PIXIE
(Primordial Inflation Explorer)
(satellite-concept to to survey CMB polarization)
PIXIE (for Primordial Inflation Explorer) is a 2011 proposal
for a NASA Explorers Program mission intended to
survey CMB polarization, using a
nulling polarimeter.
Of particular interest are B-mode polarization modes
that are expected to be the imprint of primordial gravitational waves
caused by inflation.
It covers a substantial frequency-range,
from microwave to far infrared (30 GHz to 6 THz), also allowing it to
carry out intensity mapping of redshifted
C+, N+, and CO lines.
(NASA,spacecraft,CMB,plan)
Further reading:
https://ui.adsabs.harvard.edu/abs/2011JCAP...07..025K/abstract
https://ui.adsabs.harvard.edu/abs/2019BAAS...51g.113K/abstract
https://asd.gsfc.nasa.gov/pixie/
https://physics.richmond.edu/rsb-conference/presentation-pdfs/RSB%20-%20Kogut%20PIXIE.pdf
| WaveL | Freq | Photon
Energy | | |
| 50μm | 6THz | 25meV | begin | PIXIE |
| 10mm | 30GHz | 124μeV | end | PIXIE |
|
Referenced by page:
primordial gravitational waves
Index