CWRU PAT Coffee Agenda

Tuesdays 10:30 - 11:30 | Fridays 11:30 - 12:30

+2 On Rotation Curve Analysis.

kxp265 +1 jtd55 +1

+1 Chiral Gravitational Waves and Baryon Superfluid Dark Matter. - [UPDATED]

rxl527 +1

+1 Studies of Lepton Flavor Violation at the LHC.

pxf112 +1

+1 Localization of the Standard Model via Higgs mechanism and a finite electroweak monopole from non-compact five dimensions.

pxf112 +1

+1 Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice.

jtd55 +1

+1 Conformal Standard Model, Leptogenesis and Dark Matter. - [UPDATED]

pxf112 +1

Showing votes from 2018-02-16 12:30 to 2018-02-20 11:30 | Next meeting is Tuesday Aug 5th, 10:30 am.

users

  • No papers in this section today!

astro-ph.CO

  • Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice.- [PDF] - [Article]

    Daniel Cutting, Mark Hindmarsh, David J. Weir
     

    We conduct large scale numerical simulations of gravitational wave production at a first order vacuum phase transition. We find a power law for the gravitational wave power spectrum at high wavenumber which falls off as $k^{-1.5}$ rather than the $k^{-1}$ produced by the envelope approximation. The peak of the power spectrum is shifted to slightly lower wave numbers from that of the envelope approximation. The envelope approximation reproduces our results for the peak power less well, agreeing only to within an order of magnitude. After the bubbles finish colliding the scalar field oscillates around the true vacuum. An additional feature is produced in the UV of the gravitational wave power spectrum, and this continues to grow linearly until the end of our simulation. The additional feature peaks at a length scale close to the bubble wall thickness and is shown to have a negligible contribution to the energy in gravitational waves, providing the scalar field mass is much smaller than the Planck mass.

astro-ph.HE

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astro-ph.GA

  • No papers in this section today!

astro-ph.IM

  • On Rotation Curve Analysis.- [PDF] - [Article]

    Kevin Kadowaki
     

    An analysis of analytical methods used for computing galactic masses on the basis of rotation curves (Saari 2015) is shown to be flawed.

gr-qc

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hep-ph

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hep-th

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hep-ex

  • No papers in this section today!

quant-ph

  • No papers in this section today!

other

  • No papers in this section today!