Results 101 to 110 of about 10,473 (185)
Symmetry TFTs from String Theory. [PDF]
Commun Math Phys, 2023 Apruzzi F +4 more
europepmc +1 more source
Effect of the supergravity on the formation and cycle life of non-aqueous lithium metal batteries. [PDF]
Nat Commun, 2022 Gao Y +8 more
europepmc +1 more source
Aether, dark energy and string compactifications. [PDF]
Philos Trans A Math Phys Eng Sci, 2022 Townsend PK.
europepmc +1 more source
Matter coupling in higher derivative supergravity
, 1986 This book is a collection of reprints on the structure of Poincar, anti-de Sitter and conformal supergravity theories in one to eleven dimensions, their anomalies and compactification.
PASQUINUCCI A +10 more
core +1 more source
Gravity in spacetimes with cosmological constants [PDF]
, 2009 This thesis is composed of two parts: gravity in the spacetime with a negative/positive cosmological constant. The first part, which is the negative case, devotes to constructing the IIB supergravity dual solution in AdS/CFT correspondence for N = (1, 0)
Dai, Shou-Huang
core
Higgs effect without lunch. [PDF]
Philos Trans A Math Phys Eng Sci, 2022 Erickson CW, Leung R, Stelle KS.
europepmc +1 more source
Non-static brane probes, topological charges and calibrations [PDF]
, 2004 In this thesis we consider probe branes in 10- and 11-dimensional supergravity backgrounds. Firstly, we consider probing a class of 11-dimensional backgrounds with giant gravitons. These backgrounds arise from lifting solutions of 4-dimensional U(1)(^4)
Hackett-Jones, Emily Jane
core
Emergent Sasaki-Einstein geometry and AdS/CFT. [PDF]
Nat Commun, 2022 Berman RJ, Collins TC, Persson D.
europepmc +1 more source
Machine learning supergravity vacua [PDF]
openIn this thesis we study maximally symmetric vacua for maximal supergravity in 4D. We will begin by showing that the structure of those vacua is determined by the gauging procedure.
COSTANTINI, RICCARDO
core
Brans-Dicke supergravity and the Lambda naturalness problem [PDF]
, 2015 The successful $\Lambda CDM$ cosmological model requires a small but nonzero $\Lambda$ which appears to have an unnaturally small value compared to the supersymmetry breaking scale, typically $O(10^{-60}) m_{3/2}^4$ for $m_{3/2} \sim 10 TeV$.
Hewitt, M.
core