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Robert M. Cross

Researcher at University of Rochester

Publications -  13
Citations -  368

Robert M. Cross is an academic researcher from University of Rochester. The author has contributed to research in topics: Random walk & Photon. The author has an hindex of 4, co-authored 11 publications receiving 62 citations. Previous affiliations of Robert M. Cross include Louisiana State University.

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The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

The Astropy Collaboration, +135 more
TL;DR: Astropy as mentioned in this paper is a Python package that provides commonly needed functionality to the astronomical community, such as astronomy, astronomy, and astronomy data visualization, as well as other related projects and packages.
Journal ArticleDOI

Inefficiency of classically simulating linear optical quantum computing with Fock-state inputs

TL;DR: Aaronson and Arkhipov as mentioned in this paper constructed the Hilbert space for a quantum-optical interferometer and showed that its dimension scales exponentially with all the physical resources, and compared the symmetry requirements of a multiparticle bosonic to fermionic interferometers and, using simple physical reasoning, connect the nonsimulatability of the bosonic device to the complexity of computing the permanent of a large matrix.
Journal Article

Quantum random walks with multiphoton interference and high order correlation functions

TL;DR: In this article, a simulation of quantum random walks (QRWs) with multiple photons using a staggered array of 50/50 beam splitters with a bank of detectors at any desired level is presented.
Journal ArticleDOI

Quantum random walks with multiphoton interference and high-order correlation functions

TL;DR: In this paper, a simulation of quantum random walks (QRWs) with multiple photons using a staggered array of 50/50 beam splitters with a bank of detectors at any desired level is presented.
Proceedings ArticleDOI

Eleven Year Search for Supernovae with the IceCube Neutrino Observatory

TL;DR: In this article, the tools and the method to study potential obscured or failed core collapse supernovae in our Galaxy are presented, based on 3911 days of IceCube data taken between April 17, 2008 and December 31, 2018.