Graduate Why are open strings vectors or scalars, or massive?

Click For Summary
In string theory, the boundary conditions (BCs) determine the nature of excitations, leading to massless vectors and scalars based on the configuration of Neumann (NN) and Dirichlet (DD) BCs. Specifically, NN BCs along certain dimensions yield massless vectors, while DD BCs result in massless scalars. The massless nature of these excitations is confirmed at the first excited level where the mass squared, M^2, equals zero. The relationship between the distance between two branes and the mass squared, M^2 ∝ δ^2, raises questions about the tensorial nature of these excitations. The creation operator's indices play a crucial role in determining whether the excitations are scalars or vectors, linked to the type of boundary conditions applied.
Maurice7510
Messages
52
Reaction score
0
In string theory, if we have NN BCs along ##X^i, i = 1, \ldots, n-1##
and DD BCs along ##X^a, a = n, \ldots, 25## then you get, from ##\alpha^{i,a}_{-1}|0,p\rangle ##, ##n## massless vectors and ##24-n## massless scalars. I understand that for the first excited level, ##M^2=0## and so we have no mass, but what suggests that these are scalars or vectors? In the case where we have two branes separated by a distance ##\delta##, with find ##M^2\propto\delta^2## which, in addition to the vector/scalar nature of the excitations, I don't understand.
 
Physics news on Phys.org
Their tensorial nature is determined by the index of the creation operator, no?
 
I'm not sure how that would be the case though; the indices on the creation operator are ##i## (or ##a##) and ##-1##. The lower index is the state number (i.e. ##\alpha_{-1}## creates a one particle state) and the upper indicates indicate whether the BCs are NN or DD.
 
"Supernovae evidence for foundational change to cosmological models" https://arxiv.org/pdf/2412.15143 The paper claims: We compare the standard homogeneous cosmological model, i.e., spatially flat ΛCDM, and the timescape cosmology which invokes backreaction of inhomogeneities. Timescape, while statistically homogeneous and isotropic, departs from average Friedmann-Lemaître-Robertson-Walker evolution, and replaces dark energy by kinetic gravitational energy and its gradients, in explaining...

Similar threads

  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
4K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 0 ·
Replies
0
Views
2K
  • · Replies 2 ·
Replies
2
Views
5K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K