scholarly journals Scanning of the supersymmetry breaking scale and the gravitino mass in supergravity

2016 ◽  
Vol 2016 (6) ◽  
Author(s):  
Fotis Farakos ◽  
Alex Kehagias ◽  
Davide Racco ◽  
Antonio Riotto
1997 ◽  
Vol 399 (1-2) ◽  
pp. 92-96 ◽  
Author(s):  
I. Antoniadis ◽  
J. Ellis ◽  
G.K. Leontaris

2021 ◽  
Vol 2021 (7) ◽  
Author(s):  
Thibaut Coudarchet ◽  
Emilian Dudas ◽  
Hervé Partouche

Abstract Starting from a peculiar orientifold projection proposed long ago by Angelantonj and Cardella, we elaborate on a novel perturbative scenario that involves only D-branes, together with the two types of orientifold planes O± and anti-orientifold planes $$ {\overline{\mathrm{O}}}_{\pm } $$ O ¯ ± . We elucidate the microscopic ingredients of such models, connecting them to a novel realization of brane supersymmetry breaking. Depending on the position of the D-branes in the internal space, supersymmetry can be broken at the string scale on branes, or alternatively only at the massive level. The main novelty of this construction is that it features no NS-NS disk tadpoles, while avoiding open-string instabilities. The one-loop potential, which depends on the positions of the D-branes, is minimized for maximally broken, non-linearly realized supersymmetry. The orientifold projection and the effective field theory description reveal a soft breaking of supersymmetry in the closed-string sector. In such models it is possible to decouple the gravitino mass from the value of the scalar potential, while avoiding brane instabilities.


1989 ◽  
Vol 04 (25) ◽  
pp. 2429-2435 ◽  
Author(s):  
G.K. LEONTARIS ◽  
N.D. TRACAS ◽  
C.E. VAYONAKIS

Motivated by the plethora of models, mainly remanant from superstring theories, in which several U(1) factors are present, we consider constraints on these theories from the requirement that non-perturbative, as opposed to perturbative, unification arises close to the Planck scale. We find that non-perturbative unification can be realized with three standard families up to a supersymmetry breaking scale of order 100–500 TeV and six supersymmetric families above that scale.


Author(s):  
Hervé Partouche ◽  
Balthazar de Vaulchier

When supersymmetry is spontaneously broken at the tree level, the spectrum of the heterotic string compactified on orbifolds of tori contains an infinite number of potentially tachyonic modes. We show that this implies instabilities of Minkowski space–time, when the scale of supersymmetry breaking is of the order of the string scale. We derive the phase space structure of vacua in the case where the tachyonic spectrum contains a mode with trivial momenta and winding numbers along the internal directions not involved in the supersymmetry breaking.


1990 ◽  
Vol 243 (3) ◽  
pp. 250-256 ◽  
Author(s):  
Michael Dine ◽  
Alex Kagan ◽  
Stuart Samuel

2006 ◽  
Vol 21 (17) ◽  
pp. 3441-3472 ◽  
Author(s):  
JASON KUMAR

We review some basic flux vacua counting techniques and results, focusing on the distributions of properties over different regions of the landscape of string vacua and assessing the phenomenological implications. The topics we discuss include: an overview of how moduli are stabilized and how vacua are counted; the applicability of effective field theory; the uses of and differences between probabilistic and statistical analysis (and the relation to the anthropic principle); the distribution of various parameters on the landscape, including cosmological constant, gauge group rank, and supersymmetry-breaking scale; "friendly landscapes;" open string moduli; the (in)finiteness of the number of phenomenologically viable vacua; etc. At all points, we attempt to connect this study to the phenomenology of vacua which are experimentally viable.


1992 ◽  
Vol 105 (8) ◽  
pp. 1201-1206 ◽  
Author(s):  
F. Anselmo ◽  
L. Cifarelli ◽  
A. Peterman ◽  
A. Zichichi

2017 ◽  
Vol 916 ◽  
pp. 688-708 ◽  
Author(s):  
Fredrik Björkeroth ◽  
Stephen F. King ◽  
Kai Schmitz ◽  
Tsutomu T. Yanagida

Sign in / Sign up

Export Citation Format

Share Document