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investigation. THE PHENOMENA OF THE TIME-VIOLATING PHOTON POLARIZATION PLANE AND NEUTRON SPIN ROTATION BY A DIFFRACTION GRATING. NEW METHODS OF MEASURING OF THE TIME-VIOLATING INTERACTIONS.
, 1997
"... It is shown, that the new phenomena of the T-violating photon polarization plane and neutron spin rotation appear under diffraction in a noncentrosymmetrical diffraction grating. The equations describing the T-violating photon scattering by a diffraction grating and neutron interaction with noncentr ..."
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It is shown, that the new phenomena of the T-violating photon polarization plane and neutron spin rotation appear under diffraction in a noncentrosymmetrical diffraction grating. The equations describing the T-violating photon scattering by a diffraction grating and neutron interaction
A First Experimental Limit on In-matter Torsion from Neutron Spin Rotation in Liquid 4He
"... ar ..."
Neutron experiments to search for new spin-dependent interactions
"... The consideration is presented of possible neutron experiments to search for new short-range spin-dependent forces. The spin-dependent nucleon-nucleon interaction between neutron and nuclei may cause different effects: phase shift of a neutron wave in neutron interferometers of different kind, in pa ..."
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, in partic-ular of the Lloyd mirror configuration, neutron spin rotation in the pseudo-magnetic field, and transverse deflection of polarized neutron beam by a slab of substance. Estimates of sensitivity of these experiments are performed.
T-odd particle spin rotation in nuclear target
, 1999
"... It is shown that particle spin rotation in nuclear target, caused by the imaginary part of the spin-dependent forward scattering amplitude, is T-odd rotation. Prediction of the effect of neutron spin rotation [1] in matter with polarized nuclei target has initiated a research into polarization effec ..."
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It is shown that particle spin rotation in nuclear target, caused by the imaginary part of the spin-dependent forward scattering amplitude, is T-odd rotation. Prediction of the effect of neutron spin rotation [1] in matter with polarized nuclei target has initiated a research into polarization
The spin evolution of nascent neutron stars
, 2001
"... Neutron stars may, by virtue of their oscillations, act as sources of detectable gravitational radiation. Of particular interest are the r-mode oscillations, quasi-toroidal currents that arise in rotating stars due to the action of the Coriolis force. Andersson (1998) and Friedman & Morsink (199 ..."
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the gravitational wave signal to potentially detectable levels (Owen et al 1998). The r-mode instability is likely to be most important in hot young rapidly rotating neutron stars. For such stars there appears to be a window of temperatures and spin rates in which the r-modes can grow faster
SPIN AND MAGNETISM IN OLD NEUTRON STARS
, 2000
"... Abstract. The thermal, spin and magnetic evolution of neutron stars in the old low mass binaries is first explored. Recycled to very short periods via accretion torques, the neutron stars lose their magnetism progressively. If accretion proceeds undisturbed for 100 Myrs these stars can rotate close ..."
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Abstract. The thermal, spin and magnetic evolution of neutron stars in the old low mass binaries is first explored. Recycled to very short periods via accretion torques, the neutron stars lose their magnetism progressively. If accretion proceeds undisturbed for 100 Myrs these stars can rotate close
Neutron spin turners with a rotating magnetic field: first experiments
, 2008
"... Spin turners are the key elements of a neutron spin-echo spectrometer with rotating magnetic fields. Here we describe the results of experiments with thin-film spin turners made of 25 µm amorphous ferromagnetic foils, whose in-plane magnetization is rotated by a weak external rotating field. The beh ..."
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Spin turners are the key elements of a neutron spin-echo spectrometer with rotating magnetic fields. Here we describe the results of experiments with thin-film spin turners made of 25 µm amorphous ferromagnetic foils, whose in-plane magnetization is rotated by a weak external rotating field
Gravitational radiation and rotation of accreting neutron stars”, Astrophys
- J. Lett
, 1998
"... Recent discoveries by the Rossi X-Ray Timing Explorer indicate that most of the rapidly accreting ( ˙ M ∼> 10−11M ⊙ yr−1) weakly magnetic (B ≪ 1011 G) neutron stars in the Galaxy are rotating at spin frequencies νs ∼> 250 Hz. Remarkably, they all rotate in a narrow range of frequencies (no mo ..."
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Cited by 30 (0 self)
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Recent discoveries by the Rossi X-Ray Timing Explorer indicate that most of the rapidly accreting ( ˙ M ∼> 10−11M ⊙ yr−1) weakly magnetic (B ≪ 1011 G) neutron stars in the Galaxy are rotating at spin frequencies νs ∼> 250 Hz. Remarkably, they all rotate in a narrow range of frequencies (no
High-spin structures as the probes of proton-neutron pairing
, 2006
"... Rotating N = Z nuclei in the mass A = 58 − 80 region have been studied within the framework of isovector mean field theory. Available data is well and systematically described in the calculations. The present study supports the presence of strong isovector np pair field at low spin, which is, howeve ..."
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Rotating N = Z nuclei in the mass A = 58 − 80 region have been studied within the framework of isovector mean field theory. Available data is well and systematically described in the calculations. The present study supports the presence of strong isovector np pair field at low spin, which is
Results 1 - 10
of
5,996
