1969
DOI: 10.1109/tmag.1969.1066547
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Noise of ferromagnetic materials

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1972
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Cited by 92 publications
(63 citation statements)
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“…Observations (Chakrabarty et al, 2003) of a ''speed limit'' for pulsars seem to support the theory (Bildsten, 1998) that gravitational radiation works to brake the spin of the fastest pulsars before they are ripped apart by their relativistic spins. Expectations from neutron star models indicate that the ellipticity may range from 10 À9 to 10 À6 (Ushomirsky, Cutler, and Bildsten, 2000;Owen, 2006) for conventional neutron stars and somewhat larger for more exotic stars (Owen, 2005).…”
Section: Pulsarsmentioning
confidence: 81%
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“…Observations (Chakrabarty et al, 2003) of a ''speed limit'' for pulsars seem to support the theory (Bildsten, 1998) that gravitational radiation works to brake the spin of the fastest pulsars before they are ripped apart by their relativistic spins. Expectations from neutron star models indicate that the ellipticity may range from 10 À9 to 10 À6 (Ushomirsky, Cutler, and Bildsten, 2000;Owen, 2006) for conventional neutron stars and somewhat larger for more exotic stars (Owen, 2005).…”
Section: Pulsarsmentioning
confidence: 81%
“…3). The GEO600 detector has achieved a power gain of 1000 using power recycling (Blair et al, 2012).…”
Section: B Power Recyclingmentioning
confidence: 99%
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“…can vary discontinuously when driven by external forces such as temperature [1][2][3], magnetic field [4][5][6][7][8][9], stress [10], and chemical potential [11]. The size of these changes can range over many orders of magnitude.…”
mentioning
confidence: 99%
“…Originally detected through a pair of loud speakers by Barkhausen in 1919, hence the term "Barkhausen Noise", it is the resulting voltage spikes that are usually recorded and analysed. Sources of noise in ferromagnetic materials have been reviewed by Bittel (1969).…”
mentioning
confidence: 99%