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        <datestamp>2023-07-11</datestamp>
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          <dc:contributor>Benjamin Wandelt</dc:contributor>
          <dc:creator>Yadav, Amit P.S.</dc:creator>
          <dc:date>2015-09-25T22:35:40Z</dc:date>
          <dc:date>2015-09-25T22:35:40Z</dc:date>
          <dc:date>10000-01-01</dc:date>
          <dc:date>2008</dc:date>
          <dc:date>2008</dc:date>
          <dc:description>Finally, using our estimator we found (Yadav and Wandelt 2008) evidence for primordial non-Gaussianity of the local type (fNL) in the temperature anisotropy of the Cosmic Microwave Background. Analyzing the bispectrum of the WMAP 3-year data up to lmax=750 we find 27&lt; fNL&lt;147 (95% CL). This amounts to a rejection of fNL=0 at 2.8sigma, disfavoring canonical single field slow-roll inflation. The signal is robust to variations in lmax , frequency, and masks. No known foreground, instrument systematic, or secondary anisotropy explains it. We explore the impact of several analysis choices on the quoted significance and find 2.5sigma to be conservative.</dc:description>
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  Previous issue date: 2008</dc:description>
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Lift date: Forever
Reason: Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs</dc:description>
          <dc:description>Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs</dc:description>
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          <dc:description>111 p.</dc:description>
          <dc:description>Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2008.</dc:description>
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          <dc:language>eng</dc:language>
          <dc:subject>Physics, Astronomy and Astrophysics</dc:subject>
          <dc:title>Probing the Cosmological Initial Conditions Using the CMB</dc:title>
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            <department>Astronomy</department>
            <discipline>Astronomy</discipline>
            <grantor>University of Illinois at Urbana-Champaign</grantor>
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