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Physics Update

Physics Today 56 (4), 9 (2003); https://doi.org/10.1063/1.2409961
Physics Today 56 (4), 9 (2003); https://doi.org/10.1063/1.4797020
Physics Today 56 (4), 9 (2003); https://doi.org/10.1063/1.4797023
Physics Today 56 (4), 9 (2003); https://doi.org/10.1063/1.4797026

Reference Frame

Physics Today 56 (4), 10–11 (2003); https://doi.org/10.1063/1.1580026

Letters

Physics Today 56 (4), 13 (2003); https://doi.org/10.1063/1.1580027
Physics Today 56 (4), 13–14 (2003); https://doi.org/10.1063/1.4796999
Physics Today 56 (4), 14–15 (2003); https://doi.org/10.1063/1.4797002
Physics Today 56 (4), 15 (2003); https://doi.org/10.1063/1.4797005
Physics Today 56 (4), 15–16 (2003); https://doi.org/10.1063/1.4797007
Physics Today 56 (4), 16–17 (2003); https://doi.org/10.1063/1.4797010
Physics Today 56 (4), 17 (2003); https://doi.org/10.1063/1.4797013
Physics Today 56 (4), 17–18 (2003); https://doi.org/10.1063/1.4797015
Physics Today 56 (4), 18 (2003); https://doi.org/10.1063/1.1580035
Physics Today 56 (4), 18 (2003); https://doi.org/10.1063/1.1580036

Search and Discovery

Physics Today 56 (4), 21–24 (2003); https://doi.org/10.1063/1.1580037

A year of full-sky observation by the newly rechristened Wilkinson Microwave Anisotropy Probe greatly strengthens the case for inflationary Big Bang cosmology.

Physics Today 56 (4), 23 (2003); https://doi.org/10.1063/1.1580038
Physics Today 56 (4), 24–27 (2003); https://doi.org/10.1063/1.1580039

At modest magnetic fields and microwave excitations, the resistance of a 2D semiconductor can oscillate all the way to zero.

Physics Today 56 (4), 27–29 (2003); https://doi.org/10.1063/1.1580040

The attophysics frontier is about to expand, thanks to the newly won ability to control the phase of amplified laser pulses.

Issues and Events

Physics Today 56 (4), 31–32 (2003); https://doi.org/10.1063/1.1580041

Martin Fisher puts his mind to using technology to facilitate microentre-preneurs in East Africa.

Physics Today 56 (4), 32–34 (2003); https://doi.org/10.1063/1.1580042

Russia and other former Soviet republics inherited a massive nuclear weapons program they could no longer afford. Thousands of former weapons scientists have been subsidized by US grants, but finding them permanent, civilian jobs has proven to be extremely difficult.

Physics Today 56 (4), 33 (2003); https://doi.org/10.1063/1.2409962
Physics Today 56 (4), 34–35 (2003); https://doi.org/10.1063/1.1580043
Physics Today 56 (4), 35 (2003); https://doi.org/10.1063/1.1580044
Physics Today 56 (4), 35–36 (2003); https://doi.org/10.1063/1.1580045
Physics Today 56 (4), 36 (2003); https://doi.org/10.1063/1.1580046
Physics Today 56 (4), 36–37 (2003); https://doi.org/10.1063/1.1580047
Physics Today 56 (4), 37 (2003); https://doi.org/10.1063/1.2409963
Physics Today 56 (4), 37 (2003); https://doi.org/10.1063/1.2409964
Physics Today 56 (4), 37 (2003); https://doi.org/10.1063/1.4797018

Articles

Physics Today 56 (4), 39–44 (2003); https://doi.org/10.1063/1.1580048

No longer threatened by a rival superpower, the US now faces the growing danger of clandestine terrorist groups. Effectively countering terrorists requires that physicists actively contribute to the nation’s defense.

In Special Collection: Quantum archive
Physics Today 56 (4), 46–52 (2003); https://doi.org/10.1063/1.1580049

It’s not your grandfather’s quantum mechanics. Today, researchers treat entanglement as a physical resource: Quantum information can now be measured, mixed, distilled, concentrated, and diluted.

Physics Today 56 (4), 53–60 (2003); https://doi.org/10.1063/1.1580050

Using very distant supernovae as standard candles, one can trace the history of cosmic expansion and try to find out what’s currently speeding it up.

Books

Physics Today 56 (4), 63 (2003); https://doi.org/10.1063/1.1580051
Physics Today 56 (4), 63–64 (2003); https://doi.org/10.1063/1.1580052
Physics Today 56 (4), 64 (2003); https://doi.org/10.1063/1.1580053
Physics Today 56 (4), 64–67 (2003); https://doi.org/10.1063/1.1580054
Physics Today 56 (4), 67–68 (2003); https://doi.org/10.1063/1.1580055
Physics Today 56 (4), 68 (2003); https://doi.org/10.1063/1.1580056
Physics Today 56 (4), 69–70 (2003); https://doi.org/10.1063/1.1580057
Physics Today 56 (4), 70–73 (2003); https://doi.org/10.1063/1.2409965

New Products

Physics Today 56 (4), 74–76 (2003); https://doi.org/10.1063/1.2409966

We Hear That

Physics Today 56 (4), 77 (2003); https://doi.org/10.1063/1.1580058
Physics Today 56 (4), 77–78 (2003); https://doi.org/10.1063/1.1580059
Physics Today 56 (4), 78 (2003); https://doi.org/10.1063/1.1580060
Physics Today 56 (4), 78–79 (2003); https://doi.org/10.1063/1.1580061
Physics Today 56 (4), 79 (2003); https://doi.org/10.1063/1.1580062
Physics Today 56 (4), 79–80 (2003); https://doi.org/10.1063/1.1580063
Physics Today 56 (4), 80 (2003); https://doi.org/10.1063/1.1580064

Obituaries

In Special Collection: Print Obituaries
Physics Today 56 (4), 80–81 (2003); https://doi.org/10.1063/1.4729372
In Special Collection: Print Obituaries
Physics Today 56 (4), 81–82 (2003); https://doi.org/10.1063/1.1580065
In Special Collection: Print Obituaries
Physics Today 56 (4), 82–83 (2003); https://doi.org/10.1063/1.1580066
In Special Collection: Print Obituaries
Physics Today 56 (4), 83–84 (2003); https://doi.org/10.1063/1.1580067
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