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Physics News Update
Number 855, February 5, 2008 www.aip.org/pnu by Phil Schewe and Jason S. Bardi

The Darkest Material Ever Made

Consists of a carpet of vertically oriented carbon nanotubes. The darkness or lightness of any object depends on the fraction of light falling on the object that gets reflected back. The reflectivity of the nanotube array developed by physicists at the Rensselaer Polytechnic Institute (RPI) is only 0.045%, three times smaller than the best previous dark object (see figure at <http://www.aip.org/png/2008/296.htm>). Shawn Lin and his colleagues grow the nanotubes on iron nanodots atop a silicon wafer. The resulting mat is thin (10-800 microns) and lightweight (.01-.02 g/cm^3).

Possible applications include the revision of darkness standards, such as are used by photographers. The lowest dark scale defined by NIST right now is for reflectances of about 1.5%. The material might also be useful in astronomical detectors (where you want to soak up stray radiation) or in photovoltaic cells which turn sunlight into electricity. Lin (sylin@rpi.edu) says that an additional feature of this new material is that it represents a controllably porous substance with an index of refraction (1.02) not very different from that of air. (Yang et al., NanoLetters, 9 January 2008).

Anti-Neutrinos and Nonproliferation

A new compact detector may help international inspectors peer inside a working nuclear reactor in a non-intrusive way by directly measuring the flux of anti-neutrinos coming out. Since their first use, nuclear reactors have, at least in principle, been closely related with nuclear weapons. For example, reactors produce plutonium which can later be fashioned into bomb material. The question of how to monitor the actual operation of a particular reactor and compare the changing plutonium inventory to what is expected from normal operations (producing electric power, say) is a large component of nuclear non-proliferation efforts.

The cubic-meter-scale detector, proposed by Adam Bernstein, leader of the Advanced Detectors Group at Lawrence Livermore National Laboratory (925-422-5918, bernstein3@llnl.gov) and built by a team from Livermore and Sandia National Laboratories California branch, would not attempt to monitor the reactor’s performance on a moment by moment basis. Instead its sensitivity is more attuned to the number of antineutrinos produced over hourly, daily and weeklong intervals. These time scales, Bernstein says, are well suited to the kind of monitoring performed by the International Atomic Energy Agency (IAEA).

The detector built by the LLNL/SNL collaboration operates unattended for long periods without significant maintenance, is self-calibrating, and does not affect plant operations in any way (see illustration of a detector at work, http://www.aip.org/png/2008/295.htm). Data from the detector is acquired remotely in real time. The detector module can be made tamper-proof using standard techniques, and the anti-neutrino signature seen by the detector (the arrival of a positron followed 30 microseconds later by a neutron) is hard to mimic with surrogate neutron or gamma sources. In conjunction with knowledge of the input fuel load and core design, the observed anti-neutrino flux provides a direct measure of the reactor’s power and isotopic content. (Bernstein et al.,upcoming article in the Journal of Applied Physics.)

Physical Review Letters

Celebrates its fiftieth anniversary this year. Several special events are planned, such as sessions at the upcoming March and April APS meetings. Also, a number of famous PRL papers from the past half century are being made available on the following website: http://prl.aps.org/50years/milestones> along with a brief summary of the papers’ importance.

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