- •Contents
- •Preface
- •How to use this book
- •Chapter 1 Units, constants, and conversions
- •1.1 Introduction
- •1.2 SI units
- •1.3 Physical constants
- •1.4 Converting between units
- •1.5 Dimensions
- •1.6 Miscellaneous
- •Chapter 2 Mathematics
- •2.1 Notation
- •2.2 Vectors and matrices
- •2.3 Series, summations, and progressions
- •2.5 Trigonometric and hyperbolic formulas
- •2.6 Mensuration
- •2.8 Integration
- •2.9 Special functions and polynomials
- •2.12 Laplace transforms
- •2.13 Probability and statistics
- •2.14 Numerical methods
- •Chapter 3 Dynamics and mechanics
- •3.1 Introduction
- •3.3 Gravitation
- •3.5 Rigid body dynamics
- •3.7 Generalised dynamics
- •3.8 Elasticity
- •Chapter 4 Quantum physics
- •4.1 Introduction
- •4.3 Wave mechanics
- •4.4 Hydrogenic atoms
- •4.5 Angular momentum
- •4.6 Perturbation theory
- •4.7 High energy and nuclear physics
- •Chapter 5 Thermodynamics
- •5.1 Introduction
- •5.2 Classical thermodynamics
- •5.3 Gas laws
- •5.5 Statistical thermodynamics
- •5.7 Radiation processes
- •Chapter 6 Solid state physics
- •6.1 Introduction
- •6.2 Periodic table
- •6.4 Lattice dynamics
- •6.5 Electrons in solids
- •Chapter 7 Electromagnetism
- •7.1 Introduction
- •7.4 Fields associated with media
- •7.5 Force, torque, and energy
- •7.6 LCR circuits
- •7.7 Transmission lines and waveguides
- •7.8 Waves in and out of media
- •7.9 Plasma physics
- •Chapter 8 Optics
- •8.1 Introduction
- •8.5 Geometrical optics
- •8.6 Polarisation
- •8.7 Coherence (scalar theory)
- •8.8 Line radiation
- •Chapter 9 Astrophysics
- •9.1 Introduction
- •9.3 Coordinate transformations (astronomical)
- •9.4 Observational astrophysics
- •9.5 Stellar evolution
- •9.6 Cosmology
- •Index
2.12 Laplace transforms |
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2.12 Laplace transforms
Laplace transform theorems
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Definitiona |
F(s) = L{f(t)} = 0 |
∞ f(t)e−st dt |
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(2.514) |
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Convolutionb |
F(s) · G(s) = L &0 |
∞ f(t− z)g(z) dz' |
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(2.515) |
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(2.516) |
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f(t) = |
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estF(s) ds |
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(2.517) |
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Inversec |
2πi |
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dnf(t) |
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Transform of |
L & |
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(2.519) |
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transform |
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(t)} |
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dsn |
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Substitution |
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e−asF(s) = |
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(2.522) |
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Translation |
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(2.523) |
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L{} |
Laplace |
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F(s) |
L{f(t)} |
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G(s) |
L{g(t)} |
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convolution
γconstant
ninteger > 0
aconstant
u(t) unit step function
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is finite for su ciently large t, the Laplace transform exists for s > s0. |
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Also known as the “faltung (or folding) theorem.” |
cAlso known as the “Bromwich integral.” γ is chosen so that the singularities in F(s) are left of the integral line.
56 Mathematics
Laplace transform pairs
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f(t) = F(s) = L{f(t)} = 0 |
∞ f(t)e−st dt |
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t1/2 |
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teat |
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sinat = |
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cosat = |
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sinhat = |
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coshat = |
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2.13 Probability and statistics |
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2.13Probability and statistics
Discrete statistics |
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N |
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Mean |
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(2.541) |
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var[ |
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unbiased |
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Standard |
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deviation |
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Skewness |
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Correlation |
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aIf x is derived from the data, {xi}, the relation is as shown. If x is known independently, then an unbiased estimate is obtained by dividing the right-hand side by N rather than N − 1.
bAlso known as “Pearson’s r.”
Discrete probability distributions
distribution |
pr(x) |
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Binomial |
xn px(1 − p)n−x |
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Geometric |
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Poisson |
λx exp(−λ)/x! |
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58 Mathematics
Continuous probability distributions
distribution |
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exp |
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Cauchy/ |
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aWith r degrees of freedom. Γ is the gamma function.
Multivariate normal distribution
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probability density |
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exp |
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1 (x |
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number of dimensions |
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Density function |
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(2π)k/−2[det(C)]1/−2 |
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C |
covariance matrix |
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(2.556) |
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variable (k dimensional) |
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µ |
vector of means |
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T |
transpose |
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Mean |
µ = (µ1,µ2,... ,µk) |
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(2.557) |
det |
determinant |
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µi |
mean of ith variable |
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Covariance |
C = σij = xixj |
− xi |
xj |
(2.558) |
σij |
components of C |
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Correlation |
r = |
σij |
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(2.559) |
r |
correlation coe cient |
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coe cient |
σiσj |
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1/2 |
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xi |
normally distributed deviates |
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Box–Muller |
x1 = (−2lny1)1/2 cos2πy2 |
(2.560) |
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yi |
deviates distributed |
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transformation |
x2 = (−2lny1) |
sin2πy2 |
(2.561) |
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uniformly between 0 and 1 |
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2.13 Probability and statistics |
59 |
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Random walk
One- |
pr(x) = |
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1 |
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exp |
−x2 |
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dimensional |
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(2πNl2)1/2 |
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2Nl2 |
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(2.562) |
rms |
xrms = N1/2l |
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(2.563) |
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displacement |
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a |
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3 |
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pr(r) = |
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exp(−a2r2) |
(2.564) |
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Three- |
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π1/2 |
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dimensional |
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3 |
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where a = |
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2Nl2 |
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r = |
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Mean distance |
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N1/2l |
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(2.565) |
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3π |
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rms distance |
rrms = N1/2l |
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(2.566) |
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xdisplacement after N steps (can be positive or negative)
pr(x) probability density of x |
2 |
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(%−∞∞ pr(x) dx = 1) |
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N |
number of steps |
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lstep length (all equal)
xrms root-mean-squared displacement from start point
rradial distance from start point
pr(r) probability density of r (%0∞ 4πr2 pr(r) dr = 1)
a(most probable distance)−1
r mean distance from start point
rrms |
root-mean-squared distance |
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from start point |
Bayesian inference
Conditional |
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pr(x) |
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probability (density) of x |
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pr(x) = |
pr(x |
y |
)pr(y |
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(2.567) |
pr(x |
y |
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conditional probability of x |
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probability |
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given y |
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Joint |
pr(x,y) = pr(x)pr(y|x) |
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(2.568) |
pr(x,y) |
joint probability of x and y |
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probability |
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Bayes’ theorema |
pr(y |
x) = |
pr(x|y) pr(y) |
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(2.569) |
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pr(x) |
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aIn this expression, pr(y|x) is known as the posterior probability, pr(x|y) the likelihood, and pr(y) the prior probability.