I Is Supersymmetry required by String theory?

TheHeraclitus
Messages
14
Reaction score
1
TL;DR Summary
Supersymmetry is often mentioned together with String theory, but do all String theories require it?
From what I understood Supersymmetry means there are more particles than we currently know about and they are predicted by (some/all, I do not know) versions of String theory.
Is it so important to String theory or can it work without SUSY?

Thank you!
 
Physics news on Phys.org
Susy is, as far as we know, required for the particle spectrum to be consistent. Without susy you get e.g. tachyonic particles which are hard to interpret as physical particles. So yes.
 
haushofer said:
Susy is, as far as we know, required for the particle spectrum to be consistent. Without susy you get e.g. tachyonic particles which are hard to interpret as physical particles. So yes.
Non-perturbative formulation of bosonic string-field theory reinterprets tachyonic state as an unstable state, very much like tachyonic Higgs field before symmetry breaking is reinterpreted as an unstable state. By a process of tachyon condenzation the unstable state (local maximum of the potential) settles down into a stable state (local minimum of the potential) and excitations around the stable state are no longer tachyonic. So I would say no.

But we still need susy in string theory because that's the only known way (as fas as I am aware) to incorporate fermions into string theory, and we need fermions because they are observed in nature.
 
Last edited:
I have seen multiple knowledgeable theoretical physicists state authoritatively that supersymmetry is necessary as a low energy approximation of string theory.

To some extent, however, it boils down to definitions.

If you use a fairly strict definition of string theory or M-theory, then this is probably correct.

If you use a loose definition of string theory that, for example, borrows heavily from its mathematical methods without embracing the entire discipline's canonical form for it, perhaps you could get a stringy theory that doesn't have supersymmetry as a low energy approximation.
 
https://arxiv.org/pdf/2503.09804 From the abstract: ... Our derivation uses both EE and the Newtonian approximation of EE in Part I, to describe semi-classically in Part II the advection of DM, created at the level of the universe, into galaxies and clusters thereof. This advection happens proportional with their own classically generated gravitational field g, due to self-interaction of the gravitational field. It is based on the universal formula ρD =λgg′2 for the densityρ D of DM...
Many of us have heard of "twistors", arguably Roger Penrose's biggest contribution to theoretical physics. Twistor space is a space which maps nonlocally onto physical space-time; in particular, lightlike structures in space-time, like null lines and light cones, become much more "local" in twistor space. For various reasons, Penrose thought that twistor space was possibly a more fundamental arena for theoretical physics than space-time, and for many years he and a hardy band of mostly...
Back
Top