How Does Dirichlet Boundary Condition Affect Open String Mode Expansion?

In summary, the mode expansion for an open string with Neumann boundary conditions for coordinates X^0,...,X^24 can be expressed as a sum of left- and right-moving modes in the light-cone coordinates \sigma - \tau and \sigma + \tau. To incorporate the Dirichlet boundary conditions for the 25th coordinate, we can define a new coordinate \tilde{X}^{25} and substitute it into the original expression for X^\mu. This will give us a new mode expansion that satisfies the Dirichlet boundary conditions.
  • #1
Themetricsystem
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Compute the mode expansion for an open string with Neumann boundary conditions for the coordinates X^0,..., X^24, while the remaining coordinate X^25 satisfies Dirichlet boundary conditions at both ends:
[tex]
\[
X^{25}(0, \tau) = X^{25}_0 \quad \text{and} \quad X^{25}(\pi, \tau) = X^{25}_\pi \, .
\]
[/tex]

-------

I know that the mode expansion is a sum of left- and right-moving modes
(in the light-cone coordinates [tex]\sigma - \tau[/tex] and [tex]\sigma+\tau[/tex].)

The expression for the X^\mu in the open-string expansion is
[tex]
\[
X^\mu(\tau, \sigma) = x^\mu + \ell^2_s p^\mu \tau + i\ell_s \sum_{m \neq 0} \frac{\alpha^\mu_m}{m} \, e^{-im\tau} \cos (m\sigma) \, ,
\]
[/tex]

but I'm not sure how to fit the Dirichlet conditions in the twenty-fifth coordinate.

Edit: Sorry, here are definitions for some of the symbols:

tau and sigma are timelike and spacelike coordinates, respectively. They parameterize the world-sheet and appear in the embedding functions X^\mu.

The [tex]\alpha^\mu_m[/tex] are actually operators that have harmonic-oscillator-like commutation relations:
[tex]
\[
[\alpha^\mu_m, \alpha^\nu_n] = m \eta^{\mu\nu} \delta_{m+n, 0} \, .
\]
[/tex]
 
Last edited:
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  • #2



Hi there,

To incorporate the Dirichlet boundary conditions for the 25th coordinate, we can start by defining a new coordinate \tilde{X}^{25} as

\[
\tilde{X}^{25}(\tau, \sigma) = X^{25}(\tau, \sigma) - \frac{X^{25}_0 + X^{25}_\pi}{2} \, .
\]

This shifts the origin of the coordinate to the midpoint between the two boundary conditions. We can then rewrite the mode expansion for X^{25} as

\[
X^{25}(\tau, \sigma) = \tilde{X}^{25}(\tau, \sigma) + \frac{X^{25}_0 + X^{25}_\pi}{2} \, ,
\]

and substitute this into the original expression for X^\mu. This will give us a new mode expansion for X^\mu that satisfies the Dirichlet boundary conditions for the 25th coordinate.

Hope this helps! Let me know if you have any further questions.
 

1. What is "Open-string mode expansion"?

Open-string mode expansion is a mathematical technique used in string theory to describe the behavior of open strings. It involves expanding the fields and coordinates of the string in terms of an infinite number of modes, each with a different frequency and amplitude.

2. How does open-string mode expansion relate to closed-string mode expansion?

Open-string mode expansion is the counterpart to closed-string mode expansion, which is used to describe the behavior of closed strings. While closed-string modes are quantized, open-string modes are continuous, meaning they can take on all possible values.

3. What is the significance of the mode numbers in open-string mode expansion?

The mode numbers in open-string mode expansion represent the different frequencies and amplitudes at which the string can vibrate. They are quantized and play a crucial role in determining the properties and behavior of the string.

4. How is open-string mode expansion used in practical applications of string theory?

Open-string mode expansion is a fundamental tool in string theory and is used in various calculations and predictions. For example, it is used to calculate scattering amplitudes, study the properties of black holes, and understand the dynamics of string interactions.

5. Are there any limitations or challenges associated with open-string mode expansion?

One limitation of open-string mode expansion is that it only applies to open strings, and cannot be directly applied to closed strings. Additionally, the infinite number of modes can make calculations complex and time-consuming, requiring advanced mathematical techniques and technology.

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