T-Duality and the String Length

Relativistic quantum strings wrapping around a compact dimension have a mass dependent on the winding w w and the momentum p p , which in turn depend on the radius of the compact dimension R R . The mass-squared of certain low-energy states can resultantly be written in terms of the radius as:

M 2 ( R ) = 1 R 2 + R 2 α 2 2 α . M^2 (R) = \frac{1}{R^2} + \frac{R^2}{\alpha^{\prime 2}} - \frac{2}{\alpha^{\prime}}.

Find the radius R R at which these states are massless, i.e. M 2 = 0 M^2 = 0 .

Bonus: Can you figure out why this is called the self-dual radius ?

2 α \frac{2}{\alpha^{\prime}} α \alpha^{\prime} α \sqrt{\alpha^{\prime}} 1 α 2 \frac{1}{\alpha^{\prime 2}}

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1 solution

Matt DeCross
Jan 23, 2016

Setting the mass-squared equal to zero yields the equation:

M 2 ( R ) = 0 = 1 R 2 + R 2 α 2 2 α . M^2(R) = 0 = \frac{1}{R^2} + \frac{R^2}{\alpha^{\prime 2}} - \frac{2}{\alpha^{\prime}}.

Solving for R R by inspection or by factoring the quartic yields R = α R = \sqrt{\alpha^{\prime}} .

T-duality relates spacetimes with compact dimensions of radius R R with dual spacetimes that have compact dimensions of radius α R \frac{\alpha^{\prime}}{R} . At radius R = α R = \sqrt{\alpha^{\prime}} , the radii of the original spacetime and the T-dual spacetime are equal, hence the name self-dual radius .

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