Citat:
Okej, då.
Detta kan jag dela:
"The Wow! signal (1977) remains the most compelling candidate for an extraterrestrial narrowband radio
transmission, but its origin has never been explained. Here we show that the signal can be understood as hyperfine
emission from dark hydrogen—a bound state of a dark electron and a dark proton—moving with a velocity of
4546 km s−1
toward the Solar System. This velocity is derived from a previously observed X-ray line at 619.89 eV
identified as Balmer-α of dark hydrogen, whose Doppler width of 9.4 eV implies the same bulk velocity. A friction
law v
2 = GM/R + αR with α ≈ 6.6 × 10−10 m s−2 naturally yields such velocities on galaxy cluster scales. The
dark atom model, with fine-structure constant α
′ = 0.16 and dark electron mass m′
e = 348.7 keV, predicts a
ground-state hyperfine transition at a rest frequency of 1399.0 MHz. Doppler shifting by the observed 4546 km s−1
gives exactly 1420.406 MHz—the Wow! frequency—to within 10−5
relative error. The required dark proton mass is
m′p = 240.3 GeV, consistent with a composite dark baryon. The 72−second duration implies a cloud size of
0.0044 AU, and the narrow bandwidth (< 10 kHz) indicates maser action in a cold, dense filament. Non-repetition
is explained by an unbound trajectory. We provide specific observational tests: searching for the same hyperfine
line at 1420.406 MHz and its n = 2 harmonic at ∼ 177.5 MHz, and detecting the 619.89 eV Balmer-α absorption
line in X-rays. If confirmed, the Wow! signal becomes the first spectroscopic identification of dark matter."
Detta kan jag dela:
"The Wow! signal (1977) remains the most compelling candidate for an extraterrestrial narrowband radio
transmission, but its origin has never been explained. Here we show that the signal can be understood as hyperfine
emission from dark hydrogen—a bound state of a dark electron and a dark proton—moving with a velocity of
4546 km s−1
toward the Solar System. This velocity is derived from a previously observed X-ray line at 619.89 eV
identified as Balmer-α of dark hydrogen, whose Doppler width of 9.4 eV implies the same bulk velocity. A friction
law v
2 = GM/R + αR with α ≈ 6.6 × 10−10 m s−2 naturally yields such velocities on galaxy cluster scales. The
dark atom model, with fine-structure constant α
′ = 0.16 and dark electron mass m′
e = 348.7 keV, predicts a
ground-state hyperfine transition at a rest frequency of 1399.0 MHz. Doppler shifting by the observed 4546 km s−1
gives exactly 1420.406 MHz—the Wow! frequency—to within 10−5
relative error. The required dark proton mass is
m′p = 240.3 GeV, consistent with a composite dark baryon. The 72−second duration implies a cloud size of
0.0044 AU, and the narrow bandwidth (< 10 kHz) indicates maser action in a cold, dense filament. Non-repetition
is explained by an unbound trajectory. We provide specific observational tests: searching for the same hyperfine
line at 1420.406 MHz and its n = 2 harmonic at ∼ 177.5 MHz, and detecting the 619.89 eV Balmer-α absorption
line in X-rays. If confirmed, the Wow! signal becomes the first spectroscopic identification of dark matter."
Bla bla bla signalen kommer från en dark proton eller vad är det egentligen du säger?
