activity
20042026
most citedRealization of quantum walks with negligible decoherence in waveguide lattices

538 citations · 8.5k across the 174 of their papers we have counts for

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Showing 2018 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2018★ 95 cited

Quasi-secular evolution of mildly hierarchical triple systems: analytics and applications for GW-sources and hot Jupiters

Evgeni Grishin, Hagai B. Perets, Giacomo Fragione

In hierarchical triple systems, the inner binary is perturbed by a distant companion. For large mutual inclinations, the Lidov-Kozai mechanism secularly excites large eccentricity…

astro-ph.EP2018★ 20 cited

The role of multiple giant impacts in the formation of the Earth-Moon system

Robert I. Citron, Hagai B. Perets, Oded Aharonson

The Earth-Moon system is suggested to have formed through a single giant collision, in which the Moon accreted from the impact-generated debris disk. However, such giant impacts ar…

astro-ph.EP2018★ 14 cited

Gas-Assisted Growth of Protoplanets in a Turbulent Medium

M. M. Rosenthal, R. A. Murray-Clay, H. B. Perets +1

Pebble accretion is a promising process for decreasing growth timescales of planetary cores, allowing gas giants to form at wide orbital separations. However, nebular turbulence ca…

astro-ph.EP2018★ 29 cited

Statistical Trends in the Obliquity Distribution of Exoplanet Systems

Diego J. Muñoz, Hagai B. Perets

Important clues on the formation and evolution of planetary systems can be inferred from the stellar obliquity . We study the distribution of obliquities using the California-Ke…

astro-ph.EP2018★ 9 cited

Moonfalls: Collisions between the Earth and its past moons

Uri Malamud, Hagai B. Perets, Christoph Schafer +1

During the last stages of the terrestrial planet formation, planets grow mainly through giant-impacts with large planetary embryos. The Earth's Moon was suggested to form through o…

astro-ph.EP2018★ 25 cited

Planet seeding through gas-assisted capture of interstellar objects

Evgeni Grishin, Hagai B. Perets, Yael Avni

Planet formation begins with collisional growth of small planetesimals accumulating into larger ones. Such growth occurs while planetesimals are embedded in a gaseous protoplanetar…