Unveiling the Power of \(( ๐ฅ ± ๐ 0 )^\lambda\) : A Research Scholar's Guide to Generalized Functions and Singularities Matrix Space Toolkit in SageMath Understanding \(( ๐ฅ ± ๐ 0 )^\lambda\)and the Power of Generalized Functions Why It Matters? As researchers, we often model reality with smooth, well-behaved functions. But real-world events—like a hammer strike, a lightning bolt, or an electron quantum jump—are not smooth. These sudden changes or singularities require mathematical tools that go beyond ordinary functions. Enter: \[( ๐ฅ ± ๐ 0 )^\lambda \] Complex Limits with Profound Implications A Brief History: Why Generalized Functions? In the early 20th century, quantum physics revealed the inadequacy of classical f...
Understanding Delta Function Approximations: Lorentzian Delta Sequence (Cauchy Kernel)
- Get link
- X
- Other Apps
Delta-Convergent Sequences — Refined Blog with SageMath Symbolics, Physics Insights, and Cleaner Code
The Dirac delta function isn’t a “normal” function — it’s an idealization used to represent a point source. It's infinitely narrow, infinitely tall, and yet integrates to 1. We approximate it using delta-convergent sequences: real functions depending on a parameter that becomes increasingly peaked at zero as the parameter vanishes.
This post explores the three most common delta-approximating sequences using SageMath, including plots, integration checks, and real-world meaning.
Why Study These Approximations?
Delta functions are central in many fields:
- Signal Processing: Ideal impulse, filter response
- Physics: Point charges/masses, Green's functions
- Spectral Theory: Lorentzian profiles in resonance
- Diffusion Models: Gaussians arise from the heat equation
- Numerics: Regularizing singular integrals
Each kernel has a story to tell.
Lorentzian Delta Sequence
Formula \[ f_{\epsilon}(x) = \frac{1}{\pi}. \frac{\epsilon}{x^2+ {\epsilon}^2} \]
- Sharp peak at ๐ฅ=0
- Always integrates to 1
- Smooth and rational
# Check the Function Definition
var('x epsilon')
f_lorentz(x, epsilon) = (1/pi) * (epsilon / (x^2 + epsilon^2))
f_lorentz(x, epsilon)
# Check Symbolic Integration
var('xi')
assume(epsilon > 0) # Ensure SageMath understands epsilon is positive
integral(f_lorentz(xi, epsilon), xi, -oo, oo).simplify_full()
#Check Limit at x → 0
limit(f_lorentz(x, epsilon), epsilon=0)
# Integral Test (Distributional Behavior)
var('a b')
assume(a < 0, b > 0) # Ensure a < 0 < b to match delta behavior
integral(f_lorentz(xi, epsilon), xi, a, b).simplify_full()
# Numerical Evaluation
# To see how the integral converges to 1 as ( \epsilon \to 0 ), run:
import numpy as np
import matplotlib.pyplot as plt
import sage.all as sage
def lorentzian_integral(epsilon, a=-1, b=1):
return (np.arctan(b/epsilon) - np.arctan(a/epsilon)) / np.pi
# Test for different epsilon values
epsilons = np.logspace(-3, 0, 50) # Log-spaced values from 0.001 to 1
integral_values = [lorentzian_integral(eps) for eps in epsilons]
# Plotting
plt.figure(figsize=(8, 5))
plt.plot(epsilons, integral_values, marker='o', linestyle='-', color='blue')
plt.axhline(y=1, color='r', linestyle='--', label="Expected Limit (1)")
plt.xscale("log")
plt.xlabel(r"$\epsilon$")
plt.ylabel(r"Integral Value")
plt.title("Numerical Verification: Lorentzian Integral Convergence")
plt.legend()
plt.grid(True)
plt.show()
# Lorentzian delta approximation
var('x epsilon xi')
assume(epsilon > 0) # Ensure epsilon is positive for proper symbolic handling
f_lorentz(x, epsilon) = (1/pi) * (epsilon / (x^2 + epsilon^2))
# Symbolic normalization check
integral(f_lorentz(xi, epsilon), xi, -oo, oo).simplify_full()
# Limit at x = 0 to verify ฮด-behavior
limit(f_lorentz(x, epsilon), epsilon=0)
# Plot Lorentzian for different ฮต
p1 = plot(f_lorentz(x, 0.5), (x, -5, 5), color='red', legend_label='ฮต = 0.5') + \
plot(f_lorentz(x, 0.2), (x, -5, 5), color='blue', legend_label='ฮต = 0.2') + \
plot(f_lorentz(x, 0.05), (x, -5, 5), color='green', legend_label='ฮต = 0.05')
p1.show(title='Lorentzian Approximation to ฮด(x)', ymin=0, ymax=3)
# Numerical Limits Instead of Symbolic
epsilon_vals = [0.1, 0.01, 0.001, 0.0001]
[f_lorentz(0, eps).n() for eps in epsilon_vals]
# Check Symbolic Integration
# Confirm normalization:
var('xi')
assume(epsilon > 0) # Ensure SageMath understands epsilon is positive
integral(f_lorentz(xi, epsilon), xi, -oo, oo).simplify_full()
# First & Second Derivative Computation
f_lorentz_prime(x, epsilon) = diff(f_lorentz(x, epsilon), x)
f_lorentz_double_prime(x, epsilon) = diff(f_lorentz_prime(x, epsilon), x)
f_lorentz_prime(x, epsilon), f_lorentz_double_prime(x, epsilon)
#Plot First & Second Derivative
p1 = plot(f_lorentz_prime(x, 0.5), (x, -5, 5), color='red', legend_label="ฮต=0.5") + \
plot(f_lorentz_prime(x, 0.2), (x, -5, 5), color='blue', legend_label="ฮต=0.2") + \
plot(f_lorentz_prime(x, 0.05), (x, -5, 5), color='green', legend_label="ฮต=0.05")
p1.show(title="First Derivative of Lorentzian Approximation")
p2 = plot(f_lorentz_double_prime(x, 0.5), (x, -5, 5), color='red', legend_label="ฮต=0.5") + \
plot(f_lorentz_double_prime(x, 0.2), (x, -5, 5), color='blue', legend_label="ฮต=0.2") + \
plot(f_lorentz_double_prime(x, 0.05), (x, -5, 5), color='green', legend_label="ฮต=0.05")
p2.show(title="Second Derivative of Lorentzian Approximation")
#Integration of the Lorentzian Sequence
# Compute symbolic integral
var('a b')
assume(a < 0, b > 0)
integral(f_lorentz(x, epsilon), x, a, b).simplify_full()
p1=plot(integral(f_lorentz(x, 0.1), x, -5, 5), (x, -5, 5), color='blue', legend_label="Lorentzian")
p1.show(title="Integrated Delta Approximations")
# Plotting the Integrated Sequences
# To visualize how the cumulative integrals approach step-like functions:
p1=plot(integral(f_lorentz(x, 0.1), x, -5, 5), (x, -5, 5), color='blue', legend_label="Lorentzian")
p1.show(title="Integrated Delta Approximations")
๐ก Try It Yourself! Now You can copy and paste directly into here Run SageMath Code Here
Physics Note
Used in resonance and spectral line broadening (e.g. Lorentzian profile in spectroscopy).
- Get link
- X
- Other Apps
Popular posts from this blog
Spirals in Nature: The Beautiful Geometry of Life
Spirals—nature’s perfect blend of beauty and efficiency—are everywhere around us, from the tiniest microorganisms to the vast reaches of space. But why are spirals so prevalent? Mathematics holds the key to unraveling their secrets. Let’s explore the fascinating role of spirals in nature, their mathematical roots, and the efficiency they bring to the natural world. The Fibonacci Spiral: Nature’s Design Genius The Fibonacci spiral is perhaps the most iconic spiral in nature, deeply intertwined with the Golden Ratio. The Golden Ratio (approximately 1.618) is a special number that appears in many natural patterns. But how does this spiral work? How it works : The Fibonacci sequence is a series of numbers where each number is the sum of the two preceding ones (0, 1, 1, 2, 3, 5, 8, 13, and so on). If you draw squares whose side lengths correspond to Fibonacci numbers and connect quarter circles inside each square, you create the Fibonacci spiral. Where ...
Sagemath
๐ Illuminating Light: Waves, Mathematics, and the Secrets of the Universe
Meta Description: Discover how light—both wave and particle—is unlocking secure communication, eco-energy, and global education. From photons in space to classrooms in refugee zones, explore the science, math, and mission behind the light. ๐ Introduction: Light as the Universe’s Code Light is more than brightness—it's how the universe shares its secrets. It paints rainbows, powers satellites, and now—connects minds and saves lives. Could understanding photons help us shape a better future? In this blog, you’ll explore: ๐ฌ 1. What Is Light? Both Wave and Particle Light behaves as a wave and a photon. That duality underlies quantum mechanics and modern technology. ๐งช Key Moments: ๐ Core Properties: ๐ 2. Light Through Math: Predicting Its Path ⚡ Maxwell’s Equations: Four simple expressions unify electricity, magnetism, and optics—laying the foundation for electromagnetic theory. ๐ 3. Interference: How Light Combines ...
Comments
Post a Comment
If you have any queries, do not hesitate to reach out.
Unsure about something? Ask away—I’m here for you!