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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01k3569668p
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dc.contributorJones, William C.-
dc.contributor.advisorPretorius, Frans-
dc.contributor.authorMoreno, Ignacio-
dc.date.accessioned2015-07-27T13:29:39Z-
dc.date.available2015-07-27T13:29:39Z-
dc.date.created2015-05-04-
dc.date.issued2015-07-27-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01k3569668p-
dc.description.abstractWe study the process of black hole formation caused from colliding gravitational compact objects (particles or stars). The collision of compact objects is modeled as self-gravitating fluid accompanied by a plane gravitational wave. It is theorized that when two gravitational waves collide they can produce produce a black hole, but the exact process explaining this phenomenon is not completely known. One possible explanation is the focusing effect that gravitational wave has on particles moving through it. Our thesis will run simulations exploring the effects of focusing on black hole formation for different gravitational wave distributions. Our results show that focusing plays a major role in the formation of black holes when two gravitational wave collide.en_US
dc.format.extent46 pagesen_US
dc.language.isoen_USen_US
dc.titleGravitational Waves and Black Hole Formationen_US
dc.typePrinceton University Senior Theses-
pu.date.classyear2015en_US
pu.departmentPhysicsen_US
pu.pdf.coverpageSeniorThesisCoverPage-
Appears in Collections:Physics, 1936-2020

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