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Dark radiation from particle decays during big bang nucleosynthesis

dc.contributor.advisorScherrer, Robert J. (Robert Joseph), 1959-
dc.contributor.authorMenestrina, Justin
dc.date.accessioned2012-06-01T17:44:59Z
dc.date.available2012-06-01T17:44:59Z
dc.date.issued2012-04
dc.identifier.urihttp://hdl.handle.net/1803/5098
dc.description.abstractCosmic microwave background (CMB) observations suggest the possibility of an extra dark radiation component, while the current evidence from big bang nucleosynthesis (BBN) is more ambiguous. Dark radiation from a decaying particle can affect these two processes differently. Early decays add an additional radiation component to both the CMB and BBN, while late decays can alter the radiation content seen in the CMB while having a negligible effect on BBN. Here we quantify this difference and explore the intermediate regime by examining particles decaying during BBN, i.e., particle lifetimes τ_X satisfying 0.1 sec < τ_X < 1000 sec. We calculate the change in the effective number of neutrino species, Neff, as measured by the CMB, ΔN_CMB, and the change in the effective number of neutrino species as measured by BBN, ΔN_BBN, as a function of the decaying particle initial energy density and lifetime, where DNBBN is defined in terms of the number of additional two-component neutrinos needed to produce the same change in the primordial 4He abundance as our decaying particle. As expected, for short lifetimes (τ_X < 0.1 sec), the particles decay before the onset of BBN, and DNCMB = DNBBN, while for long lifetimes (τ_X >1000 sec), ΔN_BBN is dominated by the energy density of the nonrelativistic particles before they decay, so that ΔN_BBN remains nonzero and becomes independent of the particle lifetime. By varying both the particle energy density and lifetime, one can obtain any desired combination of N_BBN and ΔN_CMB, subject to the constraint that DNCMB N_BBN. We present limits on the decaying particle parameters derived from observational constraints on ΔN_CMB, and N_BBN.en_US
dc.language.isoen_USen_US
dc.publisherVanderbilt University. Dept. of Physics and Astronomyen_US
dc.subjectCosmologyen_US
dc.subjectBig Bang Nucleosynthesisen_US
dc.subjectCosmic Microwave Backgrounden_US
dc.subjectDark Radiationen_US
dc.subjectEffective Neutrino Numberen_US
dc.subject.lcshCosmologyen_US
dc.subject.lcshCosmic background radiationen_US
dc.subject.lcshBig bang theoryen_US
dc.subject.lcshDark matter (Astronomy)en_US
dc.subject.lcshDark energy (Astronomy)en_US
dc.subject.lcshNucleosynthesisen_US
dc.subject.lcshRadioactive decayen_US
dc.titleDark radiation from particle decays during big bang nucleosynthesisen_US
dc.typeThesisen_US
dc.description.collegeCollege of Arts and Scienceen_US
dc.description.departmentDept. of Physics and Astronomyen_US


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