These phenomena are believed to be responsible for the predicted polarization anisotropy of the cosmic microwave background. One possible path to detection of these phenomena is the observation of growing perturbations of spinning neutron stars, an effect known as the Chandrasekhar-Friedman-Schutz instability. The amplitude of these tensor phenomena is given by the second time derivative of the quadrupole source term in the post-Newtonian method of analyzing them. Evidence for these phenomena includes the orbital shrinking of binary systems such as the Hulse-Taylor pulsar, and these objects are being sought by both th
These phenomena are believed to be responsible for the predicted polarization anisotropy of the cosmic microwave background. One possible path to detection of these phenomena is the observation of growing perturbations of spinning neutron stars, an effect known as the Chandrasekhar-Friedman-Schutz instability. The amplitude of these tensor phenomena is given by the second time derivative of the quadrupole source term in the post-Newtonian method of analyzing them. Evidence for these phenomena includes the orbital shrinking of binary systems such as the Hulse-Taylor pulsar, and these objects are being sought by both the Large Interferometric Space Antenna and the LIGO project. For 10 points, identify these tensor perturbations predicted by general relativity which represent emissions of energy from massive systems.
These phenomena are believed to be responsible for the predicted polarization anisotropy of the cosmic microwave background.
gravity waves [accept word forms as well as gravitational radiation]