Errata: Paramagnetism in Diamagnetic Molecules

Paramagnetism in color superconductivity and compact stars

It is quite plausible that color superconductivity occurs in the inner regions of neutron stars. At the same time, it is known that strong magnetic fields exist in the interior of these compact objects. In this paper we discuss some important effects that can occur in the color superconducting core of compact stars due to the presence of the stars’ magnetic field. In particular, we consider the...

Erratum/errata

Errata Slip

We thank our anonymous reviewers for their helpful feedback. This research was supported by the NSF under award DGE-1500084, CNS-1563848, CRI-1629851, CNS-1017265, CNS-0831300, and CNS-1149051, ONR under grant N000140911042 and N000141512162, DHS under contract No. N66001-12-C-0133, United States Air Force under contract No. FA865010-C-7025, DARPA under contract No. DARPA FA8650-15-C-7556, and ...

Diamagnetic GAM Drive Mechanism

GAMs oscillate between states of strong rotation and up-down asymmetric plasma compression. Hence, at first glance the natural turbulent drive (or damping) mechanisms for them is either a direct boost of the rotation – via Reynolds stress – or the creation of asymmetric pressure distributions – via transport. However, an up-down asymmetric pressure can also be created by the divergence of the d...

RFC 4460 SCTP Errata

This document is a compilation of issues found during six interoperability events and 5 years of experience with implementing, testing, and using Stream Control Transmission Protocol (SCTP) along with the suggested fixes. This document provides deltas to RFC 2960 and is organized in a time-based way. The issues are listed in the order they were brought up. Because some text is changed several t...