F-string, NS5-brane & D-string

  • Thread starter Thread starter crackjack
  • Start date Start date
Click For Summary
The discussion explores the relationship between fundamental strings (F-strings), NS5-branes, and extremal p-brane solutions in supergravity and Yang-Mills theories. It questions whether F-strings and NS5-branes are equivalent to extremal p-branes and how these constructs relate to D-branes. F-strings are identified as solitonic solutions of the SUGRA-YM equations coupled to the NS-NS 2-form, while D-strings correspond to solutions involving R-R 2-form couplings. The conversation also addresses the implications of these distinctions for heterotic supergravity, particularly in the context of closed string theories. Overall, the relationship between these string and brane solutions is crucial for understanding their roles in string theory.
crackjack
Messages
119
Reaction score
0
Is the fundamental string (F-string) same as an extremal 1-brane solution of su-gra-YM?
Can the same be said for the fundamental fivebrane (NS5-brane) and 5-brane?
Also, what kind of solution is a D-string?
 
Physics news on Phys.org
As a follow-up:

If F-strings & NS5-brane are different from extremal p-branes, then when p-branes are identified with as fundamental a construct as D-branes, how are F-strings & NS5-branes elevated?

If F-strings & NS5-brane are not different from extremal p-branes, what can we make out of these brane solutions in heterotic sugra when heterotic string theories are closed string theories (no open strings -> no branes to end on).
 
I asked around and got the following answer:

F-string is the solitonic solution of SUGRA-YM equations coupled to the NS-NS 2-form (B-field), whereas D-string are solutions of equations with R-R 2-form couplings.
F-strings are elevated to the normal strings of string theory, whereas D-strings are the D1-branes.
 
"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 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
1
Views
5K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K