HOW to read it:s ek parameter hai, tintegration variable hai. Integrate karne ke baad, t gayab ho jaata hai aur hum sirf s ka function lekar bachte hain.
Pehle L{eat} derive karo (yeh sabse aasaan hai aur sabse zyada reusable bhi):
L{eat}=∫0∞e−steatdt=∫0∞e−(s−a)tdt=[−(s−a)e−(s−a)t]0∞=s−a1,
Kyun s>a? Humein s−a>0 chahiye taaki exponential infinity pe decay kare. Yeh bas L{1} ka proof hai jisme s→s−a ho gaya.
L{tn} ko recursion se derive karo (integration by parts).
Maano In=∫0∞e−sttndt. ∫udv=uv−∫vdu use karo jahan u=tn,dv=e−stdt:
In=[tn−se−st]0∞+sn∫0∞e−sttn−1dt.
Yeh choice kyun?tn ko differentiate karna uski power ghataata hai, ek recursion banata hai.
Boundary term zero ho jaata hai: ∞ pe, e−st kisi bhi polynomial ko beat kar deta hai (s>0); 0 pe, n≥1 ke liye tn=0. Isliye
In=snIn−1.I0=L{1}=1/s se unroll karo:
In=sn⋅sn−1⋯s1⋅s1=sn+1n!.
Q: Bina compute kiye, L{cosat} guess karo, given ki tumhe pata hai L{sinat}=s2+a2a.
Predict: numerator s hona chahiye (cos→even, t=0 pe value 1), denominator same.
Verify:s2+a2s ✓. Note the trick: a→ia replace karne se sin/cos, sinh/cosh mein badal jaate hain, matlab s2+a2→s2−a2.
Laplace transform of f(t) ka defining integral kya hai?
∫0∞e−stf(t)dt, s ke liye region of convergence mein.
L{1}=? aur uski condition
1/s, valid for s>0.
L{eat}=?
s−a1 for s>a.
L{1} ke integral ko s>0 kyun chahiye?
Taaki e−st→0 jab t→∞; warna area diverge karta hai.
L{tn}=? aur yeh derive kaise hota hai?
n!/sn+1; recursion In=snIn−1 se, integration by parts ke zariye, I0=1/s se start karke.
L{sinat} aur L{cosat}?
s2+a2a aur s2+a2s.
Sin/cos transforms L{eiat} se kaise milte hain?
s−ia1=s2+a2s+ia compute karo, phir real part (cos) aur imaginary part (sin) lo.
L{coshat} aur L{sinhat}?
s2−a2s aur s2−a2a, for s>∣a∣.
Trig denominator hyperbolic mein kaise banta hai?
a→ia replace karo: s2+a2→s2−a2.
Recall Feynman: 12-saal ke bacche ko samjhao
Socho tum ek function ko wazan kar rahe ho. Har moment t pe jo weight daala jaata hai wo hai e−st — shuruaat ke paas bhaari, baad mein fade hota hua. Tum "function × weight" ko poore time pe add karte ho taaki s ki har choice ke liye ek number mile. Simple functions ke liye — jaise flat line, badhta exponential, ya hilta-dulta sine — yeh add-up saaf fractions deta hai. Hum har ek ko carefully add-up karke prove karte hain (ek integral), aur note karte hain ki s kitna bada hona chahiye taaki total infinity pe na bhaag jaaye.