Time Asymmetries in Pulsar Signals

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Supernova Asymmetries and Pulsar Kicks — Views on Controversial Issues

Two-and three-dimensional simulations demonstrate that hydro-dynamic instabilities can lead to low-mode (l = 1, 2) asymmetries of the fluid flow in the neutrino-heated layer behind the supernova shock. This provides a natural explanation for aspherical mass ejection and for pulsar recoil velocities even in excess of 1000 km/s. We propose that the bimodality of the pulsar velocity distribution m...

متن کامل

Hue shifts produced by temporal asymmetries in chromatic signals.

Observers viewed M- or L-cone-isolating stimuli and compared slowly-on and slowly-off sawtooth waveforms of the same mean chromaticity and luminance. Between 6 and 13 Hz, the mean hue of slowly-on L-cone and slowly-off M-cone sawtooth flicker appeared redder, and the mean hue of slowly-off L-cone and slowly-on M-cone sawtooth stimuli appeared greener-despite all the waveforms' having the same m...

متن کامل

Determination of pseudo-Goldstone-boson-photon coupling by the differential time delay of pulsar signals.

Pseudo-Goldstone bosons couple with photons through a P and T violating interaction of the form L I = g aγγ aF˜F. Strong magnetic fields in rotating compact stars induce a non-zero E · B outside the stellar surface which acts as a source for the pseudo-scalar field. Pulsar signals propagating through this pseudo-scalar 'hair' suffer a differential time lag between the left and the right circula...

متن کامل

Algorithm of ensemble pulsar time

An algorithm of the ensemble pulsar time based on the Wiener filtration method has been constructed. This algorithm has allowed the separation of the contributions of an atomic clock and a pulsar itself to the post-fit pulsar timing residuals. The method has been applied to the timing data of the millisecond pulsars PSR B1855+09 and PSR B1937+21 and allowed to filter out the atomic scale compon...

متن کامل

Time - Dependent CP Asymmetries in B 0 →

Y. Ushiroda, K. Sumisawa, K. Abe, K. Abe, I. Adachi, H. Aihara, D. Anipko, K. Arinstein, A. M. Bakich, E. Barberio, M. Barbero, A. Bay, I. Bedny, K. Belous, U. Bitenc, I. Bizjak, S. Blyth, A. Bondar, A. Bozek, M. Bračko, 13 J. Brodzicka, T. E. Browder, P. Chang, Y. Chao, A. Chen, K.-F. Chen, W. T. Chen, B. G. Cheon, R. Chistov, Y. Choi, Y. K. Choi, S. Cole, J. Dalseno, M. Dash, S. Eidelman, N. ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Symposium - International Astronomical Union

سال: 1981

ISSN: 0074-1809

DOI: 10.1017/s0074180900092871