Asymptotically flat spacetimes in three dimensional higher spin gravity

MD simulations in this and previous work has allowed us to propose a relation between the nature of the interactions at the interface and the observed properties of nanofluids:

The results also indicate that although the PPML is less affected by heteroskedasticity than other estimators, its performance is similar, in terms of bias and

Inspired by our previous similar work on f ðRÞ gravity [18], we extend it to the case of f ðTÞ gravity models and use the standard joint likelihood analysis of the recent

Let us now explore the consequences of (6.10); we will take τ = 2π iβ in what follows, so that we have an ordinary partition function. In other words, in the high temperature

NECESSARY AND SUFFICIENT CONDITIONS FOR THE APPEARANCE OF A HETEROCLINIC CONTOUR Necessary and sufficient conditions for the continuous counterpart of (1) in the three-dimensional

the trace and diffoemorphism anomalies in chiral CFTs, but the mechanism for higher spin is different since the identity operator cannot appear in the OPE of the higher spin

To be eligible for inclusion in our meta-analysis, studies had to fulfill the following requirements: (a) the type of sample must include at least a nonclinical

There can be no doubt that a higher-dimensional coun- terpart of this infinite symmetry would provide novel insights into the analysis and formulation of new non-linear