ERD

grackle: a chemistry and cooling library for astrophysics

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Rapid formation of massive black holes in close proximity to embryonic protogalaxies

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Periodic Reporting for period 1 - SmartStars (Pathways towards forming super-massive black holes in the early Universe)

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

The Sherwood simulation suite: overview and data comparisons with the Lyman α forest at redshifts 2 ≤ z ≤ 5

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

An analytic resolution to the competition between Lyman–Werner radiation and metal winds in direct collapse black hole...

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

The growth of black holes from Population III remnants in the Renaissance simulations

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

The formation of direct collapse black holes under the influence of streaming velocities

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Gravitational wave signals from the first massive black hole seeds

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Fragmentation inside atomic cooling haloes exposed to Lyman–Werner radiation

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Rise of the first supermassive stars

Project: SmartStars

Updated at: 28-04-2024

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Project acronym SmartStars

Resources

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grackle: a chemistry and cooling library for astrophysics

Rapid formation of massive black holes in close proximity to embryonic protogalaxies

Periodic Reporting for period 1 - SmartStars (Pathways towards forming super-massive black holes in the early Universe)

The Sherwood simulation suite: overview and data comparisons with the Lyman α forest at redshifts 2 ≤ z ≤ 5

An analytic resolution to the competition between Lyman–Werner radiation and metal winds in direct collapse black hole...

The growth of black holes from Population III remnants in the Renaissance simulations

The formation of direct collapse black holes under the influence of streaming velocities

Gravitational wave signals from the first massive black hole seeds

Fragmentation inside atomic cooling haloes exposed to Lyman–Werner radiation

Rise of the first supermassive stars