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Quantum Gravity : Mathematical Models and Experimental Bounds

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16 Claus Lämmerzahl<br />

compared with the st<strong>and</strong>ard results. Therefore, one trivial answer to the above<br />

questionsisthatany experiment is also an experiment searching for QG effects.<br />

However, from general considerations one may extract some kind of strategy of<br />

where it is preferable to look for such effects, that is, in which situations QG<br />

effects are expected to show up more pronounced than in other situations. This is<br />

one issue addressed in this contribution.<br />

Another aspect is the present status of experimental test of the validity of<br />

the st<strong>and</strong>ard theories. The validity of a theory relies on the experimental verification<br />

of the basic principles or foundations of the theory under consideration. This<br />

experimental exploration defines the ”l<strong>and</strong>scape” of the experimentally explored<br />

regime which then is covered by st<strong>and</strong>ard theories. QG effects can be present only<br />

outside this explored domains.<br />

These remarks define the outline of this paper: At first we recall the basic<br />

principles present day st<strong>and</strong>ard physics relies on. This is the Einstein Equivalence<br />

Principle which essentially determines the structure of all equations of motion. This<br />

is followed by a compact review of most of the experiments aimed at testing the<br />

Einstein Equivalence Principle. Then we come to open problems (“dark clouds”)<br />

of present physics which found no explanation so far. This leads us to the issue of<br />

how we could search for QG effects. We discuss the expected magnitude of these<br />

effects <strong>and</strong> also where we might expect QG effects <strong>and</strong> how we should search for<br />

these effects. That is, we discuss some strategy for the search for QG effects. We<br />

close this contribution by outlining which experimental progress we can we expect<br />

in the future.<br />

2. The basic principles of st<strong>and</strong>ard physics<br />

The basic principle of st<strong>and</strong>ard physics is the Einstein Equivalence Principle which<br />

consists of three parts<br />

The Universality of Free Fall (UFF): This principle states that in a gravitational<br />

field all kinds of structureless matter fall in the same way. In principle,<br />

this is an amazing fact; gravity is the only interaction with this property. In<br />

the frame of elementary particle theory this just means that all elementary<br />

particles fall in the gravitational field in the same way. Therefore one carries<br />

through experiments with various macroscopic species of materials with<br />

different proton to neutron ratio.<br />

The Universality of the Gravitational Redshift (UGR): This universality means<br />

that all clocks based on non-gravitational physics behave in the same way<br />

when moved together in gravitational fields. This again is an amazing fact<br />

<strong>and</strong> means that in addition to all particles also all (non-gravitational) interactions<br />

(also represented by particles) couple to the gravitational field in the<br />

same way. Again, one has to test this for all kinds of clocks <strong>and</strong> to analyze<br />

the results in terms of the coupling of elementary particles to gravity.

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