نتایج جستجو برای: 3he

تعداد نتایج: 1796  

Journal: :Physical review letters 2004
A Casey J Parpia R Schanen B Cowan J Saunders

A high precision torsional oscillator has been used to study 3He films of thickness from 100 to 350 nm, in the temperature range 5<T<200 mK. This thickness is much smaller than the viscous penetration depth, and also much smaller than the low temperature inelastic mean-free path of 3He quasiparticles. Such films are observed to decouple from the motion of the oscillator below 60 mK. We interpre...

Journal: :Physical review letters 2013
Lev V Levitin Robert G Bennett Evgeny V Surovtsev Jeevak M Parpia Brian Cowan Andrew J Casey John Saunders

The B phase of superfluid 3He is a three-dimensional time-reversal invariant topological superfluid, predicted to support gapless Majorana surface states. We confine superfluid 3He into a thin nanofluidic slab geometry. In the presence of a weak symmetry-breaking magnetic field, we have observed two possible states of the confined 3He-B phase manifold, through the small tipping angle NMR respon...

2000
G. E. Volovik

Linear defects are generic in continuous media. In quantum systems they appear as topological line defects which are associated with a circulating persistent current. In relativistic quantum vacuum they are known as cosmic strings, in superconductors as quantized flux lines, and in superfluids and low-density atomic Bose-Einstein condensates as quantized vortex lines. We discuss unconventional ...

2008
Neelima G. Kelkar

The triton energy spectra of the charge-exchange 12C(3He,t) reaction at 2 GeV beam energy are analyzed in the quasi-elastic nucleon knock-out region. Considering that this region is mainly populated by the charge-exchange of a proton in 3He with a neutron in the target nucleus and the final proton going in the continuum, the cross-sections are written in the distorted-wave impulse approximation...

1999
L. E. Marcucci

The electromagnetic form factors of the trinucleons 3H and 3He are calculated with wave functions obtained with the Argonne v18 two-nucleon and Urbana IX three-nucleon interactions. Full account is taken of the two-body currents required by current conservation with the v18 interaction as well as those associated with N∆ transition currents and the currents of ∆ resonance components in the wave...

2001
Joseph M. Licciardi Peter U. Clark Edward J. Brook Kenneth L. Pierce Mark D. Kurz David Elmore Pankaj Sharma

Cosmogenic 3He and 10Be ages measured on surface boulders from the moraine sequence deposited by the northern outlet glacier of the Yellowstone ice cap indicate that the outlet glacier reached its terminal position at 16.5 6 0.4 3He ka and 16.2 6 0.3 10Be ka, respectively. Concordance of these ages supports the scaled production rates used for 3He (118.6 6 6.6 atoms · g21 · yr21) and 10Be (5.1 ...

2000
Monica Tosi

The predictions of Galactic chemical evolution models for D and 3He are described in connection with those on the other Galactic quantities for which observational constraints are available. Models in agreement with the largest set of data predict deuterium depletions from the Big Bang to the present epoch smaller than a factor of 3 and do not allow for D/H primordial abundances larger than ∼ 4...

2005
E. Fourre P. Jean-Baptiste J. I. Ishibashi

We present isotopic analysis of helium in hydrothermal fluids from the Manus back-arc basin, collected during the French-Japanese Manusflux and Manaute cruises in 1995 and 2000, respectively. The helium isotope composition of the fluids is comparable to that measured elsewhere in similar subduction environments, with 3He/4He values (7.4 to 7.9 Ra) slightly lower than typical MORB values, except...

2008
L. E. Marcucci

The astrophysical S-factor for the proton weak capture on 3He is calculated with correlated-hyperspherical-harmonics bound and continuum wave functions corresponding to realistic Hamiltonians consisting of the Argonne v14 or Argonne v18 two-nucleon and Urbana-VIII or Urbana-IX three-nucleon interactions. The nuclear weak charge and current operators have vector and axial-vector components, that...

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