NOISE STATISTICS & PERCEIVED LOUDNESS .............................................................................. 4 NOISE SPECTRUMS ..................................................................................................................... 5 No noise shaping (TPDF dithering)..................................................................................... 5 Cool Edit (C1 curve) ...

We establish that in Quantum Chromodynamics (QCD) at zero temperature, SUL+R(NF ) exhibits the vector mode conjectured by Georgi and SUL−R(NF ) is realized in either the Nambu-Goldstone mode or else Q5 is also screened from view at infinity. The Wigner-Weyl mode is ruled out unless the beta function in QCD develops an infrared stable zero. PACS numbers: 11.3 Qc., 11.30.Rd., 12.38.Aw Typeset usi...

In a coalescing neutron star-neutron star or neutron star-black hole binary, oscillation modes of the neutron star can be resonantly excited by the companion during the final minutes of the binary inspiral, when the orbital frequency sweeps up from a few Hertz to a few thousand Hertz. The resulting resonant energy transfer between the orbit and the neutron star speeds up or slows down the inspi...

R-mode oscillations of rotating neutron stars are promising candidates for continuous gravitational wave (GW) observations. The r-mode frequencies slowly Newtonian well-known and independent the equation state (EOS) but stars, several mechanisms can alter frequency which relativistic correction is dominant relevant most stars. sensitive searches GWs those known pulsars GW in targeted narrow ban...