output
20122026
most citedDawes Review 4: Spiral Structures in Disc Galaxies

264 citations

Showing 2014Show all

18 papers · 1 filter

physics.optics2014★ 15 cited

Chaotic oscillation and random-number generation based on nanoscale optical-energy transfer

Makoto Naruse, Song-Ju Kim, Masashi Aono +2

By using nanoscale energy-transfer dynamics and density matrix formalism, we demonstrate theoretically and numerically that chaotic oscillation and random-number generation occur i…

physics.optics2014★ 37 cited

Decision making based on optical excitation transfer via near-field interactions between quantum dots

Makoto Naruse, Wataru Nomura, Masashi Aono +5

Optical near-field interactions between nanostructured matter, such as quantum dots, result in unidirectional optical excitation transfer when energy dissipation is induced. This r…

astro-ph.EP2014★ 35 cited

An updated estimate of the number of Jupiter-family comets using a simple fading law

R. Brasser, J. -H. Wang

It has long been hypothesised that the Jupiter-family comets (JFCs) come from the scattered disc, an unstable planetesimal population beyond Neptune. This viewpoint has been widely…

astro-ph.GA2014★ 38 cited

Kinematics of classical Cepheids in the Nuclear Stellar Disk

N. Matsunaga, K. Fukue, R. Yamamoto +13

Classical Cepheids are useful tracers of the Galactic young stellar population because their distances and ages can be determined from their period-luminosity and period-age relati…

astro-ph.EP2014★ 54 cited

Reassessing the formation of the Inner Oort cloud in an embedded star cluster II: Probing the inner edge

R. Brasser, M. E. Schwamb

The detached object Sedna is likely at the inner edge of the Oort cloud, more precisely the inner Oort cloud (IOC). Until recently it was the sole member of this population. The re…

astro-ph.EP2014★ 14 cited

Orbital Circularization of a Planet Accreting Disk Gas: Formation of Distant Jupiters in Circular Orbits based on Core Accretion Model

A. Kikuchi, A. Higuchi, S. Ida

Recently, gas giant planets in nearly circular orbits with large semimajor axes ( 30--1000AU) have been detected by direct imaging. We have investigated orbital evolution i…