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In this thesis project, the geometry of homogeneous and isotropic universe, which can <br /> <br /> <br /> be represented in Robertson-Walker metric, is discussed. This metric is applied to <br /> <br /> <br /> solve Einstein’s field equation, and the solut...
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| Format: | Final Project |
| Language: | Indonesia |
| Online Access: | https://digilib.itb.ac.id/gdl/view/16018 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |
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id-itb.:160182017-09-27T11:45:09Z#TITLE_ALTERNATIVE# MUTTAQIN (NIM 102 03 050) ; pembimbing : Pembimbing : Bobby Eka Gunara, Dr.rer.nat, IMAMAL Indonesia Final Project INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/16018 In this thesis project, the geometry of homogeneous and isotropic universe, which can <br /> <br /> <br /> be represented in Robertson-Walker metric, is discussed. This metric is applied to <br /> <br /> <br /> solve Einstein’s field equation, and the solution is called as Friedmann equation. In <br /> <br /> <br /> the Friedmann equation, there are three main parameters. First, scale factor of the <br /> <br /> <br /> universe R(t), which describes the expantion rate of our universe. Second, curvature <br /> <br /> <br /> index k, which describes the geometry of our universe. Third, cosmological constant <br /> Λ which is a correction of Einstein field equation. Finally, we discuss possible <br /> <br /> <br /> universe model appeared in the model. text |
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Institut Teknologi Bandung |
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| continent |
Asia |
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Indonesia Indonesia |
| content_provider |
Institut Teknologi Bandung |
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| language |
Indonesia |
| description |
In this thesis project, the geometry of homogeneous and isotropic universe, which can <br />
<br />
<br />
be represented in Robertson-Walker metric, is discussed. This metric is applied to <br />
<br />
<br />
solve Einstein’s field equation, and the solution is called as Friedmann equation. In <br />
<br />
<br />
the Friedmann equation, there are three main parameters. First, scale factor of the <br />
<br />
<br />
universe R(t), which describes the expantion rate of our universe. Second, curvature <br />
<br />
<br />
index k, which describes the geometry of our universe. Third, cosmological constant <br />
Λ which is a correction of Einstein field equation. Finally, we discuss possible <br />
<br />
<br />
universe model appeared in the model. |
| format |
Final Project |
| author |
MUTTAQIN (NIM 102 03 050) ; pembimbing : Pembimbing : Bobby Eka Gunara, Dr.rer.nat, IMAMAL |
| spellingShingle |
MUTTAQIN (NIM 102 03 050) ; pembimbing : Pembimbing : Bobby Eka Gunara, Dr.rer.nat, IMAMAL #TITLE_ALTERNATIVE# |
| author_facet |
MUTTAQIN (NIM 102 03 050) ; pembimbing : Pembimbing : Bobby Eka Gunara, Dr.rer.nat, IMAMAL |
| author_sort |
MUTTAQIN (NIM 102 03 050) ; pembimbing : Pembimbing : Bobby Eka Gunara, Dr.rer.nat, IMAMAL |
| title |
#TITLE_ALTERNATIVE# |
| title_short |
#TITLE_ALTERNATIVE# |
| title_full |
#TITLE_ALTERNATIVE# |
| title_fullStr |
#TITLE_ALTERNATIVE# |
| title_full_unstemmed |
#TITLE_ALTERNATIVE# |
| title_sort |
#title_alternative# |
| url |
https://digilib.itb.ac.id/gdl/view/16018 |
| _version_ |
1820737602620227584 |