It is known that soft photon and graviton theorems can be regarded as the Ward-Takahashi identities of asymptotic symmetries. In this paper, we consider soft theorem for pions, i.e., Nambu-Goldstone b...
“Today I learned about Asymptotic Notation-the math behind analyzing an algorithm’s efficiency.”
Asymptotic notation is a way to describe how the running time or space requirement of an algorithm gro...
In this chapter, we review the state-of-the-art of black holes in asymptotically safe gravity. After a brief recap of the asymptotic safety program, we shall summarize derivations and features of the ...
We study the charge-to-mass ratios of BPS states in four-dimensional N = 2 supergravities arising from Calabi-Yau threefold compactifications of Type IIB string theory. We present a formula for the as...
We study the charge-to-mass ratios of BPS states in four-dimensional N = 2 supergravities arising from Calabi-Yau threefold compactifications of Type IIB string theory. We present a formula for the as...
In this chapter, we review the state-of-the-art of black holes in asymptotically safe gravity. After a brief recap of the asymptotic safety program, we shall summarize derivations and features of the ...
Asymptotically anti-de Sitter spacetimes are considered in a general dimension dicons/Journals/Common/ge" ALT="ge" ALIGN="TOP"/> 4. As one might expect, the boundary conditions at infinity ensure t...
The Asymptotic Iteration Method (AIM) is a technique for solving analytically and approximately the linear second-order differential equation, especially the eigenvalue problems that frequently appear...
We derive an asymptotic formula for operator product expansion coefficients of heavy operators in two dimensional conformal field theory. This follows from modular invariance of the genus two partitio...
The structure of the gravitational field at infinity of asymptotically anti-de Sitter space-times is analyzed in detail using conformal techniques. It is found that the situation differs from that in ...
Anti-de Sitter supergravity models are considered in three dimensions. Precise asymptotic conditions involving a chiral projection are given on the Rarita-Schwinger fields. Together with the known bou...
