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author | debashisdeb | 2014-06-20 15:42:42 +0530 |
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committer | debashisdeb | 2014-06-20 15:42:42 +0530 |
commit | 83c1bfceb1b681b4bb7253b47491be2d8b2014a1 (patch) | |
tree | f54eab21dd3d725d64a495fcd47c00d37abed004 /Engineering_Physics/Chapter3_1.ipynb | |
parent | a78126bbe4443e9526a64df9d8245c4af8843044 (diff) | |
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removing problem statements
Diffstat (limited to 'Engineering_Physics/Chapter3_1.ipynb')
-rw-r--r-- | Engineering_Physics/Chapter3_1.ipynb | 294 |
1 files changed, 261 insertions, 33 deletions
diff --git a/Engineering_Physics/Chapter3_1.ipynb b/Engineering_Physics/Chapter3_1.ipynb index e20ce99f..7f02f8be 100644 --- a/Engineering_Physics/Chapter3_1.ipynb +++ b/Engineering_Physics/Chapter3_1.ipynb @@ -1,6 +1,7 @@ { "metadata": { - "name": "Chapter3" + "name": "", + "signature": "sha256:366ab969956cd234404db0091b17960805856ec3ff44007e36b0efdbe1414f5e" }, "nbformat": 3, "nbformat_minor": 0, @@ -11,25 +12,51 @@ "cell_type": "heading", "level": 1, "metadata": {}, - "source": "3: Interference" + "source": [ + "3: Interference" + ] }, { "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.1, Page number 71" + "source": [ + "Example number 3.1, Page number 71" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the velocity of light\n\n#importing modules\nfrom __future__ import division\nimport math\n\n#Variable declaration\nbeta = 0.51; #Fringe width(mm)\nd = 2.2; #Distance between the slits(mm)\nD = 2; #Distance between the slits and the screen(m)\n\n#Calculation\nbeta = beta*10**-1; #Fringe width(cm)\nd = d*10**-1; #Distance between the slits(cm)\nD=D*10**2; #Distance between the slits and the screen(cm)\nlamda = beta*d/D; #Wavelength of light(cm)\nlamda = lamda*10**8; #Wavelength of light(A)\n\n#Result\nprint \"The wavelength of light is\",lamda, \"angstrom\"", + "input": [ + " \n", + "#importing modules\n", + "from __future__ import division\n", + "import math\n", + "\n", + "#Variable declaration\n", + "beta = 0.51; #Fringe width(mm)\n", + "d = 2.2; #Distance between the slits(mm)\n", + "D = 2; #Distance between the slits and the screen(m)\n", + "\n", + "#Calculation\n", + "beta = beta*10**-1; #Fringe width(cm)\n", + "d = d*10**-1; #Distance between the slits(cm)\n", + "D=D*10**2; #Distance between the slits and the screen(cm)\n", + "lamda = beta*d/D; #Wavelength of light(cm)\n", + "lamda = lamda*10**8; #Wavelength of light(A)\n", + "\n", + "#Result\n", + "print \"The wavelength of light is\",lamda, \"angstrom\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The wavelength of light is 5610.0 angstrom\n" + "text": [ + "The wavelength of light is 5610.0 angstrom\n" + ] } ], "prompt_number": 4 @@ -38,19 +65,47 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.2, Page number 71" + "source": [ + "Example number 3.2, Page number 71" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the seperation between the third fringe\n\n#importing modules\nfrom __future__ import division\nimport math\n\n#Variable declaration\nlambda1 = 4250; #First wavelength emitted by source of light(A)\nlambda2 = 5050; #Second wavelength emitted by source of light(A)\nD = 1.5; #Distance between the source and the screen(m)\nd = 0.025; #Distance between the slits(mm)\nn = 3; #Number of fringe from the centre\n\n#Calculation\nlambda1 = lambda1*10**-10; #First wavelength emitted(m)\nlambda2 = lambda2*10**-10; #Second wavelength emitted(m)\nd = d*10**-3; #Distance between the slits(m)\nx3 = n*lambda1*D/d; #Position of third bright fringe due to lambda1(m)\nx3_prime = n*lambda2*D/d; #Position of third bright fringe due to lambda2(m)\nx = x3_prime-x3; #separation between the third bright fringe(m)\nx = x*10**2; #separation between the third bright fringe(cm)\n\n#Result\nprint \"The separation between the third bright fringe due to the two wavelengths is\",x, \"cm\"\n", + "input": [ + " \n", + "#importing modules\n", + "from __future__ import division\n", + "import math\n", + "\n", + "#Variable declaration\n", + "lambda1 = 4250; #First wavelength emitted by source of light(A)\n", + "lambda2 = 5050; #Second wavelength emitted by source of light(A)\n", + "D = 1.5; #Distance between the source and the screen(m)\n", + "d = 0.025; #Distance between the slits(mm)\n", + "n = 3; #Number of fringe from the centre\n", + "\n", + "#Calculation\n", + "lambda1 = lambda1*10**-10; #First wavelength emitted(m)\n", + "lambda2 = lambda2*10**-10; #Second wavelength emitted(m)\n", + "d = d*10**-3; #Distance between the slits(m)\n", + "x3 = n*lambda1*D/d; #Position of third bright fringe due to lambda1(m)\n", + "x3_prime = n*lambda2*D/d; #Position of third bright fringe due to lambda2(m)\n", + "x = x3_prime-x3; #separation between the third bright fringe(m)\n", + "x = x*10**2; #separation between the third bright fringe(cm)\n", + "\n", + "#Result\n", + "print \"The separation between the third bright fringe due to the two wavelengths is\",x, \"cm\"\n" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The separation between the third bright fringe due to the two wavelengths is 1.44 cm\n" + "text": [ + "The separation between the third bright fringe due to the two wavelengths is 1.44 cm\n" + ] } ], "prompt_number": 5 @@ -59,19 +114,40 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.3, Page number 71" + "source": [ + "Example number 3.3, Page number 71" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the refractive index of the sheet of glass\n\n#importing modules\nimport math\n\n#Variable declaration\nlamda = 5.5*10**-5; #Wavelength emitted by source of light(cm)\nn = 4; #Number of fringes shifted\nt = 3.9*10**-4; #Thickness of the thin glass sheet(cm)\n\n#Calculation\nmew = (n*lamda/t)+1; #Refractive index of the sheet of glass\nmew = math.ceil(mew*10**4)/10**4; #rounding off the value of v to 4 decimals\n\n#Result\nprint \"The refractive index of the sheet of glass is\",mew", + "input": [ + " \n", + " \n", + "#importing modules\n", + "import math\n", + "\n", + "#Variable declaration\n", + "lamda = 5.5*10**-5; #Wavelength emitted by source of light(cm)\n", + "n = 4; #Number of fringes shifted\n", + "t = 3.9*10**-4; #Thickness of the thin glass sheet(cm)\n", + "\n", + "#Calculation\n", + "mew = (n*lamda/t)+1; #Refractive index of the sheet of glass\n", + "mew = math.ceil(mew*10**4)/10**4; #rounding off the value of v to 4 decimals\n", + "\n", + "#Result\n", + "print \"The refractive index of the sheet of glass is\",mew" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The refractive index of the sheet of glass is 1.5642\n" + "text": [ + "The refractive index of the sheet of glass is 1.5642\n" + ] } ], "prompt_number": 6 @@ -80,19 +156,46 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.4, Page number 72" + "source": [ + "Example number 3.4, Page number 72" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the least thickness of the film that appears bright and dark\n\n#importing modules\nimport math\n\n#Variable declaration\nlamda = 5893; #Wavelength of monochromatic lihgt used(A)\nn = 1; #Number of fringe for the least thickness of the film\ncosr = 1; #for normal incidence\nmew = 1.42; #refractive index of the soap film\n\n#Calculation\n#As for constructive interference, \n#2*mew*t*cos(r) = (2*n-1)*lambda/2, solving for t\nt = (2*n-1)*lamda/(4*mew*cosr); #Thickness of the film that appears bright(A)\n#As for destructive interference, \n#2*mu*t*cos(r) = n*lambda, solving for t\nt1 = n*lamda/(2*mew*cosr); #Thickness of the film that appears bright(A)\n\n#Result\nprint \"The thickness of the film that appears bright is\",t, \"angstrom\"\nprint \"The thickness of the film that appears dark is\",t1, \"angstrom\"", + "input": [ + " \n", + "#importing modules\n", + "import math\n", + "\n", + "#Variable declaration\n", + "lamda = 5893; #Wavelength of monochromatic lihgt used(A)\n", + "n = 1; #Number of fringe for the least thickness of the film\n", + "cosr = 1; #for normal incidence\n", + "mew = 1.42; #refractive index of the soap film\n", + "\n", + "#Calculation\n", + "#As for constructive interference, \n", + "#2*mew*t*cos(r) = (2*n-1)*lambda/2, solving for t\n", + "t = (2*n-1)*lamda/(4*mew*cosr); #Thickness of the film that appears bright(A)\n", + "#As for destructive interference, \n", + "#2*mu*t*cos(r) = n*lambda, solving for t\n", + "t1 = n*lamda/(2*mew*cosr); #Thickness of the film that appears bright(A)\n", + "\n", + "#Result\n", + "print \"The thickness of the film that appears bright is\",t, \"angstrom\"\n", + "print \"The thickness of the film that appears dark is\",t1, \"angstrom\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The thickness of the film that appears bright is 1037.5 angstrom\nThe thickness of the film that appears dark is 2075.0 angstrom\n" + "text": [ + "The thickness of the film that appears bright is 1037.5 angstrom\n", + "The thickness of the film that appears dark is 2075.0 angstrom\n" + ] } ], "prompt_number": 7 @@ -101,19 +204,42 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.5, Page number 72" + "source": [ + "Example number 3.5, Page number 72" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the angle of the wedge\n\n#importing modules\nimport math\n\n#Variable declaration\nlamda = 5893; #Wavelength of monochromatic lihgt used(A)\nn = 10; #Number of fringe that are found \nd = 1; #Distance of 10 fringes(cm)\n\n#Calculation\nbeta = d/n; #Fringe width(cm)\nlamda = lamda*10**-8; #Wavelength of monochromatic lihgt used(cm)\ntheta = lamda/(2*beta); #Angle of the wedge(rad)\ntheta = theta*10**4;\ntheta = math.ceil(theta*10**4)/10**4; #rounding off the value of theta to 4 decimals\n\n#Result\nprint \"The angle of the wedge is\",theta,\"*10**-4 rad\"", + "input": [ + " \n", + "#importing modules\n", + "import math\n", + "\n", + "#Variable declaration\n", + "lamda = 5893; #Wavelength of monochromatic lihgt used(A)\n", + "n = 10; #Number of fringe that are found \n", + "d = 1; #Distance of 10 fringes(cm)\n", + "\n", + "#Calculation\n", + "beta = d/n; #Fringe width(cm)\n", + "lamda = lamda*10**-8; #Wavelength of monochromatic lihgt used(cm)\n", + "theta = lamda/(2*beta); #Angle of the wedge(rad)\n", + "theta = theta*10**4;\n", + "theta = math.ceil(theta*10**4)/10**4; #rounding off the value of theta to 4 decimals\n", + "\n", + "#Result\n", + "print \"The angle of the wedge is\",theta,\"*10**-4 rad\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The angle of the wedge is 2.9465 *10**-4 rad\n" + "text": [ + "The angle of the wedge is 2.9465 *10**-4 rad\n" + ] } ], "prompt_number": 12 @@ -122,19 +248,41 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.6, Page number 72" + "source": [ + "Example number 3.6, Page number 72" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the separation between consecutive bright fringes\n\n#importing modules\nimport math\nfrom __future__ import division\n\n#Variable declaration\nlamda = 5900; #Wavelength of monochromatic lihgt used(A)\nt = 0.010; #Spacer thickness(mm)\nl = 10; #Wedge length(cm)\n\n#Calculation\nt = t*10**-1; #Spacer thickness(cm)\ntheta = t/l; #Angle of the wedge(rad)\nlamda = lamda*10**-8; #Wavelength of monochromatic lihgt used(cm)\nbeta = lamda/(2*theta); #Fringe width(cm)\n\n#Result\nprint \"The separation between consecutive bright fringes is\",beta, \"cm\"", + "input": [ + " \n", + "import math\n", + "from __future__ import division\n", + "\n", + "#Variable declaration\n", + "lamda = 5900; #Wavelength of monochromatic lihgt used(A)\n", + "t = 0.010; #Spacer thickness(mm)\n", + "l = 10; #Wedge length(cm)\n", + "\n", + "#Calculation\n", + "t = t*10**-1; #Spacer thickness(cm)\n", + "theta = t/l; #Angle of the wedge(rad)\n", + "lamda = lamda*10**-8; #Wavelength of monochromatic lihgt used(cm)\n", + "beta = lamda/(2*theta); #Fringe width(cm)\n", + "\n", + "#Result\n", + "print \"The separation between consecutive bright fringes is\",beta, \"cm\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The separation between consecutive bright fringes is 0.295 cm\n" + "text": [ + "The separation between consecutive bright fringes is 0.295 cm\n" + ] } ], "prompt_number": 13 @@ -143,19 +291,40 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.7, Page number 72" + "source": [ + "Example number 3.7, Page number 72" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the diameter of 20th dark ring\n\n#importing modules\nimport math\n\n#Variable declaration\nD4 = 0.4; #Diameter of 4th dark ring(cm)\nD12 = 0.7; #Diameter of 12th dark ring(cm)\n\n#Calculation\n#We have (dn_plus_k**2)-Dn**2 = 4*k*R*lamda\n#D12**2-D4**2 = 32*R*lamda and D20**2-D12**2 = 32*R*lamda for k = 8\n#since RHS are equal, by equating the LHS we get D12**2-D4**2 = D20**2-D12**2\nD20 = math.sqrt((2*D12**2)-D4**2); #Diameter of 20th dark ring(cm)\nD20 = math.ceil(D20*10**4)/10**4; #rounding off the value of D20 to 4 decimals\n\n#Result\nprint \"The diameter of 20th dark ring is\",D20, \"cm\"", + "input": [ + " \n", + "import math\n", + "\n", + "#Variable declaration\n", + "D4 = 0.4; #Diameter of 4th dark ring(cm)\n", + "D12 = 0.7; #Diameter of 12th dark ring(cm)\n", + "\n", + "#Calculation\n", + "#We have (dn_plus_k**2)-Dn**2 = 4*k*R*lamda\n", + "#D12**2-D4**2 = 32*R*lamda and D20**2-D12**2 = 32*R*lamda for k = 8\n", + "#since RHS are equal, by equating the LHS we get D12**2-D4**2 = D20**2-D12**2\n", + "D20 = math.sqrt((2*D12**2)-D4**2); #Diameter of 20th dark ring(cm)\n", + "D20 = math.ceil(D20*10**4)/10**4; #rounding off the value of D20 to 4 decimals\n", + "\n", + "#Result\n", + "print \"The diameter of 20th dark ring is\",D20, \"cm\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The diameter of 20th dark ring is 0.9056 cm\n" + "text": [ + "The diameter of 20th dark ring is 0.9056 cm\n" + ] } ], "prompt_number": 14 @@ -164,19 +333,38 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.8, Page number 73" + "source": [ + "Example number 3.8, Page number 73" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the refractive index of the liquid\n\n#importing modules\nimport math\nfrom __future__ import division\n\n#Variable declaration\nDn = 0.30; #Diameter of nth dark ring with air film(cm)\ndn = 0.25; #Diameter of nth dark ring with liquid film(cm)\n\n#Calculation\nmew = (Dn/dn)**2; #Refractive index of the liquid\n\n#Result\nprint \"The refractive index of the liquid is\", mew\n", + "input": [ + " \n", + "#importing modules\n", + "import math\n", + "from __future__ import division\n", + "\n", + "#Variable declaration\n", + "Dn = 0.30; #Diameter of nth dark ring with air film(cm)\n", + "dn = 0.25; #Diameter of nth dark ring with liquid film(cm)\n", + "\n", + "#Calculation\n", + "mew = (Dn/dn)**2; #Refractive index of the liquid\n", + "\n", + "#Result\n", + "print \"The refractive index of the liquid is\", mew\n" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The refractive index of the liquid is 1.44\n" + "text": [ + "The refractive index of the liquid is 1.44\n" + ] } ], "prompt_number": 15 @@ -185,19 +373,39 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.9, Page number 73" + "source": [ + "Example number 3.9, Page number 73" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the wavelength of light\n\n#importing modules\nimport math\n\n#Variable declaration\nx = 0.002945; #Distance through which movable mirror is shifted(cm)\nN = 100; #Number of fringes shifted\n\n#Calculation\nx = x*10**-2; #Distance through which movable mirror is shifted(m)\nlamda = 2*x/N; #Wavelength of light(m)\nlamda = lamda*10**10; #Wavelength of light(A)\n\n#Result\nprint \"The wavelength of light is\",lamda, \"angstrom\"", + "input": [ + " \n", + "#importing modules\n", + "import math\n", + "\n", + "#Variable declaration\n", + "x = 0.002945; #Distance through which movable mirror is shifted(cm)\n", + "N = 100; #Number of fringes shifted\n", + "\n", + "#Calculation\n", + "x = x*10**-2; #Distance through which movable mirror is shifted(m)\n", + "lamda = 2*x/N; #Wavelength of light(m)\n", + "lamda = lamda*10**10; #Wavelength of light(A)\n", + "\n", + "#Result\n", + "print \"The wavelength of light is\",lamda, \"angstrom\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The wavelength of light is 5890.0 angstrom\n" + "text": [ + "The wavelength of light is 5890.0 angstrom\n" + ] } ], "prompt_number": 16 @@ -206,19 +414,39 @@ "cell_type": "heading", "level": 2, "metadata": {}, - "source": "Example number 3.10, Page number 73" + "source": [ + "Example number 3.10, Page number 73" + ] }, { "cell_type": "code", "collapsed": false, - "input": "#To calculate the shift in movable mirror\n\n#importing modules\nimport math\n\n#Variable declaration\nlambda1 = 5896; #Wavelength of D1 line of sodium(A)\nlambda2 = 5890; #Wavelength of D2 line of sodium(A)\n\n#Calculation\nlamda = (lambda1+lambda2)/2;\nx = (lamda**2)/(2*(lambda1-lambda2)); #Shift in movable mirror of Michelson Interferometer(A)\nx = x*10**-7; #Shift in movable mirror of Michelson Interferometer(mm)\nx = math.ceil(x*10**4)/10**4; #rounding off the value of D20 to 4 decimals\n\n#Result\nprint \"The shift in movable mirror is\",x, \"mm\"", + "input": [ + " \n", + "import math\n", + "\n", + "#Variable declaration\n", + "lambda1 = 5896; #Wavelength of D1 line of sodium(A)\n", + "lambda2 = 5890; #Wavelength of D2 line of sodium(A)\n", + "\n", + "#Calculation\n", + "lamda = (lambda1+lambda2)/2;\n", + "x = (lamda**2)/(2*(lambda1-lambda2)); #Shift in movable mirror of Michelson Interferometer(A)\n", + "x = x*10**-7; #Shift in movable mirror of Michelson Interferometer(mm)\n", + "x = math.ceil(x*10**4)/10**4; #rounding off the value of D20 to 4 decimals\n", + "\n", + "#Result\n", + "print \"The shift in movable mirror is\",x, \"mm\"" + ], "language": "python", "metadata": {}, "outputs": [ { "output_type": "stream", "stream": "stdout", - "text": "The shift in movable mirror is 0.2894 mm\n" + "text": [ + "The shift in movable mirror is 0.2894 mm\n" + ] } ], "prompt_number": 17 @@ -226,7 +454,7 @@ { "cell_type": "code", "collapsed": false, - "input": "", + "input": [], "language": "python", "metadata": {}, "outputs": [] |