activity
20152026
most citedNLTE and LTE Lick indices for red giants from [M/H] 0.0 to -6.0 at SDSS and IDS spectral resolution

4 citations · 4 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2026

A Complete Invariant Analysis of the Kerr Spacetime and its Photon Region

Nicholas Layden, Dipanjan Dey, Alan Coley

We present an invariant characterization of the Kerr spacetime, and utilize the invariant structure of the spacetime to derive a function whose zeros identify a special family of n…

gr-qc2024

The Definition of a Photon Surface in an Invariant Spin Frame

Dipanjan Dey, Alan A. Coley, Nicholas T. Layden

This paper defines the photon surface conditions using Cartan scalars within an invariant spin frame, offering a comprehensive description of the local spacetime geometry. By emplo…

gr-qc2023

Invariant description of static and dynamical Brans-Dicke spherically symmetric models

Nicholas Layden, Alan Coley, Dipanjan Dey

We investigate spherically symmetric static and dynamical Brans-Dicke theory exact solutions using invariants and, in particular, the Newman Penrose formalism utilizing Cartan scal…

gr-qc2023

The equilibrium condition in gravitational collapse and its application to a cosmological scenario

Dipanjan Dey, N. T. Layden, A. A. Coley +1

We discuss the equilibrium conditions of the gravitational collapse of a spherically symmetric matter cloud. We analyze the spinor structure of a general collapsing space-time and…

gr-qc2021

An invariant characterization of the quasi-spherical Szekeres dust models

A. A. Coley, N. Layden, D. D. McNutt

The quasi-spherical Szekeres dust solutions are a generalization of the spherically symmetric Lemaitre-Tolman-Bondi dust models where the spherical shells of constant mass are non-…

astro-ph.SR2015★ 4 cited

NLTE and LTE Lick indices for red giants from [M/H] 0.0 to -6.0 at SDSS and IDS spectral resolution

C. Ian Short, Mitchell E. Young, Nicholas Layden

We investigate the dependence of the complete system of 22 Lick indices on overall metallicity scaled from solar abundances, [M/H], from the solar value, 0.0, down to the extremely…