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Published on: November 15, 2013
Constraining the noncommutative spectral action via astrophysical observations
William Nelson1, Joseph Ochoa, Mairi Sakellariadou
1Institute of Gravitation and the Cosmos, Penn State University, State College, Pennsylvania 16801, USA. nelson@gravity.psu.edu
This study constrains a modified Einstein-Hilbert gravity theory using pulsar timing. Current observations show no deviations from general relativity, but future data may offer stronger constraints on this noncommutative spectral action.
Area of Science:
- Theoretical Physics
- Quantum Gravity
- Particle Physics
Background:
- The noncommutative spectral action provides a framework for unifying particle physics and gravity.
- It extends commutative spaces using spectral triples on almost commutative spaces.
Purpose of the Study:
- To constrain the gravitational sector of the noncommutative spectral action.
- To test for deviations from general relativity using astrophysical observations.
Main Methods:
- Utilizing pulsar timing observations.
- Comparing observational data with predictions from a modified Einstein-Hilbert gravity theory.
Main Results:
- Established weak bounds on the coupling constants of the modified gravitational theory.
- Demonstrated that current pulsar timing data shows no significant deviation from general relativity.
Conclusions:
- The noncommutative spectral action's gravitational sector is constrained, though current bounds are weak.
- Future pulsar timing observations hold potential for more stringent tests of this theory and general relativity.
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