 - y^2) \right] dA
\end{aligned}
\]
---
### **Step 6: Symmetry considerations**
- The terms involving \( x \arctan(y^2) \) and \( y \ln(x^2 + 1) \) are **odd** functions in \( x \) or \( y \) over a symmetric disk centered at the origin.
- When integrating over the disk \( x^2 + y^2 \leq 1 \), integrals of odd functions across symmetric limits are zero.
**Therefore:**
\[
\iint_D 2x (2 - x^2 - y^2) \arctan(y^2) dA = 0
\]
and
\[
\iint_D 2y (2 - x^2 - y^2)^3 \ln(x^2 + 1) dA = 0
\]
The remaining term is:
\[
\iint_D x^2 (2 - x^2 - y^2) dA
\]
---
### **Step 7: Convert remaining integral to polar coordinates**
In polar coordinates:
\[
x = r \cos \theta,\quad y = r \sin \theta,\quad dA = r dr d\theta
\]
Also:
\[
x^2 = r^2 \cos^2 \theta,\quad x^2 + y^2 = r^2
\]
The integral becomes:
\[
\text{Flux} = \int_0^{2\pi} \int_0^1 r^2 \cos^2 \theta \cdot (2 - r^2) \cdot r dr d\theta
\]
which simplifies to:
\[
\int_0^{2\pi} \cos^2 \theta \, d\theta \times \int_0^1 r^3 (2 - r^2) dr
\]
---
### **Step 8: Compute angular integral**
\[
\int_0^{2\pi} \cos^2 \theta d\theta = \pi
\]
(using the standard integral \( \int_0^{2\pi} \cos^2 \theta d\theta = \pi \))
---
### **Step 9: Compute radial integral**
\[
\int_0^1 r^3 (2 - r^2) dr = 2 \int_0^1 r^3 dr - \int_0^1 r^5 dr
\]
Calculate each:
\[
\int_0^1 r^3 dr = \left[\frac{r^4}{4}\right]_0^1 = \frac{1}{4}
\]
\[
\int_0^1 r^5 dr = \left[\frac{r^6}{6}\right]_0^1 = \frac{1}{6}
\]
So:
\[
2 \times \frac{1}{4} - \frac{1}{6} = \frac{1}{2} - \frac{1}{6} = \frac{3}{6} - \frac{1}{6} = \frac{2}{6} = \frac{1}{3}
\]
---
### **Step 10: Final result**
Multiply angular and radial integrals:
\[
\text{Flux} = \pi \times \frac{1}{3} = \boxed{\frac{\pi}{3}}
\]
---
### **### **Final Answer:**
\[
\boxed{\frac{\pi}{3}}
\]
This is the flux of the vector field \( \mathbf{F} \) across the specified surface \( S \).
📢 Instructions:
- Ask anything relatd to above question only.
- For new Question goto :
VIPSolutions