<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">445386754</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180317143034.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170323e20111001xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/s10714-011-1199-1</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/s10714-011-1199-1</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="4">
   <subfield code="a">The value of the cosmological constant</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[John Barrow, Douglas Shaw]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">We make the cosmological constant, Λ, into a field and restrict the variations of the action with respect to it by causality. This creates an additional Einstein constraint equation. It restricts the solutions of the standard Einstein equations and is the requirement that the cosmological wave function possess a classical limit. When applied to the Friedmann metric it requires that the cosmological constant measured today, t U , be $${\Lambda \sim t_{U}^{-2} \sim 10^{-122}}$$ , as observed. This is the classical value of Λ that dominates the wave function of the universe. Our new field equation determines Λ in terms of other astronomically measurable quantities. Specifically, it predicts that the spatial curvature parameter of the universe is $${\Omega _{\mathrm{k0}} \equiv -k/a_{0}^{2}H^{2}=-0.0055}$$ , which will be tested by Planck Satellite data. Our theory also creates a new picture of self-consistent quantum cosmological history.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Springer Science+Business Media, LLC, 2011</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Cosmology</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Cosmological constant</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Dark energy</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Barrow</subfield>
   <subfield code="D">John</subfield>
   <subfield code="u">DAMTP, Centre for Mathematical Sciences, Cambridge University, CB3 0WA, Cambridge, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Shaw</subfield>
   <subfield code="D">Douglas</subfield>
   <subfield code="u">DAMTP, Centre for Mathematical Sciences, Cambridge University, CB3 0WA, Cambridge, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">General Relativity and Gravitation</subfield>
   <subfield code="d">Springer US; http://www.springer-ny.com</subfield>
   <subfield code="g">43/10(2011-10-01), 2555-2560</subfield>
   <subfield code="x">0001-7701</subfield>
   <subfield code="q">43:10&lt;2555</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">43</subfield>
   <subfield code="o">10714</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/s10714-011-1199-1</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1007/s10714-011-1199-1</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Barrow</subfield>
   <subfield code="D">John</subfield>
   <subfield code="u">DAMTP, Centre for Mathematical Sciences, Cambridge University, CB3 0WA, Cambridge, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Shaw</subfield>
   <subfield code="D">Douglas</subfield>
   <subfield code="u">DAMTP, Centre for Mathematical Sciences, Cambridge University, CB3 0WA, Cambridge, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">General Relativity and Gravitation</subfield>
   <subfield code="d">Springer US; http://www.springer-ny.com</subfield>
   <subfield code="g">43/10(2011-10-01), 2555-2560</subfield>
   <subfield code="x">0001-7701</subfield>
   <subfield code="q">43:10&lt;2555</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">43</subfield>
   <subfield code="o">10714</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
