Probing large-scale filaments with H I and 3He II

Yoshitaka Takeuchi, Saleem Zaroubi, Naoshi Sugiyama

Research output: Contribution to journalArticlepeer-review


We explore the observability of the neutral hydrogen (H I) and the singly ionized isotope helium-3 (3He II) in the intergalactic medium (IGM) from the Epoch of Reionization down to the local Universe. The hyperfine transition of 3He II, which is not as well known as the H I transition, has energy splitting corresponding to 8 cm. It also has a larger spontaneous decay rate than that of neutral hydrogen, whereas its primordial abundance is much smaller. Although both species are mostly ionized in the IGM, the balance between ionization and recombination in moderately high-density regions renders them abundant enough to be observed. We estimate the emission signal of both hyperfine transitions from large-scale filamentary structures and discuss the prospects for observing them with current and future radio telescopes. We conclude that H I in filaments is possibly observable even with current telescopes after 100 h of observation. On the other hand, 3He II is only detectable with future telescopes, such as Square Kilometre Array, after the same amount of time.

Original languageEnglish
Pages (from-to)2236-2250
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Issue number3
StatePublished - 2014
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2014 The Authors.


  • Intergalactic medium
  • Large-scale structure of universe
  • Radio lines: General


Dive into the research topics of 'Probing large-scale filaments with H I and 3He II'. Together they form a unique fingerprint.

Cite this