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Logo: Sonderforschungsbereich geo-Q
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C03 - Clock network modeling

Figure 01: isometric embedding of fully general relativistic equipotential surfaces
Figure 01: An example of an isometric embedding of fully general relativistic equipotential surfaces (in particular the geoid) of a space-time of a quadrupoler, rotating, axially symmetric mass distribution.

In general, networks of high precision clocks and their comparison enable the very precise determination of the relative gravitational potential (and the relative velocity). In this project we investigate the capabilities of such networks of the new generation of optical clocks connected by optical fiber links for a variety of applications such as Earth gravity field determination, time comparison or synchronization, navigation and positioning, and also fundamental physics tests. Since clocks directly measure the gravitational potential this opens up a fundamentally new concept for physical geodesy, that is, for e.g. geoid determination and the realization of a new global dynamic reference system. For the latter we will also make use of clocks in space.

For the thorough theoretical description of clocks and networks of clocks, one has to take into account all special and general relativistic effects like gravitational redshift, Doppler effect, gravitational time delay, Sagnac effect, and even the Lense-Thirring effect for clocks (gravito-magnetic clock effect). In fact, these effects give the information about the clocks’ relative motion and the gravitational field at their location. Based on this we then can model mass and height variations affecting the clock measurement, e.g., related to solid Earth tides.

We split this task into three main steps and an add-on regarding tests of Special and General Relativity.

  • Calculation of all (relativistic) effects within clock networks on Earth.
  • Investigation of new and possibly more powerful and effective concepts for height determination over long distances or to remote areas (islands) based on networks of clocks on Earth (and possibly with the help of clocks in space).
  • Development of fully relativistic notions for geodesy, e.g., a fully relativistic geoid based on clocks as well as on freely falling bodies (see figure 01).
  • Geodetic modeling of time-dependent gravitational fields, i.e. modeling of all relevant mass variations (mainly tidal effects) arising during the measurement time and between the epochs.
  • As an add-on we would like to analyze whether these high precision clocks in the gravitational field of the Earth can also be used for new high precision tests of Special and General Relativity.

This project will also prepare the theoretical foundations for the description of clocks with accuracies better than the present one and also serves as interface project between physics/General Relativity and geodesy. 

Scientists working on this project

Dr.-Ing. Hu Wu
email: wuhuife.uni-hannover.de

phone: +49 511 762-4891
details

Selected Publications


Peer-Reviewed Literature

Philipp D., Perlick V., Puetzfeld D., Hackmann E. and Lämmerzahl C. (2017): Definition of the relativistic geoid in terms of isochronometric surfaces, Phys. Rev. D 95, 104037
DOI: 10.1103/PhysRevD.95.104037
arXiv: 1702.08412

Philipp D., Pützfeld D. and Lämmerzahl C. (2016): On the applicability of the geodesic deviation equation in General Relativity (submitted)
arXiv: 1604.07173

Pützfeld D. and Obukhov Y.N. (2016): Generalized deviation equation and determination of the curvature in General Relativity, Phys. Rev. D 93 (2016) 044073
DOI: 10.1103/PhysRevD.93.044073
arXiv: 1511.08465

Obukhov Y.N., Portales-Oliva F., Pützfeld D. and Rubilar G.F. (2015): Invariant conserved currents in generalized gravity, Phys. Rev. D 92 (2015) 104010
DOI: 10.1103/PhysRevD.92.104010
arXiv: 1507.02191

Pützfeld D. and Obukhov Y.N. (2015): Equivalence principle in scalar-tensor gravity, Phys. Rev. D 92 (2015) 081502(R)
DOI: 10.1103/PhysRevD.92.081502
arXiv: 1505.01285

Obukhov Y.N. and Pützfeld D. (2014): Equations of motion in scalar-tensor theories of gravity: A covariant multipolar approach, Phys. Rev. D 90 (2014) 104041
DOI: 10.1103/PhysRevD.90.104041
arXiv: 1404.6977


Non Peer-Reviewed Literature

Müller J. (2016): Erdmessung mit Quanten und Relativität, BWG Jahrbuch 2016
arXiv: 1608.08407

Obukhov Y.N. and Pützfeld D. (2016): Dynamics of test bodies in scalar-tensor theory and equivalence principle, Gravitation, Astrophysics, and Cosmology - Proceedings of the Twelfth Asia-Pacific International Conference, Moscow, 28 Jun - 5 July 2015, Eds. V. Melnikov and J.-P. Hsu, World Scientific (Singapore), 2016, pp. 231-235
DOI: 10.1142/9789814759816_0043
arXiv: 1603.09106

Obukhov Y.N. and Pützfeld D. (2015): Multipolar test body equations of motion in generalized gravity theories, Equations of Motion in Relativistic Gravity, D. Pützfeld et. al. (eds.), Fundamental theories of Physics 179, pages 67-119, Springer 2015
DOI: 10.1007/978-3-319-18335-0_2
arXiv: 1505.01680

Philipp D. and Pützfeld D. (2015): On geodesic deviation in static spherically symmetric situations, April 2016, Proceedings of the 14th Marcel Grossmann Meeting, July 12-18, 2015, Rome, Italy


Presentations, Talks and Posters

Pützfeld D. (2016): The Measurement of the Gravitational Field in General Relativity, Relativity seminar, University of Cologne, Germany.