Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ | Paper Citation Record

Observation b6a48b22-2cef-471a-b1f0-309a6bdccc52 · outbound

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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This paper cites Hlozek, J.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Hlozek, J

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Observation 1bd748b4-0c81-46a7-b167-4f9957d0f99b · outbound

This paper cites Constraining ultra slow roll inflation using cosmological datasets.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining ultra slow roll inflation using cosmological datasets

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Observation b8a388f6-a837-43b0-9790-c8d8210db343 · outbound

This paper cites Generalised constraints on the curvature perturbation from primordial black holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Generalised constraints on the curvature perturbation from primordial black holes

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Observation f5515e87-4136-47a5-a28c-3f5dc7d44da3 · outbound

This paper cites Constraints on the small scale curvature perturbation using Planck-2015 data.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraints on the small scale curvature perturbation using Planck-2015 data

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Observation ad118f31-2076-45e2-8a94-24735938af7c · outbound

This paper cites Constraints on the curvature power spectrum from primordial black hole evaporation.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraints on the curvature power spectrum from primordial black hole evaporation

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Observation 8433c3b1-612f-4d53-8243-e912de4c8f20 · outbound

This paper cites Sato-Polito, E.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Sato-Polito, E

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Observation 70e558fa-4fca-4481-bc46-07133988c996 · outbound

This paper cites Constraints on primordial black holes and curvature perturbations from the global 21cm signal.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraints on primordial black holes and curvature perturbations from the global 21cm signal

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Observation 648b329b-fcfb-487c-896f-46e729619f7c · outbound

This paper cites Primordial black holes in the Dark Ages: Observational prospects for future 21cm surveys.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Primordial black holes in the Dark Ages: Observational prospects for future 21cm surveys

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Observation e262ad52-e167-4e6a-8907-3edce3ed106d · outbound

This paper cites Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features

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This paper cites Ultra-Slow-Roll Inflation on the Lattice I: Backreaction and Nonlinear Effects.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Ultra-Slow-Roll Inflation on the Lattice I: Backreaction and Nonlinear Effects

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Observation dd66c4bf-560e-4e8f-95a8-521a31ff75ae · outbound

This paper cites Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Observation 3efb1b4c-fc7c-49ee-aa65-7eaa5f0094cf · outbound

This paper cites Investigating dark matter substructure with pulsar timing: II. Improved limits on small-scale cosmology.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Investigating dark matter substructure with pulsar timing: II. Improved limits on small-scale cosmology

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Observation 49b78386-e107-40dc-8894-ca5331d824c2 · outbound

This paper cites Gamma-rays from ultracompact minihalos: potential constraints on the primordial curvature perturbation.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Gamma-rays from ultracompact minihalos: potential constraints on the primordial curvature perturbation

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This paper cites A New Probe of Dark Matter and High-Energy Universe Using Microlensing.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ A New Probe of Dark Matter and High-Energy Universe Using Microlensing

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Observation ce74c746-2b8c-4ef7-8b93-150210dfdb65 · outbound

This paper cites Zhang, X.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Zhang, X

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Observation 6927231f-8aee-4ff6-bcf7-ba07bd50b21b · outbound

This paper cites Constraining the primordial black hole abundance through Big-Bang nucleosynthesis.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining the primordial black hole abundance through Big-Bang nucleosynthesis

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Observation a24e7014-d9e0-4ace-89bd-70e74a4b2b82 · outbound

This paper cites Do Black Holes Destroy Information?.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Do Black Holes Destroy Information?

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Observation 7a4e8d2c-ed46-45cb-bd6b-4fdf30648220 · outbound

This paper cites Black Hole Metamorphosis and Stabilization by Memory Burden.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Black Hole Metamorphosis and Stabilization by Memory Burden

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This paper cites A Microscopic Model of Holography: Survival by the Burden of Memory.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ A Microscopic Model of Holography: Survival by the Burden of Memory

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This paper cites Memory Burden Effect in Black Holes and Solitons: Implications for PBH.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Memory Burden Effect in Black Holes and Solitons: Implications for PBH

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Observation 0e175c9d-3995-403d-8276-c5a1bca43c5f · outbound

This paper cites Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate

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Observation c3c7f032-9558-452e-8a2d-a109404b775a · outbound

This paper cites Light burden of memory: Constraining primordial black holes with high-energy neutrinos.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Light burden of memory: Constraining primordial black holes with high-energy neutrinos

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Ultralight Black Holes as Sources of High-Energy Particles

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This paper cites Curvature profiles as initial conditions for primordial black hole formation.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Curvature profiles as initial conditions for primordial black hole formation

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining primordial black holes as dark matter using AMS-02 data

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Observation fc2c7095-04e4-4cf7-8ccb-fa34356371dc · outbound

This paper cites Prospects of Future CMB Anisotropy Probes for Primordial Black Holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Prospects of Future CMB Anisotropy Probes for Primordial Black Holes

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This paper cites Constraining Mixed Dark-Matter Scenarios of WIMPs and Primordial Black Holes from CMB and 21-cm observations.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining Mixed Dark-Matter Scenarios of WIMPs and Primordial Black Holes from CMB and 21-cm observations

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Observation 83ad3122-a551-4111-b878-403633a6c9d8 · outbound

This paper cites Constraining the primordial black hole abundance with 21cm cosmology.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining the primordial black hole abundance with 21cm cosmology

Reference 35

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Observation 5359f2a4-99f3-424e-944a-76783741f997 · outbound

This paper cites Constraining primordial black holes in dark matter with kinematics of dwarf galaxies.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraining primordial black holes in dark matter with kinematics of dwarf galaxies

Reference 36

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Observation 002cb7c0-a775-478d-9e86-e3e22c1fe756 · outbound

This paper cites Constraints on a mixed model of dark matter particles and primordial black holes from the Galactic 511 keV line.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraints on a mixed model of dark matter particles and primordial black holes from the Galactic 511 keV line

Reference 37

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Observation 14db325b-8a2f-496e-9752-0ef7f110d3cd · outbound

This paper cites Constraint on the abundance of primordial black holes in dark matter from Planck data.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Constraint on the abundance of primordial black holes in dark matter from Planck data

Reference 38

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Observation 84e8b5f1-32ae-47b5-9daa-3fb7180a3671 · outbound

This paper cites New X-ray bound on density of primordial black holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ New X-ray bound on density of primordial black holes

Reference 39

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Observation 44a70365-0156-4adb-856d-a3576aeae4e9 · outbound

This paper cites Cosmic microwave background limits on accreting primordial black holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Cosmic microwave background limits on accreting primordial black holes

Reference 40

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Observation 0a6c86d9-6413-4217-920b-f71e8b843403 · outbound

This paper cites 21cm Limits on Decaying Dark Matter and Primordial Black Holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ 21cm Limits on Decaying Dark Matter and Primordial Black Holes

Reference 41

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This paper cites NANOGrav Hints to Primordial Black Holes as Dark Matter.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ NANOGrav Hints to Primordial Black Holes as Dark Matter

Reference 42

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Observation 942cf04b-3e74-42f7-b84a-63d42a86bf78 · outbound

This paper cites The abundance of primordial black holes from the global 21cm signal and extragalactic gamma-ray background.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ The abundance of primordial black holes from the global 21cm signal and extragalactic gamma-ray background

Reference 43

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Observation f6813285-0318-4d01-9ad9-54f3483cccc4 · outbound

This paper cites Primordial Black Holes.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Primordial Black Holes

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ Unresolved cited work

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This paper cites The Giant Radio Array for Neutrino Detection (GRAND): Science and Design.

Constraints on the primordial curvature power spectrum at small scales between $3\times 10^{18}$ and $4.5\times 10^{21}~\rm Mpc^{-1}$ The Giant Radio Array for Neutrino Detection (GRAND): Science and Design

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