Figure
1: The positions in galactic coordinates of the GRBs in the BATSE 4B
catalog, showing the isotropy of the burst sky distribution (see C.A.
Meegan, et al., Nature, vol. 355, 1993, p. 143.
by Eric J. Heller
Departments of Chemistry and Physics
Harvard University, Cambridge, Massachusetts
Gamma-ray bursts pose one of the greatest mysteries of modern astrophysics. Almost every day, there is a huge, localized burst of gamma-rays lighting up the sky, which often outshines all the other gamma ray sources in the sky put together. Then the source of the burst vanishes, often in a few seconds. The bursts come from all over the sky, seemingly at random. Until now there has been no convincing explanation for them. The answer, it turns out, may be automotive in nature
The Mystery of Gamma Ray Bursts
Gamma ray bursts (GRB) were discovered in 1967 by satellite-borne detectors looking for violations of the Nuclear Test Ban Treaty. They are extremely bright sources of radiation, typically lasting for seconds. Some are very sharply peaked in time, others have a longer falloff. Burst time-scales go through the 30 ms scale to hundreds of seconds. Even if the GRBs we see are somehow collimated toward us (as we shall argue they are) , they are by far the brightest electromagnetic events in the Universe. They are more or less randomly distributed across the sky, as seen in Figure 1, and happen about once a day. There is strong evidence that the GRBs seen so far are extragalactic, since recent observations have associated faint galaxies to the burst sights. It is now known that they emanate from distant galaxies. While the bursts were detected in the gamma region of the spectrum, there are also x-ray and visible portions of the spectrum. GRBs remain an active area of research [1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20]. Typical bursts are shown in Figure 2 . A galaxy from which another burst originated is shown in Figure 3.
Figure
2: Sample of GRBs detected by the BeppoSAX/GRBM. It shows just an
example of the possible morphology, duration and intensity variety of
the GRBs
Explanation
The explanation of GRBs falls into place if we consider the activities of extraterrestrial intelligent beings. It is assumed that such beings, in our galaxy or other galaxies, are quite capable of space travel over great distances, at speeds near the speed of light, c. The relativistic time dilationSpace travel at relativistic speeds is not without its hazards. It is well known that “brown” matter and other debris populates intragalactic space, and perhaps intergalactic space, with some density. Objects ranging in size from baryons and atoms to masses of the order of Jupiter might be encountered, though the larger ones would certainly be known ahead of time, or easily seen. Smaller sized objects are another issue. We assume here that a collision at relativistic speeds with something the size of a baseball, or perhaps even small molecules, is bad even for space vehicles of very advanced societies. At the very least, such vehicles must “look ahead” for larger objects it would collide with, and move out of the way when they are detected. It should also have a way of moving the much more numerous small objects out of harm’s way.
In other words, space ships must have headlights, and perhaps beams powerful enough to disintegrate or displace small bodies well in advance of arrival. These would naturally need to be extremely collimated. The requirement to see far enough ahead might make them quite energetic. An observer along the line of the path vehicle would always see very blue shifted (i.e., mostly gamma) radiation, since we would see only those beams from ships traveling directly toward us at relativistic speeds. But why do we see a “burst” of 0.1–10 seconds?
Figure
3: Galactic region (left) and host galaxy (right) from which the gamma
ray burst GRB 9901231 originated (from reference 21
Proposal for a Test
The solar system is sufficiently large to test the idea of extreme collimation of the beam. Let us suppose that the beam has an initial width of 100 m, with a mean wavelength of 10-12 m, in the gamma region. Using the asymptotic formula for the spreading of a Gaussian beam (Born and Wolf, Principles of Optics), we have the angular spread in radians, given by radians (1)After one billion years of travel this beam would spread to a size of about 106 kilometers, only about 1% of the earth-sun distance. If the GRBs are remnants of destruction beams, their width at the beam waist might be 100 times smaller, giving a width a billion years later on the order 1 AU. These figures make it worthwhile to contemplate building a solar orbiting gamma ray camera, in order to detect differences between arrival signatures on earth and on the satellite which might reveal a beam width on the order of a few AUs or less.
Conclusion
We have shown that GRBs are explained as byproducts of narrowly collimated headlights and protection beams of extraterrestrial vehicles in other galaxies, where the bursts are known to originate. These beams would have an approximately 10–15 radian spread. This explanation requires ten to twenty orders of magnitude less energy in the source than an assumed astrophysical “collimated” source with a beam spread of 1 to 10 degrees.
Figure 4. Headlights. This particular example is of terrestrial origin.
The GRBs originate only within distant galaxies as far as we know. This is easily explained, since extragalactic travel is either out of the question (even for advanced societies) because of the great distances involved, or else intergalactic space is so empty that it is common practice to leave your headlights off when traveling between galaxies.
Editor’s note: This work is consonant with the evidence amassed by Scott Sandford of NASA that internal combustion engines may be common in interstellar space. See “Proof that UFOs are Powered by Internal Combustion Engines,” Scott A. Sandford, AIR 6:2.
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