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Results 1 - 20 of 89  for All Library Resources

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1
New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasets
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New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasets

arXiv.org, 2019-03

2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1903.05645

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2
Comparing Dark Energy models with Hubble versus Growth Rate data
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Comparing Dark Energy models with Hubble versus Growth Rate data

arXiv.org, 2018-08

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1808.05660

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3
Perturbations in Tachyon Dark Energy and their Effect on Matter Clustering
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Perturbations in Tachyon Dark Energy and their Effect on Matter Clustering

arXiv.org, 2020-05

2020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1907.13309

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4
Validating the methodology for constraining the linear growth rate from clustering anisotropies
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Validating the methodology for constraining the linear growth rate from clustering anisotropies

arXiv.org, 2020-03

2020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1909.08016

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5
Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
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Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys

arXiv.org, 2020-02

2020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1905.05122

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6
A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
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A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids

arXiv.org, 2018-10

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1805.09349

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7
The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
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The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions

arXiv.org, 2019-08

2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1810.05183

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8
Synergies between radio, optical and microwave observations at high redshift
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Synergies between radio, optical and microwave observations at high redshift

arXiv.org, 2019-06

2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1810.00911

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9
Modelling the environmental dependence of the growth rate
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Article
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Modelling the environmental dependence of the growth rate

arXiv.org, 2018-06

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1806.04684

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10
Growth of perturbations in dark energy parametrization scenarios
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Growth of perturbations in dark energy parametrization scenarios

arXiv.org, 2018-04

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1804.09886

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11
Deconstructing the neutrino mass constraint from galaxy redshift surveys
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Deconstructing the neutrino mass constraint from galaxy redshift surveys

arXiv.org, 2018-03

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1712.01857

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12
Uneven flows: On cosmic bulk flows, local observers, and gravity
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Article
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Uneven flows: On cosmic bulk flows, local observers, and gravity

arXiv.org, 2018-02

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1802.03391

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13
Growth of matter perturbations in non-minimal teleparallel dark energy
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Growth of matter perturbations in non-minimal teleparallel dark energy

arXiv.org, 2018-11

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1807.10167

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14
Information Content of the Angular Multipoles of Redshift-Space Galaxy Bispectrum
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Article
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Information Content of the Angular Multipoles of Redshift-Space Galaxy Bispectrum

arXiv.org, 2016-12

2016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1610.03488

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15
Measuring the Universe with galaxy redshift surveys
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Article
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Measuring the Universe with galaxy redshift surveys

arXiv.org, 2018-03

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1803.10814

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16
Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
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Article
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Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions

arXiv.org, 2017-03

2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1606.03092

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17
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
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Article
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2

arXiv.org, 2018-01

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1801.03062

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18
Can Holographic dark energy models fit the observational data?
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Article
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Can Holographic dark energy models fit the observational data?

arXiv.org, 2018-10

2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1809.08792

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19
Validating estimates of the growth rate of structure with modified gravity simulations
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Article
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Validating estimates of the growth rate of structure with modified gravity simulations

arXiv.org, 2016-11

2016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1605.03965

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20
Hidden Charged Dark Matter and Chiral Dark Radiation
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Article
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Hidden Charged Dark Matter and Chiral Dark Radiation

arXiv.org, 2017-09

2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1706.05605

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