Gravity and strings
Steven B. Giddings
Abstract
This is a broad-brush review of how string theory addresses several important questions of gravitational physics. The problem of non-renormalizability is first reviewed, followed by introduction of string theory as an ultraviolet-finite theory of gravity. String theory's successes also include predicting both gauge theory and fermions. The difficulty of extra dimensions becomes a possible virtue, when one notes that these lead to mechanisms to explain fermion generations, as well as a means to break the large gauge symmetries of string theory. Finally, a long standing problem of string theory, that of fixing the size and shape of the extra dimensions, has recently been addressed and may shed light on the origin of the cosmological constant, the ultimate fate of our universe, as well as the question of why gravityis so weak.
Create a lesson
Related papers
Chiral anomalies in two dimensions
Clément Liesse, Cypris Plantier, Christopher Smith
Renormalization and Factorization Scale-Invariant Predictions for the e+e- J/ψ+ηc process at B factories
Si-Qi Gong, Ting Sun, Sheng-Quan Wang et al.
Probing the Spatial Coherence of Chiral-Imbalance Fluctuations with Hyperon Spin Correlations
Guangyu Zheng, Zilin Yuan, Mei Huang et al.
Unitary KK and Kπ inputs for an amplitude analysis of the D+ K-K+π+ decay
Felipe C. L. Lopes, Patrícia C. Magalhães, Gustavo A. Loachamin O
Next-to-leading order QCD corrections to fully charm tetraquark radiative decays
Xiang Li, Yan-Qing Ma, Bo-Xuan Shi et al.
DAMA/LIBRA dark matter signal: a global analysis
Matti Heikinheimo, Sebastian Sassi, Alex Stendahl et al.