Search Publications

Detection of B-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
DOI: 10.1103/PhysRevLett.111.141301 Bibcode: 2013PhRvL.111n1301H

Ade, P. A. R.; Bock, J. J.; Chiang, H. C. +65 more

Gravitational lensing of the cosmic microwave background generates a curl pattern in the observed polarization. This “B-mode” signal provides a measure of the projected mass distribution over the entire observable Universe and also acts as a contaminant for the measurement of primordial gravity-wave signals. In this Letter we present the first det…

2013 Physical Review Letters
Herschel 278
Regimes of the Electron Diffusion Region in Magnetic Reconnection
DOI: 10.1103/PhysRevLett.110.135004 Bibcode: 2013PhRvL.110m5004L

Egedal, J.; Daughton, W.; Karimabadi, H. +3 more

The electron diffusion region during magnetic reconnection lies in different regimes depending on the pressure anisotropy, which is regulated by the properties of thermal electron orbits. In kinetic simulations at the weakest guide fields, pitch angle mixing in velocity space causes the outflow electron pressure to become nearly isotropic. Above a…

2013 Physical Review Letters
Cluster 103
Bifurcated Structure of the Electron Diffusion Region in Three-Dimensional Magnetic Reconnection
DOI: 10.1103/PhysRevLett.110.265004 Bibcode: 2013PhRvL.110z5004L

Li, H.; Daughton, W.; Karimabadi, H. +2 more

Three-dimensional kinetic simulations of magnetic reconnection reveal that the electron diffusion region is composed of two or more current sheets in regimes with weak magnetic shear angles ϕ≲80°. This new morphology is explained by oblique tearing modes which produce flux ropes while simultaneously driving enhanced current at multiple resonance s…

2013 Physical Review Letters
Cluster 89
Energy Partition in Magnetic Reconnection in Earth's Magnetotail
DOI: 10.1103/PhysRevLett.110.225001 Bibcode: 2013PhRvL.110v5001E

Eastwood, J. P.; Lavraud, B.; Phan, T. D. +4 more

The partition of energy flux in magnetic reconnection is examined experimentally using Cluster satellite observations of collisionless reconnection in Earth’s magnetotail. In this plasma regime, the dominant component of the energy flux is ion enthalpy flux, with smaller contributions from the electron enthalpy and heat flux and the ion kinetic en…

2013 Physical Review Letters
Cluster 83
Limits on the Dependence of the Fine-Structure Constant on Gravitational Potential from White-Dwarf Spectra
DOI: 10.1103/PhysRevLett.111.010801 Bibcode: 2013PhRvL.111a0801B

Barstow, M. A.; Holberg, J. B.; Webb, J. K. +5 more

We propose a new probe of the dependence of the fine-structure constant α on a strong gravitational field using metal lines in the spectra of white-dwarf stars. Comparison of laboratory spectra with far-UV astronomical spectra from the white-dwarf star G191-B2B recorded by the Hubble Space Telescope Imaging Spectrograph gives limits of Δα/α=(4.2±1…

2013 Physical Review Letters
eHST 71
Stochastic Acceleration by Multi-Island Contraction during Turbulent Magnetic Reconnection
DOI: 10.1103/PhysRevLett.110.151101 Bibcode: 2013PhRvL.110o1101B

Kontar, Eduard P.; Bian, Nicolas H.

The acceleration of charged particles in magnetized plasmas is considered during turbulent multi-island magnetic reconnection. The particle acceleration model is constructed for an ensemble of islands which produce adiabatic compression of the particles. The model takes into account the statistical fluctuations in the compression rate experienced …

2013 Physical Review Letters
Cluster 33
New Constraints on the Early Expansion History of the Universe
DOI: 10.1103/PhysRevLett.111.041301 Bibcode: 2013PhRvL.111d1301H

Hojjati, Alireza; Samsing, Johan; Linder, Eric V.

Cosmic microwave background measurements have pushed to higher resolution, lower noise, and more sky coverage. These data enable a unique test of the early Universe’s expansion rate and constituents such as effective number of relativistic degrees of freedom and dark energy. Using the most recent data from Planck and WMAP9, we constrain the expans…

2013 Physical Review Letters
Planck 27