The
principle of operation of an atomic clock is based on atomic
physics; it measures the electromagnetic signal that electrons in
atoms emit when they change energy
levels. Early atomic clocks were based on masers at
room temperature. Since 2004, more accurate atomic clocks first cool the atoms
to near absolute
zero temperature by slowing them with lasers and probing them
in atomic
fountains in a microwave-filled
cavity. An example of this is the NIST-F1 atomic
clock, one of the national primary time and frequency standards of the United
States.
The
accuracy of an atomic clock depends on two factors: the first is temperature of
the sample atoms—colder atoms move much more slowly, allowing longer probe
times, the second is the frequency and intrinsic
linewidth of the electronic or hyperfine transition. Higher
frequencies and narrow lines increase the precision.
National
standards agencies in many countries maintain a network of atomic clocks which
are intercompared and kept synchronized to an accuracy of 10−9 seconds
per day (approximately 1 part in 1014). These clocks collectively
define a continuous and stable time scale, the International
Atomic Time (TAI). For civil time, another time scale is
disseminated, Coordinated Universal Time (UTC). UTC is derived from
TAI, but has added leap
seconds from UT1,
to account for variations in the rotation
of the Earth with respect to the solar time.
Mechanism
Since 1968,
the International System of Units (SI) has defined the second as
the duration of 9192631770 cycles of radiation corresponding to
the transition between two energy levels of the ground state of the caesium-133 atom.
In 1997, the International Committee for Weights
and Measures (CIPM) added that the preceding definition refers
to a caesium atom at rest at a temperature of absolute
zero.[15]
This
definition makes the caesium oscillator the primary standard for time and
frequency measurements, called the caesium
standard. The definitions of other physical units, e.g., the volt and
the metre,
rely on the definition of the second.[16]
In this
particular design, the time-reference of an atomic clock consists of an
electronic oscillator operating at microwave frequency. The oscillator is
arranged so that its frequency-determining components include an element that
can be controlled by a feedback signal. The feedback signal keeps the
oscillator tuned in resonance with
the frequency of the hyperfine transition of caesium or rubidium.
The core of
the radio
frequency atomic clock is a tunable microwave
cavity containing a gas. In a hydrogen
maser clock the gas emits microwaves (the
gas mases)
on a hyperfine transition, the field in the cavity oscillates, and the cavity
is tuned for maximum microwave amplitude. Alternatively, in a caesium or
rubidium clock, the beam or gas absorbs microwaves and the cavity contains an
electronic amplifier to make it oscillate. For both types the atoms in the gas
are prepared in one hyperfine state prior to filling them into the cavity. For
the second type the number of atoms which change hyperfine state is detected
and the cavity is tuned for a maximum of detected state changes.
Most of the
complexity of the clock lies in this adjustment process. The adjustment tries
to correct for unwanted side-effects, such as frequencies from other electron
transitions, temperature changes, and the spreading in frequencies caused
by ensemble effects.[clarification
needed] One way of doing this is to sweep the
microwave oscillator's frequency across a narrow range to generate a modulated
signal at the detector.
The
detector's signal can then be demodulated to
apply feedback to control long-term drift in the radio frequency. In this way,
the quantum-mechanical properties of the atomic transition frequency of the
caesium can be used to tune the microwave oscillator to the same frequency,
except for a small amount of experimental error. When a clock is first turned
on, it takes a while for the oscillator to stabilize. In practice, the feedback
and monitoring mechanism is much more complex.
A number of other atomic clock
schemes used for other purposes. Rubidium standard clocks are prized for their
low cost, small size (commercial standards are as small as 17 cm3)[13] and
short-term stability. They are used in many commercial, portable and aerospace
applications. Hydrogen masers (often manufactured in Russia) have superior
short-term stability compared to other standards, but lower long-term accuracy.
Often, one standard is used to
fix another. For example, some commercial applications use a rubidium standard
periodically corrected by a global
positioning system receiver (see GPS disciplined oscillator). This achieves excellent
short-term accuracy, with long-term accuracy equal to (and traceable to) the US
national time standards.
The lifetime of a standard is
an important practical issue. Modern rubidium standard tubes last more than ten
years, and can cost as little as US$50.[citation
needed] Caesium reference tubes suitable for national
standards currently last about seven years and cost about US$35,000. The
long-term stability of hydrogen maser standards decreases because of changes in
the cavity's properties over time.
Modern clocks use magneto-optical
traps to cool the atoms for improved precision.
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