TY - JOUR
T1 - Cold atom clocks and applications
AU - Bize, S.
AU - Laurent, P.
AU - Abgrall, M.
AU - Marion, H.
AU - Maksimovic, I.
AU - Cacciapuoti, L.
AU - Grunert, J.
AU - Vian, C.
AU - Pereira Dos Santos, F.
AU - Rosenbusch, P.
AU - Lemonde, P.L.
AU - Santarelli, G.
AU - Wolf, P.
AU - Clarion, A.
AU - Luiten, Andre
AU - Tobar, Michael
AU - Salomon, C.
PY - 2005
Y1 - 2005
N2 - This paper describes advances in microwave frequency standards using laser-cooled atoms at BNM-SYRTE. First, recent improvements of the Cs-133 and Rb-87 atomic fountains are described. Thanks to the routine use of a cryogenic sapphire oscillator as an ultra-stable local frequency reference, a fountain frequency instability of 1.6 x 10(-14) iota(-1/2) where iota is the measurement time in seconds is measured. The second advance is a powerful method to control the frequency shift due to cold collisions. These two advances lead to a frequency stability of 2 x 10(-16) at 50 000 s for the first time for primary standards. In addition, these clocks realize the SI second with an accuracy of 7 x 10-16, one order of magnitude below that of uncooled devices. In a second part, we describe tests of possible variations of fundamental constants using 87Rb and (CS)-C-133 fountains. Finally we give an update on the cold atom space clock PHARAO developed in collaboration with CNES. This clock is one of the main instruments of the ACES/ESA mission which is scheduled to fly on board the International Space Station in 2008, enabling a new generation of relativity tests.
AB - This paper describes advances in microwave frequency standards using laser-cooled atoms at BNM-SYRTE. First, recent improvements of the Cs-133 and Rb-87 atomic fountains are described. Thanks to the routine use of a cryogenic sapphire oscillator as an ultra-stable local frequency reference, a fountain frequency instability of 1.6 x 10(-14) iota(-1/2) where iota is the measurement time in seconds is measured. The second advance is a powerful method to control the frequency shift due to cold collisions. These two advances lead to a frequency stability of 2 x 10(-16) at 50 000 s for the first time for primary standards. In addition, these clocks realize the SI second with an accuracy of 7 x 10-16, one order of magnitude below that of uncooled devices. In a second part, we describe tests of possible variations of fundamental constants using 87Rb and (CS)-C-133 fountains. Finally we give an update on the cold atom space clock PHARAO developed in collaboration with CNES. This clock is one of the main instruments of the ACES/ESA mission which is scheduled to fly on board the International Space Station in 2008, enabling a new generation of relativity tests.
U2 - 10.1088/0953-4075/38/9/002
DO - 10.1088/0953-4075/38/9/002
M3 - Article
SN - 0953-4075
VL - 38
SP - S449-S468
JO - Journal of Physics B: Atomic, Molecular and Optical Physics
JF - Journal of Physics B: Atomic, Molecular and Optical Physics
IS - 9
ER -