The boundary condition admits independent periodic functions of , for left-moving and right-moving modes respectively. It also admits linear solutions where the coefficients of , are equal. The most general solution admits an expansion

.

  • It is convenient to set .
  • The constant can be interpreted as the position of the centre of mass of a string in spacetime .
  • The coefficient of the linear terms, , has the interpretation of spacetime momentum.
  • The coefficients and correspond to the excitations of the left-moving and right-moving modes of the string. We require that the coordinate functions are real, i.e., .
  • Finally, is a parameter with dimensions of length. By convention, we set , and often introduce another related parameter .

Open Strings

Open strings admit a similar mode expansion. Since the string now has a spatial boundary, we must re-examine the action principle and ensure that the boundary terms cancel out. Variation of the gauge-fixed action principle produces a boundary condition

which must vanish to have a consistent action principle.

There are two ways to cancel boundary variations:

  1. Dirichlet boundary conditions:
  2. Neumann boundary conditions: .

In principle, we could choose either of the two boundary conditions independently for each index and boundary . Dirichlet boundary conditions break Poincaré symmetry though.

Here, we consider Neumann boundary conditions for all coordinates at both boundaries. This corresponds to a freely propagating open string. This forces the left-moving and right-moving modes to combine into trigonometric functions. The general solution takes the form

,

where the coefficients have a similar interpretation as before.

Reminder: .