Analytic study of the supersymmetry-breaking scale at two loops

1992 ◽  
Vol 105 (8) ◽  
pp. 1201-1206 ◽  
Author(s):  
F. Anselmo ◽  
L. Cifarelli ◽  
A. Peterman ◽  
A. Zichichi
1997 ◽  
Vol 399 (1-2) ◽  
pp. 92-96 ◽  
Author(s):  
I. Antoniadis ◽  
J. Ellis ◽  
G.K. Leontaris

2016 ◽  
Vol 2016 (6) ◽  
Author(s):  
Fotis Farakos ◽  
Alex Kehagias ◽  
Davide Racco ◽  
Antonio Riotto

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.


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

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