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Issues

Letters

Physics Today 63 (1), 7 (2010); https://doi.org/10.1063/1.3293422
Physics Today 63 (1), 7–8 (2010); https://doi.org/10.1063/1.4797236
Physics Today 63 (1), 8 (2010); https://doi.org/10.1063/1.3293424
Physics Today 63 (1), 8 (2010); https://doi.org/10.1063/1.4797238

Search and Discovery

Physics Today 63 (1), 9–10 (2010); https://doi.org/10.1063/1.3293425

Molecules have more degrees of freedom than atoms do, so guiding them into the same few quantum states is a challenge.

Physics Today 63 (1), 11–13 (2010); https://doi.org/10.1063/1.3293401

The eagerly anticipated observation of the fractional quantum Hall effect raises hopes of seeing even more exotic behavior.

Physics Today 63 (1), 13–17 (2010); https://doi.org/10.1063/1.3293402

The long-held presumption that most cosmic rays are accelerated in supernova remnants has, until now, lacked convincing evidence.

Physics Today 63 (1), 16 (2010); https://doi.org/10.1063/1.3293403
Physics Today 63 (1), 16 (2010); https://doi.org/10.1063/1.4797226
Physics Today 63 (1), 16–17 (2010); https://doi.org/10.1063/1.4797228
Physics Today 63 (1), 17 (2010); https://doi.org/10.1063/1.4797229
Physics Today 63 (1), 17 (2010); https://doi.org/10.1063/1.4797231

Issues and Events

Physics Today 63 (1), 18–20 (2010); https://doi.org/10.1063/1.3293404

Nearly a year after passage of the stimulus package, federal agencies are close to committing the entire $18.4 billion provided for basic research. But what happens when funding runs out?

Physics Today 63 (1), 20–23 (2010); https://doi.org/10.1063/1.3293405

By ratcheting up the sensitivity about an order of magnitude, a handful of experiments aim to see neutrinoless double beta decay and measure the neutrino mass; if unsuccessful, larger experiments would be the next step.

Physics Today 63 (1), 23–25 (2010); https://doi.org/10.1063/1.3293406

Agencies move tentatively to implement Obama’s plan, but Iran isn’t invited to the table, and funding is scarce.

Physics Today 63 (1), 24 (2010); https://doi.org/10.1063/1.3293407
Physics Today 63 (1), 25–26 (2010); https://doi.org/10.1063/1.3293408
Physics Today 63 (1), 26 (2010); https://doi.org/10.1063/1.3293409
Physics Today 63 (1), 26 (2010); https://doi.org/10.1063/1.4797233
Physics Today 63 (1), 26 (2010); https://doi.org/10.1063/1.4797234

Articles

Physics Today 63 (1), 27–32 (2010); https://doi.org/10.1063/1.3293410

In a dispute with more than just scientific import, Alexis Clairaut, Leonhard Euler, and Jean le Rond d’Alembert each employed their own strategies to establish that they were the first to understand a puzzling feature of the Moon’s orbit.

Physics Today 63 (1), 33–38 (2010); https://doi.org/10.1063/1.3293411

In topological insulators, spin–orbit coupling and time-reversal symmetry combine to form a novel state of matter predicted to have exotic physical properties.

Physics Today 63 (1), 40–45 (2010); https://doi.org/10.1063/1.3293412

In 1960 two rival laboratories reported the creation of lasers. Controversy over priority and proper behavior has persisted for half a century. Now three Bell Labs veterans of that confused but exciting summer tell the story as they remember it.

Books

Physics Today 63 (1), 47–48 (2010); https://doi.org/10.1063/1.3293413
Physics Today 63 (1), 48 (2010); https://doi.org/10.1063/1.3293414
Physics Today 63 (1), 48–49 (2010); https://doi.org/10.1063/1.3293415
Physics Today 63 (1), 49–50 (2010); https://doi.org/10.1063/1.3293416
Physics Today 63 (1), 50–54 (2010); https://doi.org/10.1063/1.3293417

New Products

Physics Today 63 (1), 56–58 (2010); https://doi.org/10.1063/1.3293418

Obituaries

In Special Collection: Print Obituaries
Physics Today 63 (1), 60–61 (2010); https://doi.org/10.1063/1.3293419
In Special Collection: Print Obituaries
Physics Today 63 (1), 61 (2010); https://doi.org/10.1063/1.3293420

Quick Study

Physics Today 63 (1), 62–63 (2010); https://doi.org/10.1063/1.3293421

The observation of gravitational waves will offer astronomers a new view of the cosmos. One promising approach for detecting those spacetime perturbations relies on the precise timing of signals from radio pulsars.

Back Scatter

Physics Today 63 (1), 80 (2010); https://doi.org/10.1063/1.3293423
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