Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1994-02-28
Phys.Rev.D53:5723-5726,1996
Physics
High Energy Physics
High Energy Physics - Phenomenology
REVTEX, 13 pages, IP/BBSR/93-79
Scientific paper
10.1103/PhysRevD.53.5723
The orbital period of the binary pulsar PSR 1913+16 has been observed to decrease at the rate of $2.40\times 10^{-12}$ s/s which agrees with the prediction of the quadropole formula for gravitational radiation to within one percent. The decrease in orbital period may also occur by radiation of other massless particles like scalars and pseudoscalar Nambu-Goldstone bosons. Assuming that this energy loss is less than one percent of the gravitational radiation, we can establish bounds on couplings of these particles to nucleons. For a scalar nucleon coupling of the form $g_s~\phi~\bar\psi~\psi$ we find that $g_s< 3\times 10^{-19}$. From the radiation loss of massless Goldstone bosons we establish the upper bound $\theta /f< 7.5\times 10^{-16}$ GeV$^{-1}$ on the QCD vacuum angle $\theta$ and the scale $f$ at which the baryon number symmetry can be broken spontaneously.
Mohanty Subhendra
Panda Prafulla Kumar
No associations
LandOfFree
Particle Physics Bounds from the Hulse-Taylor Binary does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Particle Physics Bounds from the Hulse-Taylor Binary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Particle Physics Bounds from the Hulse-Taylor Binary will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-637114