Other
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002iaf..confe.512g&link_type=abstract
IAF abstracts, 34th COSPAR Scientific Assembly, The Second World Space Congress, held 10-19 October, 2002 in Houston, TX, USA.,
Other
Scientific paper
Institute of Space Studies of Catalonia (IEEC); Nexus Building; 2-4, Gran Capità St. Office 201; electromagnetic radiation. Neutrino radiation constitutes another way of looking through the universe, but still no progress has been made on this area due to the attribute of poor interaction of this radiation with matter. capable of revealing to us the very moment of its formation: that is gravitational radiation. systems, coalescent binaries, black holes... to the Big Bang itself. With electromagnetic waves, we are restricted to observe the Universe from the age when it was 300.000 years old up to now. With neutrino radiation, we can even reach a younger Universe: approximately when it was only one second old - at the end of the so-called leptonic epoch. But with gravitational radiation, we can access the very beginning of the Big Bang itself. reach limits not achievable until now. Furthermore, the detection of this sort of radiation could perhaps play the same role as the detection of electromagnetic waves by Heinrich Hertz in 1887: it would be experimentally and systematically studied, and this research would be a preliminary step for the formulation of a quantized theory of gravitation. The next step would be the consecution of a Unified Theory of all fundamental interactions. The detection of gravitational waves will open a new era in Science. their basic properties, their most likely sources and the different existing methods aiming to detect them.
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