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  • During the epoch of first star formation, molecular hydrogen (H-2) generated via associative detachment (AD) of H- and H is believed to have been the main coolant of primordial gas for temperatures below 10(4) kelvin. The uncertainty in the cross section for this reaction has limited our understanding of protogalaxy formation during this epoch and of the characteristic masses and cooling times for the first stars. We report precise energy-resolved measurements of the AD reaction, made with the use of a specially constructed merged-beams apparatus. Our results agreed well with the most recent theoretically calculated cross section, which we then used in cosmological simulations to demonstrate how the reduced AD uncertainty improves constraints of the predicted masses for Population III stars.
  • During the epoch of first star formation, molecular hydrogen (H-2) generated via associative detachment (AD) of H- and H is believed to have been the main coolant of primordial gas for temperatures below 10(4) kelvin. The uncertainty in the cross section for this reaction has limited our understanding of protogalaxy formation during this epoch and of the characteristic masses and cooling times for the first stars. We report precise energy-resolved measurements of the AD reaction, made with the use of a specially constructed merged-beams apparatus. Our results agreed well with the most recent theoretically calculated cross section, which we then used in cosmological simulations to demonstrate how the reduced AD uncertainty improves constraints of the predicted masses for Population III stars. (en)
Title
  • Experimental Results for H-2 Formation from H- and H and Implications for First Star Formation
  • Experimental Results for H-2 Formation from H- and H and Implications for First Star Formation (en)
skos:prefLabel
  • Experimental Results for H-2 Formation from H- and H and Implications for First Star Formation
  • Experimental Results for H-2 Formation from H- and H and Implications for First Star Formation (en)
skos:notation
  • RIV/00216208:11320/10:10079249!RIV11-GA0-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA202/07/0833), Z(MSM0021620860)
http://linked.open...iv/cisloPeriodika
  • 5987
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 258327
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/10:10079249
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • star formation; associative detachment; merged-beams experiments (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [FA6578FED2DB]
http://linked.open...i/riv/nazevZdroje
  • Science
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 329
http://linked.open...iv/tvurceVysledku
  • Bruhns, H.
  • Kreckel, H.
  • Miller, K. A.
  • Savin, D. W.
  • Urbain, X.
  • Čížek, Martin
  • Glover, S. C. O.
http://linked.open...ain/vavai/riv/wos
  • 000279402700033
http://linked.open...n/vavai/riv/zamer
issn
  • 0036-8075
number of pages
http://localhost/t...ganizacniJednotka
  • 11320
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