Why do we need a normalisation constant for wavefunctions?

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The normalization constant 'A' in wavefunctions, such as ψ = Ae-kx², is essential to ensure that the total probability of finding a particle is equal to one. This is achieved through the normalization condition, which requires integrating the product of the wavefunction and its complex conjugate over all space. The value of 'A' is determined mathematically to satisfy this condition, ensuring that the modulus squared of the wavefunction reflects a valid probability distribution. Adjusting 'A' does not physically alter the amplitude of the wavefunction in experiments; rather, it allows the wavefunction to be interpreted correctly as a probability. Thus, the normalization process is crucial for the accurate representation of quantum states.
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ψ = Ae-kx2 ; A = normalisation constant
For normalising,
-infinf A2ψ°ψ dx = A2M (say) = 1
so we put A = 1/√M
My question is why we need 'A' ??

The thing is either we find a particle or we do not and if we think of a simple waveform...'A' gives the amplitude part...so can we put it in this way - we are altering the amplitude of the wavefunction to make the probability of finding the particle 1..?? If it is so, how altering the amplitude can do it physically..(cannot form the mental picture clearly)..
 
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You made a math error. Double check your substitutions.
 
Didn't do the integration at first so took the value to be 'M' .
The integration gives A = √(2k/π) . So we still have to put this value to normalise the wavefunction ...right...? Why ...??
 
You don't alter the amplitude of a wavefunction physically in your experiment to make it representable as a probability. We have hypothesized that the modulus square of the expansion coefficient of a wavefunction in some basis represents the probability upon measurement to find the state in the basis state associated with that expansion coefficient. Therefore the sum of all modulus squared of the expansion coefficients must yield unity, and one can prove that if the representing basis states are orthonormal, the inner product of the system's wavefunction being expanded must be unity, in order to satisfy the assumption that the expansion coefficient represent a probability. What you do in you calculation is to adjust the coefficient A such that the ψ(x) can be interpreted as a probability.
 
thanks...much clearer now...:smile:
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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