The force of gravity looks like two copies of the strong subnuclear interactions working in unison.
Does this double gluon thingie give any kind of green light to exotic space flight propulsion concepts?
Hmm, well in that case, maybe some of these nucleonic isomers would also provide similarly useful possibilities for testing - or is that what you were referring to? I think I put up a post on Bismuth-212 some time back:http://forum.nasaspaceflight.com/index.php?topic=32318.0Since nucleonic isomers offer up altered states of the strong force, and this new theory connects the strong force to gravity, then maybe this would be a good place to start looking. I'm not sure what the electronic shell has to do with things, since that's not really strong force, right?I wonder if it might be possible to have nucleus which behaves anisotropically in a gravitational field - ie. the response of the nucleus to the gravitational field would depend on the orientation of the nucleus.
The Science Obejctives (SO) for LISA describe the science that LISA will enable. The subsequent Science Investigations (SI) highlight the ways of obtaining the science by evaluating the LISA data. More details of the science objectives can be found in the LISA Science Requirement Document (SciRD)SO 1 Study the formation and evolution of compact binary stars in the Milky Way Galaxy SI 1.1 Elucidate the formation and evolution of Galactic Binaries by measuring their period, spatial and mass distributions SI 1.2 Enable joint gravitational and electromagnetic observations of galactic binaries to study the interplay between gravitational radiation and tidal dissipation in interacting stellar systems SO 2 Trace the origin, growth and merger history of massive black holes across cosmic ages SI 2.1 Search for seed black holes at cosmic dawn SI 2.2 Study the growth mechanism of MBHs before the epoch of reionization SI 2.3 Observation of EM counterparts to unveil the astrophysical environment around merging binaries SI 2.4 Test the existence of intermediate-mass black holes (IMBHs) SO 3 Probe the dynamics of dense nuclear clusters using extreme mass-ratio inspirals (EMRIs) SI 3.1 Study the immediate environment of Milky Way like massive black holes (MBHs) at low redshift SO 4 Understand the astrophysics of stellar origin black holes SI 4.1 Study the close environment of Stellar Origin Black Holes (SOBHs) by enabling multi-band and multi-messenger observations at the time of coalescence SI 4.2 Disentangle SOBHs binary formation channels SO 5 Explore the fundamental nature of gravity and black holes SI 5.1 Use ring-down characteristics observed in massive black hole binary (MBHB) coalescences to test whether the post-merger objects are the black holes predicted by General Theory of Relativity SI 5.2 Use EMRIs to explore the multipolar structure of MBHs SI 5.3 Testing for the presence of beyond-GR emission channels SI 5.4 Test the propagation properties of gravitational waves 5.1. Test the presence of massive fields around massive black holes with masses larger than 103 M☉ SO 6 Probe the rate of expansion of the Universe SI 6.1 Measure the dimensionless Hubble parameter by means of gravitational wave observations only SI 6.2 Constrain cosmological parameters through joint gravitational wave and electro-magnetic observations SO 7 Understand stochastic gravitational wave backgrounds and their implications for the early Universe and TeV-scale particle physics SI 7.1 Characterise the astrophysical stochastic gravitational wave background SI 7.2 Measure, or set upper limits on, the spectral shape of the cosmological stochastic gravitational wave background SO 8 Search for gravitational wave bursts and unforeseen sources SI 8.1 Search for cusps and kinks of cosmic strings SI 8.2 Search for unmodelled sources