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PERSPECTIVES<br />
770<br />
a means for further optimizing the editing<br />
performance of Cas9.<br />
Effi cient strategies for directed editing<br />
of mamm<strong>al</strong>ian genomes will enable sophisticated<br />
gen<strong>et</strong>ic engineering for both fundament<strong>al</strong><br />
and applied purposes. Especi<strong>al</strong>ly in<br />
medic<strong>al</strong> applications, high-fi delity targ<strong>et</strong> recognition<br />
is critic<strong>al</strong>, as off-site nuclease activity<br />
will jeopardize the saf<strong>et</strong>y of the engineering<br />
operation; thus, long str<strong>et</strong>ches of nucleotides<br />
should be specifi c<strong>al</strong>ly recognized. In<br />
addition, adjusting the system’s specifi city<br />
toward new targ<strong>et</strong> sequences should be easy<br />
and affordable; this is a major advantage of<br />
the Cas9 system, as it merely requires changing<br />
the sequence of the guide RNA. Further-<br />
PHYSICS<br />
Demonstrating Uncertainty<br />
Gerard J. Milburn<br />
Anyone using a modern camera is<br />
implementing an optic<strong>al</strong> position<br />
measurement. In an active autofocus<br />
camera, a pulse of infrared light is emitted<br />
from the camera, and the time taken for<br />
it to be refl ected back to the camera is used<br />
to compute the distance b<strong>et</strong>ween the object<br />
and the image plane. Imagine how diffi cult<br />
it would be to operate such a system if the<br />
object recoiled every time the<br />
infrared pulse was refl ected from<br />
it. Heisenberg suggested that this<br />
is precisely what would happen if<br />
light were used to d<strong>et</strong>ermine the<br />
position of a quantum object as<br />
accurately as his famous uncertainty<br />
principle would <strong>al</strong>low. On<br />
page 801 of this issue, Purdy <strong>et</strong><br />
<strong>al</strong>. ( 1) demonstrate this quantum<br />
back-action effect in an optic<strong>al</strong><br />
measurement of the position of a<br />
macroscopic mirror.<br />
The mechanic<strong>al</strong> action of<br />
light has long been known ( 2).<br />
Kepler suggested that the reason<br />
com<strong>et</strong> tails point away from<br />
the Sun is due to the mechanic<strong>al</strong><br />
action of light. In the early<br />
1970s, Arthur Ashkin of Bell Sign<strong>al</strong><br />
Laboratories showed that optic<strong>al</strong><br />
intensity gradients could exert a Probe<br />
force on microm<strong>et</strong>er-size parti-<br />
Centre for Engineered Quantum Systems, The<br />
University of Queensland, St Lucia, Brisbane,<br />
QLD 4072, Austr<strong>al</strong>ia. E-mail: milburn@<br />
physics.uq.edu.au<br />
more, the recombination should be fast, effi -<br />
cient, and sc<strong>al</strong>able. Compared to the most<br />
promising currently available genome editing<br />
systems (zinc fi nger domains and TAL-<br />
ENs), the RNA-guided Cas9 nuclease probably<br />
is closest to me<strong>et</strong>ing these requirements.<br />
However, effi ciency and specifi city still can<br />
be improved—for instance, by laboratory<br />
evolution. Applying these genome surgery<br />
techniques to correct human disease-associated<br />
gen<strong>et</strong>ic mutations, resulting in function<strong>al</strong><br />
gene therapy and in curing gen<strong>et</strong>ic disorders,<br />
will therefore take time. The spectacular<br />
recent development of dedicated nucleases<br />
suggests, however, that we are entering<br />
the fi n<strong>al</strong> stage of this quest.<br />
cles. This observation eventu<strong>al</strong>ly led to laser<br />
cooling and the fi eld of atom optics.<br />
The history of using optic<strong>al</strong> transducers<br />
to monitor the quantized position of an<br />
object at the Heisenberg limit goes back to<br />
the early propos<strong>al</strong>s for the optic<strong>al</strong> d<strong>et</strong>ection<br />
of gravitation<strong>al</strong> radiation ( 3). The relative<br />
length of the two orthogon<strong>al</strong> arms<br />
in a Michelson-Morley interferom<strong>et</strong>er is<br />
Incident<br />
Reflected<br />
15 FEBRUARY 2013 VOL 339 SCIENCE www.sciencemag.org<br />
Published by AAAS<br />
Transmitted<br />
Sign<strong>al</strong><br />
Probe<br />
References<br />
1. L. Cong <strong>et</strong> <strong>al</strong>., Science 339, 819 (2013);<br />
10.1126/science.1231143.<br />
2. P. M<strong>al</strong>i <strong>et</strong> <strong>al</strong>., Science 339, 823 (2013);<br />
10.1126/science.1232033.<br />
3. B. L. Stoddard, Structure 19, 7 (2011).<br />
4. F. D. Urnov, E. J. Rebar, M. C. Holmes, H. S. Zhang,<br />
P. D. Gregory, Nat. Rev. Gen<strong>et</strong>. 11, 636 (2010).<br />
5. A. J. Bogdanove, D. F. Voytas, Science 333, 1843 (2011).<br />
6. K. Eisenschmidt <strong>et</strong> <strong>al</strong>., Nucleic Acids Res. 33, 7039<br />
(2005).<br />
7. B. Wiedenheft, S. H. Sternberg, J. A. Doudna, Nature<br />
482, 331 (2012).<br />
8. E. R. Westra <strong>et</strong> <strong>al</strong>., Annu. Rev. Gen<strong>et</strong>. 46, 311 (2012).<br />
9. E. Deltcheva <strong>et</strong> <strong>al</strong>., Nature 471, 602 (2011).<br />
10. M. Jinek <strong>et</strong> <strong>al</strong>., Science 337, 816 (2012).<br />
11. G. Gasiunas, R. Barrangou, P. Horvath, V. Siksnys, Proc.<br />
Natl. Acad. Sci. U.S.A. 109, E2579 (2012).<br />
12. M. Jinek <strong>et</strong> <strong>al</strong>., elife 2013; 2:300471 (2013).<br />
10.1126/science.1234726<br />
Heisenberg’s uncertainty principle is<br />
demonstrated with a vibrating macroscopic<br />
mirror.<br />
changed by the tid<strong>al</strong> forces exerted by gravitation<strong>al</strong><br />
waves. This length difference leads<br />
to changes in the interference of light at the<br />
output mirror. Monitoring the output intensity<br />
can thus be used to measure the relative<br />
position of the end mirrors.<br />
The effect is sm<strong>al</strong>l, however, and very<br />
sm<strong>al</strong>l changes in the intensity need to be<br />
d<strong>et</strong>ected. This eventu<strong>al</strong>ly runs into a problem<br />
caused by the essenti<strong>al</strong> granular<br />
nature of light (light pulses are<br />
made up of individu<strong>al</strong> photons).<br />
Even the most carefully stabilized<br />
laser produces light with<br />
intensity fl uctuations due to the<br />
random arriv<strong>al</strong> of individu<strong>al</strong> photons,<br />
c<strong>al</strong>led shot noise. We rarely<br />
need to account for this as the relative<br />
size of the intensity fl uctuation<br />
f<strong>al</strong>ls off as the inverse square<br />
root of the intensity, so we can<br />
<strong>al</strong>ways increase the intensity to<br />
improve the sign<strong>al</strong>-to-noise ratio.<br />
But there is another problem.<br />
If we take into account the<br />
mechanic<strong>al</strong> action of light, we<br />
see that a price must be paid for<br />
An optic<strong>al</strong> cavity with a vibrating<br />
mirror. As this mirror moves, the<br />
intensity of the transmitted light can<br />
be used to monitor its position. (Ins<strong>et</strong>)<br />
When the quantum nature of light is<br />
included, the random reflection of<br />
individu<strong>al</strong> photons shakes the mirror,<br />
adding radiation pressure noise to the<br />
position measurement.<br />
on February 14, 2013<br />
www.sciencemag.org<br />
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