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-rw-r--r--3411/CH1/EX1.1/Ex1_1.sce12
-rw-r--r--3411/CH1/EX1.1/Ex1_1.txt1
-rw-r--r--3411/CH1/EX1.10/Ex1_10.sce11
-rw-r--r--3411/CH1/EX1.10/Ex1_10.txt1
-rw-r--r--3411/CH1/EX1.11/Ex1_11.sce8
-rw-r--r--3411/CH1/EX1.11/Ex1_11.txt1
-rw-r--r--3411/CH1/EX1.12/Ex1_12.sce14
-rw-r--r--3411/CH1/EX1.12/Ex1_12.txt1
-rw-r--r--3411/CH1/EX1.2/Ex1_2.sce15
-rw-r--r--3411/CH1/EX1.2/Ex1_2.txt1
-rw-r--r--3411/CH1/EX1.3/Ex1_3.sce19
-rw-r--r--3411/CH1/EX1.3/Ex1_3.txt2
-rw-r--r--3411/CH1/EX1.4/Ex1_4.sce14
-rw-r--r--3411/CH1/EX1.4/Ex1_4.txt1
-rw-r--r--3411/CH1/EX1.5/Ex1_5.sce11
-rw-r--r--3411/CH1/EX1.5/Ex1_5.txt1
-rw-r--r--3411/CH1/EX1.6/Ex1_6.sce26
-rw-r--r--3411/CH1/EX1.6/Ex1_6.txt5
-rw-r--r--3411/CH1/EX1.7/Ex1_7.sce12
-rw-r--r--3411/CH1/EX1.7/Ex1_7.txt1
-rw-r--r--3411/CH1/EX1.8/Ex1_8.sce10
-rw-r--r--3411/CH1/EX1.8/Ex1_8.txt1
-rw-r--r--3411/CH1/EX1.9/Ex1_9.sce14
-rw-r--r--3411/CH1/EX1.9/Ex1_9.txt1
24 files changed, 183 insertions, 0 deletions
diff --git a/3411/CH1/EX1.1/Ex1_1.sce b/3411/CH1/EX1.1/Ex1_1.sce
new file mode 100644
index 000000000..35a68a85b
--- /dev/null
+++ b/3411/CH1/EX1.1/Ex1_1.sce
@@ -0,0 +1,12 @@
+//Example 1.1
+clc();
+clear;
+//To calculate the location of screen from slits
+d=0.08 //units in cm
+d=d*10^-2 //units in mts
+betaa=6*10^-4 //units in mts
+v=8*10^11 //units in kHz
+c=3*10^8 //units in mts
+lamda=c/(v*10^3) //units in mts
+d=(betaa*d)/lamda //units in mts
+printf("The distance of the screen from the slits is %.2fmts",d)
diff --git a/3411/CH1/EX1.1/Ex1_1.txt b/3411/CH1/EX1.1/Ex1_1.txt
new file mode 100644
index 000000000..877edc1aa
--- /dev/null
+++ b/3411/CH1/EX1.1/Ex1_1.txt
@@ -0,0 +1 @@
+ The distance of the screen from the slits is 1.28mts \ No newline at end of file
diff --git a/3411/CH1/EX1.10/Ex1_10.sce b/3411/CH1/EX1.10/Ex1_10.sce
new file mode 100644
index 000000000..ea62936bc
--- /dev/null
+++ b/3411/CH1/EX1.10/Ex1_10.sce
@@ -0,0 +1,11 @@
+//Example 1.10
+clc();
+clear;
+//To find the diameter of the 20th dark ring
+D4=0.4 //units in cm
+D12=0.7 //units in cm
+//As we have (D20^2-D4^2)/(D12^2-D4^2)=(4*16)/(4*8)
+ans=(4*16)/(4*8)
+D20_2=(ans*((D12)^2-(D4)^2))+(D4)^2 //units in cm^2
+D20=sqrt(D20_2) //units in cm
+printf("Diameter of the 20th dark ring is %.3fcm",D20)
diff --git a/3411/CH1/EX1.10/Ex1_10.txt b/3411/CH1/EX1.10/Ex1_10.txt
new file mode 100644
index 000000000..935d8934e
--- /dev/null
+++ b/3411/CH1/EX1.10/Ex1_10.txt
@@ -0,0 +1 @@
+Diameter of the 20th dark ring is 0.906cm \ No newline at end of file
diff --git a/3411/CH1/EX1.11/Ex1_11.sce b/3411/CH1/EX1.11/Ex1_11.sce
new file mode 100644
index 000000000..a5e2eaadf
--- /dev/null
+++ b/3411/CH1/EX1.11/Ex1_11.sce
@@ -0,0 +1,8 @@
+//Example 1.11
+clc();
+clear;
+//To calculate refractive Index of liquid
+ d10=1.40
+ d_10=1.27
+ u=(d10/d_10)^2
+ printf("The refractive index of liquid is %.3f",u)
diff --git a/3411/CH1/EX1.11/Ex1_11.txt b/3411/CH1/EX1.11/Ex1_11.txt
new file mode 100644
index 000000000..77e40fa8b
--- /dev/null
+++ b/3411/CH1/EX1.11/Ex1_11.txt
@@ -0,0 +1 @@
+The refractive index of liquid is 1.215 \ No newline at end of file
diff --git a/3411/CH1/EX1.12/Ex1_12.sce b/3411/CH1/EX1.12/Ex1_12.sce
new file mode 100644
index 000000000..27043d537
--- /dev/null
+++ b/3411/CH1/EX1.12/Ex1_12.sce
@@ -0,0 +1,14 @@
+//Example 1.12
+clc();
+clear;
+//To calculate the wavelength of the light used
+Dnp=0.8 //units in cm
+Dn=0.3 //units in cm
+n1=25
+n2=5
+p=n1-n2
+R=100 //units in cm
+lamda=(Dnp^2-Dn^2)/(4*p*R) //units in cm
+printf("The wavelength of light used is %.8fcm",lamda)
+//In text book the answer is printed wrong as 4.87*10^-5cm
+//correct Answer is 6.875*10^-5cm
diff --git a/3411/CH1/EX1.12/Ex1_12.txt b/3411/CH1/EX1.12/Ex1_12.txt
new file mode 100644
index 000000000..077d048d1
--- /dev/null
+++ b/3411/CH1/EX1.12/Ex1_12.txt
@@ -0,0 +1 @@
+The wavelength of light used is 0.00006875cm \ No newline at end of file
diff --git a/3411/CH1/EX1.2/Ex1_2.sce b/3411/CH1/EX1.2/Ex1_2.sce
new file mode 100644
index 000000000..20c9c6298
--- /dev/null
+++ b/3411/CH1/EX1.2/Ex1_2.sce
@@ -0,0 +1,15 @@
+//Example 1.2
+clc();
+clear;
+//To calculate the wavelength
+//First case to calculte the wavelengths of the light source to obtain fringes 0.46*10^-2 mts
+lamda1=4200 //units in armstrongs
+lamda1=lamda1*10^-10 //units in mts
+betaa=0.64*10^-2 //units in mts
+D_d=betaa/lamda1 //units in mts
+//Second caseDistance between slits and screen is reduced to half
+beeta1=0.46*10^-2 //units in mts
+lamdaD_d=beeta1*2 //units in mts
+lamda=(lamda1*lamdaD_d)/betaa //units in mts
+lamda=lamda*10^10 //units in armstrongs
+printf("The wavelength of the Light source is %.1fArmstrongs",lamda)
diff --git a/3411/CH1/EX1.2/Ex1_2.txt b/3411/CH1/EX1.2/Ex1_2.txt
new file mode 100644
index 000000000..924cad728
--- /dev/null
+++ b/3411/CH1/EX1.2/Ex1_2.txt
@@ -0,0 +1 @@
+The wavelength of the Light source is 6037.5Armstrongs \ No newline at end of file
diff --git a/3411/CH1/EX1.3/Ex1_3.sce b/3411/CH1/EX1.3/Ex1_3.sce
new file mode 100644
index 000000000..a0e529224
--- /dev/null
+++ b/3411/CH1/EX1.3/Ex1_3.sce
@@ -0,0 +1,19 @@
+//Example 1.3
+clc();
+clear;
+//To compare the intensity at a point distance 1mm from the center to that at its center and to find minimum dist from center of point
+//Path difference=(Y*d)/D
+y=1 //units in mm
+y=y*10^-3 //units in mts
+D=1 //units in mts
+d=1 //units in mm
+d=d*10^-3 //units in mts
+pathdifference=(y*d)/D //units in mts
+lamda=5893 //units in armstrongs
+lamda=lamda*10^-10 //units in mts
+phasedifference=(2*pathdifference)/lamda //units in pi radiand
+ratioofintensity=(cos((phasedifference/2)*%pi))^2 //units in
+printf("The ratio of intensity with central maximum is %.4f\n",ratioofintensity)
+pathdifference=lamda/4
+distance=(pathdifference*D)/d //units in mts
+printf("The Distance of the point on the screen from center is %fmts",distance)
diff --git a/3411/CH1/EX1.3/Ex1_3.txt b/3411/CH1/EX1.3/Ex1_3.txt
new file mode 100644
index 000000000..9a5c604aa
--- /dev/null
+++ b/3411/CH1/EX1.3/Ex1_3.txt
@@ -0,0 +1,2 @@
+The ratio of intensity with central maximum is 0.3363
+The Distance of the point on the screen from center is 0.000147mts \ No newline at end of file
diff --git a/3411/CH1/EX1.4/Ex1_4.sce b/3411/CH1/EX1.4/Ex1_4.sce
new file mode 100644
index 000000000..407667f07
--- /dev/null
+++ b/3411/CH1/EX1.4/Ex1_4.sce
@@ -0,0 +1,14 @@
+//Example 1.4
+clc();
+clear;
+//To calculate thickness of plate
+//t=(n*lamda)/(u-u1)
+n=5
+u=1.7
+u1=1.4
+lamda=4800 //units in armstrongs
+lamda=lamda*10^-10 //units in mts
+t=(n*lamda)/(u-u1) //units in mts
+printf("Thickness of glass plate is %.6fmts",t)
+//In text book the answer is printed wrong as 8*10^-8 mts
+//the correct answer is 8*10^-6 mts
diff --git a/3411/CH1/EX1.4/Ex1_4.txt b/3411/CH1/EX1.4/Ex1_4.txt
new file mode 100644
index 000000000..1659250bd
--- /dev/null
+++ b/3411/CH1/EX1.4/Ex1_4.txt
@@ -0,0 +1 @@
+Thickness of glass plate is 0.000008mts \ No newline at end of file
diff --git a/3411/CH1/EX1.5/Ex1_5.sce b/3411/CH1/EX1.5/Ex1_5.sce
new file mode 100644
index 000000000..c211b994b
--- /dev/null
+++ b/3411/CH1/EX1.5/Ex1_5.sce
@@ -0,0 +1,11 @@
+//Example 1.5
+clc();
+clear;
+//To find the refractive index of coil
+volume=0.2 //units in CC
+thickness=volume/(100*100) //units in cm
+n=1
+lamda=5.5*10^-5 //units in cm
+r=0
+u=(n*lamda)/(2*thickness*cos(r))
+printf("Refractive index of oil is %.3f",u)
diff --git a/3411/CH1/EX1.5/Ex1_5.txt b/3411/CH1/EX1.5/Ex1_5.txt
new file mode 100644
index 000000000..9ae748b0b
--- /dev/null
+++ b/3411/CH1/EX1.5/Ex1_5.txt
@@ -0,0 +1 @@
+Refractive index of oil is 1.375 \ No newline at end of file
diff --git a/3411/CH1/EX1.6/Ex1_6.sce b/3411/CH1/EX1.6/Ex1_6.sce
new file mode 100644
index 000000000..99f489e0c
--- /dev/null
+++ b/3411/CH1/EX1.6/Ex1_6.sce
@@ -0,0 +1,26 @@
+//Example 1.6
+clc();
+clear;
+//Calculate the wavelengths of light in visible spectrum
+i=35 //units in degrees
+u=1.33
+d=5*10^-5 //units in cm
+r=asin(sin(i*%pi/180)/u) //units in radians
+r=r*180/%pi //units in degrees
+//For n=1
+n=1
+lamda1=(2*u*d*cos(r*%pi/180))/n //units in cm
+printf("For n=1 lamda=%.6fcm which lies in infrared region",lamda1)
+//For n=2
+n=2
+lamda2=(2*u*d*cos(r*%pi/180))/n //units in cm
+printf("\nFor n=2 lamda=%.6fcm which lies in visible region",lamda2)
+//For n=3
+n=3
+lamda3=(2*u*d*cos(r*%pi/180))/n //units in cm
+printf("\nFor n=3 lamda=%.6fcm which lies in visible region",lamda3)
+//For n=4
+n=4
+lamda4=(2*u*d*cos(r*%pi/180))/n //units in cm
+printf("\nFor n=4 lamda=%.6fcm which lies in ultraviolet region",lamda4)
+printf("\nHence absent wavelengths in reflected region are %.6fcm and %.6fcm",lamda2,lamda3)
diff --git a/3411/CH1/EX1.6/Ex1_6.txt b/3411/CH1/EX1.6/Ex1_6.txt
new file mode 100644
index 000000000..dfebdc2f5
--- /dev/null
+++ b/3411/CH1/EX1.6/Ex1_6.txt
@@ -0,0 +1,5 @@
+For n=1 lamda=0.000120cm which lies in infrared region
+For n=2 lamda=0.000060cm which lies in visible region
+For n=3 lamda=0.000040cm which lies in visible region
+For n=4 lamda=0.000030cm which lies in ultraviolet region
+Hence absent wavelengths in reflected region are 0.000060cm and 0.000040cm \ No newline at end of file
diff --git a/3411/CH1/EX1.7/Ex1_7.sce b/3411/CH1/EX1.7/Ex1_7.sce
new file mode 100644
index 000000000..1359ac720
--- /dev/null
+++ b/3411/CH1/EX1.7/Ex1_7.sce
@@ -0,0 +1,12 @@
+//Example1.7
+clc();
+clear;
+//To calculate the fring width
+//betaa=(lamda)/(2*alpha)
+lamda=6000 //units in armstrongs
+lamda=lamda*10^-8 //units in cm
+diameter=0.05 //units in mm
+distance=15 //units in cm
+alpha=(diameter/distance)*10^-1 //units in radians
+betaa=lamda/(2*alpha) //units in cm
+printf("The fringe width is %.2fcm",betaa)
diff --git a/3411/CH1/EX1.7/Ex1_7.txt b/3411/CH1/EX1.7/Ex1_7.txt
new file mode 100644
index 000000000..3303a42dc
--- /dev/null
+++ b/3411/CH1/EX1.7/Ex1_7.txt
@@ -0,0 +1 @@
+The fringe width is 0.09cm \ No newline at end of file
diff --git a/3411/CH1/EX1.8/Ex1_8.sce b/3411/CH1/EX1.8/Ex1_8.sce
new file mode 100644
index 000000000..3db76f95e
--- /dev/null
+++ b/3411/CH1/EX1.8/Ex1_8.sce
@@ -0,0 +1,10 @@
+//Example 1.8
+clc();
+clear;
+//To calculate the distance from the edge of wedge
+alpha=0.01 //units in radians
+n=10
+lamda=6000 //units in armstrongs
+lamda=lamda*10^-10 //units in mts
+x=((2*n-1)*lamda)/(4*alpha) //units in mts
+printf("Distance from the edge of the wedge is %.6fmts",x)
diff --git a/3411/CH1/EX1.8/Ex1_8.txt b/3411/CH1/EX1.8/Ex1_8.txt
new file mode 100644
index 000000000..9d7cad977
--- /dev/null
+++ b/3411/CH1/EX1.8/Ex1_8.txt
@@ -0,0 +1 @@
+Distance from the edge of the wedge is 0.000285mts \ No newline at end of file
diff --git a/3411/CH1/EX1.9/Ex1_9.sce b/3411/CH1/EX1.9/Ex1_9.sce
new file mode 100644
index 000000000..4ff832115
--- /dev/null
+++ b/3411/CH1/EX1.9/Ex1_9.sce
@@ -0,0 +1,14 @@
+//Example 1.9
+clc();
+clear;
+//To calculate diameter of the fifth bright ring
+n=5
+lamda=5460 //units in armstrongs
+lamda=lamda*10^-6 //units in cm
+f=400 //units in cm
+u=1.5
+R=(u-1)*2*f //units in cm
+diameter=sqrt(2*(2*n-1)*lamda*R)
+printf("Diameter of the 5th bright ring is %.4fcm",diameter)
+//In text book the answer is printed wrong as 0.627cm
+//The correct answer is 6.269 cms
diff --git a/3411/CH1/EX1.9/Ex1_9.txt b/3411/CH1/EX1.9/Ex1_9.txt
new file mode 100644
index 000000000..399401da9
--- /dev/null
+++ b/3411/CH1/EX1.9/Ex1_9.txt
@@ -0,0 +1 @@
+Diameter of the 5th bright ring is 6.2699cm \ No newline at end of file
generated by cgit (git 2.34.1) at 2024-12-19 17:58:56 +0000