Results 61 to 70 of about 1,220,618 (361)
The D^{2k} R^4 Invariants of N=8 Supergravity [PDF]
JHEP 1104:006,2011, 2011 The existence of a linearized SUSY invariant for N=8 supergravity whose gravitational components are usually called R^4 was established long ago by on-shell superspace arguments. Superspace and string theory methods have also established analogous higher dimensional D^{2k} R^4 invariants.
arxiv +1 more source
A double-label study of efferent projections from the Edinger-Westphal nucleus in goldfish and kelp bass [PDF]
, 1988 The Edinger-Westphal nucleus in goldfish was identified by retrograde labeling from the ciliary ganglion. In the same animals a few neurons near this nucleus (perinuclear Edinger-Westphal neurons) were labeled by a different retrograde tracer injected ...
Akert +22 more
core +1 more source
Advanced Engineering Materials, EarlyView.Herein the metal‐to‐insulator transition is investigated when depositing vanadium dioxide (VO2) on glass or aluminum‐doped zinc oxide (AZO). O2 flow tuning during the deposition and additional post annealing are effective to control the metal‐to‐insulator transition. However, the VO2/AZO/glass stack reveals an increase in the transition temperature and
Eduard Llorens Balada +3 more
wiley +1 more source
Collisional invariants for the phonon Boltzmann equation [PDF]
, 2006 For the phonon Boltzmann equation with only pair collisions we characterize the set of all collisional invariants under some mild conditions on the dispersion relation.
arxiv +1 more source
One method for constructing exact solutions of equations of two-dimensional hydrodynamics of an incompressible fluid [PDF]
Theoretical and Mathematical Physics Volume 147, Number 1,
501-508, (2006) DOI: 10.1007/s11232-006-0057-x, 2012 We propose a simple algebraic method for constructing exact solutions of equations of two-dimensional hydrodynamics of an incompressible fluid. The problem reduces to consecutively solving three linear partial differential equations for a nonviscous fluid and to solving three linear partial differential equations and one first-order ordinary ...
arxiv +1 more source
Student Understanding of Rotational and Rolling Motion Concepts [PDF]
, 2007 Provides pedagogical insight concerning learners' pre-conceptions and misconceptions about torque and rolling motion The resource being annotated is: http://www.dlese.org/dds/catalog_DLESE-000-000-006-235 ...
Lamont-Doherty Earth Observatory, Columbia University
core
Entanglement amplification of fermionic systems in an accelerated frame
, 2012 In this article we present an analysis to derive physical results in the entanglement amplification of fermonic systems in the relativistic regime, that is, beyond the single-mode approximation. This leads a recent work in [M. Montero and E.
Chang, Jinho, Kwon, Younghun
core +2 more sources
The functional role of GABA and glycine in monaural and binaural processing in the inferior colliculus of horseshoe bats [PDF]
, 1992 The functional role of GABA and glycine in monaural and binaural signal analysis was studied in single unit recordings from the central nucleus of the inferior colliculus (IC) of horseshoe bats (Rhinolophus rouxi) employing microiontophoresis of the ...
Grothe, Benedikt +3 more
core +1 more source
Advanced Engineering Materials, EarlyView.This article presents the development of Fe‐Mn‐Zn nanocrystalline alloys (0–9 wt% Zn) by mechanical alloying and subsequently hot pressing. Their microstructure, density, hardness, wear resistance, corrosion behavior, and antibacterial properties are systematically examined.
Ilker Emin Dag +3 more
wiley +1 more source
GSH 006-15+7: A local Galactic supershell featuring transition from HI emission to absorption [PDF]
, 2012 We report on the discovery of a new Galactic supershell, GSH 006-15+7, from the Galactic All Sky Survey data. Observed and derived properties are presented and we find that GSH 006-15+7 is one of the nearest physically large supershells known, with dimensions of ~ 780 x 520 pc at a distance of ~ 1.5 kpc. The shell wall appears in HI emission at b <~ -6.
arxiv +1 more source