The current experiments use such
a small number of photons that it would take a standard laptop a fraction of a second to make the same calculation.
Because one of the leading techniques is the manipulation of
small numbers of photons, one critical need has been for a highly efficient photon counter that can measure the number of photons in a pulse of light.
Not exact matches
In the quantum world, physicists study the tiny particles that make up our classical world — neutrons, electrons,
photons — either one at a time or in
small numbers because the behaviour
of the particles is completely different on such a
small scale.
The authors found that their heat engine model only yields high efficiency and output power when the
number of photons involved is
small; accordingly, its efficiency and power output rapidly decrease as the
number of photons increases.
Stephen Hawking theorized in 1974 that black holes radiate
small numbers of particles (mainly
photons), a process known as «Hawking Radiation».
A very
small number of microwave
photons are sent into the box where their quantum fields interact with the superconducting circuit.
A
number of infinitesimally
small, dust devil — like energy vortices called quarks and
photons collectively make up the structure
of the atom.
To select a
small number of parameters conveying the maximal information about the [
photon] shower shape, we uncorrelated the above parameters through a principal component analysis in which these seven parameters are transformed into new seven uncorrelated parameters given by the eigenvectors
of the covariance matrix.
i.e. if c is higher, then also dQ must be higher in order to get the same dT with the same m. Thus the same
number of the longwave
photons will give a
smaller rise
of temperature
of water as compared to the material in the pavement.
So to argue for the insignificance
of the thermosphere to radiative balance it is not sufficient to point to its
small mass and
number of molecules — one must accompany this with physics showing for instance the mean free path
of photons between interactions with air molecules to be sufficiently long that the thermosphere will not significantly affect outgoing flux.