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The finding that distant Type Ia supernovae are dimmer than expected has led to the notion that the rate of expansion of the universe is accelerating. I suggest an alternative model in which the extra dimness is caused by a postulated intrinsic small blueshift in these supernovae. (I should perhaps add at the outset that I do not support the Big Bang model, but rather a static, equilibrium-type model; that's probably why I automatically question this idae of universal acceleration.)
Here is the basic idea. When multiple redshifts are involved in observations it is incorrect to simply add them up, as is the usual practice, but rather they must be multiplied together. (In Stuart Clark’s book "Redshift", for instance, conventional astronomers use the correct multiplication formula to try to counter Arp’s interpretation of the large redshift of Markarian 205). A 'typical' composite redshift might be given by (1 + zc) = (1 + zH)(1 + zG)(1 + zD), where the 'subscripts' c, H, G and D stand for composite, Hubble, gravitational and Doppler respectively. Thus, if we have zH = 1 and zG = 1, then zc = 3, whereas merely adding them gives zc = 2. The composite redshift law could explain the dearth of quasars beyond z = 2, often hailed by Big Bang proponents as proof of ‘cosmic evolution’. The high intrinsic redshifts of quasars quickly inflate zc for these objects far beyond the value which would be obtained through simply adding the redshifts. I suggest a similar type of effect might be true for the Type Ia supernovae, but in reverse. If they have a small intrinsic blueshift zS, then the correct formula for their composite shift would be of the form (1 + zc) = (1 + zH)(1 + zS), where zS is now negative. At higher values for zc, we would see the effect of the small intrinsic blueshift progressively kick in. The distances to the more distant supernovae would be further than expected from the composite redshift alone. As to what could be causing the blueshift I don't have any suggestions, but merely note that some galaxies appear to have intrinsic blueshifts. |
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There are proximal causes and then there are ultimate causes. Discussions about proximal causes should pose no big problems for Big Bang supporters. After all, they accept universal expansion without having to know why this expansion is occurring. I am just talking about a possible proximal cause (of dim supernovae) here.
My information on the blueshifted galaxies comes from Arp's book Seeing Red. According to Arp, the galaxies in our system see the dominant galaxy of the system, M31, to be blueshifted. A similar pattern is seen within the members of the nearby M81 system. |
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E.E.M.
Whether dopler, gravitational and Hubble redshifts are added or multiplied does not change the conclusion; galaxies that are further away have a larger redshift. M31 is a very big, very nearby galaxie. It and the Milk Way are headed toward each other. So it is blue shifted. Galaxies in nearby clusters are also swirling around each other. Some of them happen to be heading towards us at this particular moment in cosmic time. So they are blueshifted. But as galaxies get fainter and smaller in the obsever's telescope, their redshift gets bigger. I agree the SNe's should be blueshifted. After all, we see what is beeing blasted towards us. More so with gamma ray bursts. If GRB's are relatavistic jets beamed straight at us, you'd expect a hefty blue shift in the emmission lines from the initial gamma rays. But all the emmission lines we get to measure are from the afterglow, which moves much more slowly. I think the real problem here is lack of a high resolution spectrometer in the 100 kev - 10 Mev range. ~Bub |
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We do of course see a blueshift of material heading outward from the core of a supernova (SN), toward us. The velocity is typically a few thousand kilometers per second, for a blueshift of, say, 1/30 or 3% (for a 10,000 km/s velocity, compared to 300,000 km/sec velocity of light). That's small compared to the redshift of a very distant supernova, with a z=1 for example. So as you get farther away, that blueshift becomes less important. Also, it's pretty much constant for every supernova and can be accounted for.
Now, an intrinsic blueshift that's enough to account for the acceleration would have definite observational effects. For example, a z=1 SN would suffer a time dilation, because of relativity. This effect is seen, clearly, in distant SNe. They can match the rise and decay time of the SN to the redshift, and see that they fit; that is, if you assume a redshift, that gives you a time dilation factor, and you can then slow down a "standard" SN light curve by that amount and see if it fits. If there were a significant intrinsic blueshift, that would alter that fit. This would at the very least put an upper limit to the intrinsic blueshift of a SN. I don't know if this has been done, but it is an interesting question. I'll ask around when I can. Bear in mind, though, that we see SNe at essentially zero redshift as well. That is, they are very close. An intrinsic blueshift would be seen to make a supernova appear to be headed toward us, even if it's in, say, the Virgo cluster, which has a definite redshift. I have never heard of this happening, and if it did, it would be huge news to the supernova community. Also, it would be easily observable to anyone with a spectrometer, so if this idea were right, I really think we'd have seen evidence of it by now. Just from that counterexample I strongly suspect this idea won't fly.
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Phil Plait The Bad Astronomer http://www.badastronomy.com badastro@badastronomy.com |
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Thanks BA. That helps.
Let me put my question very bluntly: If a jet of matter is accelerated in our direction from a distance of z=3.2769, and the ultimate velocity of the jet reaches 0.99835 c in our direction, what will the blue/redshift be? And second, how much spectroscopic resolution do we have available in the >1 Mev range? ~Bub |
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By the way, a review I read of Arp's book stated that there is not one mention of supernovas throughout the text. How can anyone deal with red shift without discussing supernovae evidence?
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Its interesting that Arp's anomalies are often dismissed because people don't like the proposed intrinsic redshift mechanism but it is ok to conclude Type Ia supernova indicate an accelerating universe even though the mechanism that causes Type Ia supernova is unknown (though thought to involve white dwarfs). |
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Toward us:
IC 3258............-517 km/s SBmp
M86 (NGC 4406).....-419 S0
M90 (NGC 4569).....-383 Sb+
NGC 4419...........-342 Ep
NGC 4318...........-300 E
M98 (NGC 4192).....-220 Sb I-II
Away from us:
NGC 4388...........+2535 km/s Sb
IC 3453............+2489 Ir+
NGC 4607...........+2367 SBb
NGC 4168...........+2342 E0
M99 (NGC 4254).....+2324 Sc I
NGC 4354...........+2305 SBb-p
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______________________________ Ref: http://www.seds.org/messier/more/virgo_gal.html
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Seriously though, I'm surprised the interstellar extinction factor was not determined directly for each of the SN Ia's (rather than adjusting the magnitude via formula... or not adjusting it at all). Extinction is detectable (and measurable) by the change in the ratios of light of different colors, indicating dust and gas have preferentially absorbed the blues or violets. After adjusting for Hubble flow redshift, astronomers can compare the spectra of nearby and distant supernovas. In the case of the two high-z supernova teams, it is quite possible that this was indeed done, with a finding that the spectra of near and distant supernovas were nearly identical - with the same relative amounts of light at each wavelength. If light from the distant supernovas was getting blocked by more gas and dust, the spectra would not be identical. Rowan-Robinson is right to question this remarkable finding that the expansion is accelerating, especially since there is no known mechanism that could make it accelerate. But more and better data is being collected, so we'll see if R-R's criticisms hold up.
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Everyone is entitled to his own opinion, but not his own facts. |
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NGC 4254 ScI +1281 NGC 4303 SBbcI +465 NGC 4321 SBbcI +588 NGC 4535 SBcI-II +891 NGC 4501 SbI-II (Seyfert) +947 NGC 4536 SBbcI-II +773 NGC 4192 SBbII -1133 NGC 4216 SBbII - 821 NGC 4548 SBbI-II -579 NGC 4569 SBabI-II -1059 Sab/Sb galaxies would have to have systematically approaching peculiar motions while ScI and Seyferts have systematically receding peculiar motions. And these are the largest galaxies - the ones that are supposed to be tossing around the smaller ones. And the large ellipticals (> 20kpc) in the core which have surface brightness fluctuation method distances: NGC 4365 -134 NGC 4374 -285 NGC 4406 -1400 NGC 4472 -204 NGC 4486 +240 NGC 4526 - 663 NGC 4552 -693 NGC 4621 -762 If we look at mean redshifts we find that the ellipticals with SBF distances break down the following way: > 20 kpc (9 galaxies) mean redshift = 784 km s-1 <20 kpc (18 galaxies) mean redshift = 1201 km s-1 For Sa/Sb spirals: rotational velocity (10) > 160 km s-1 mean redshift = 865 km s-1 rotational velocity (11) <160 km s-1 mean redshift = 1142 km s-1 for ScI/Seyferts: 11 galaxies mean redshift = 1854 km s-1 for ScII-III to ScIV galaxies: 18 galaxies mean redshift = 1310 km s-1 This is traditionally dismissed as a fluke, but there can be little doubt that there is a morphological/diameter pattern to the redshift distribution of Virgo Cluster galaxies which is certainly not expected in the traditional view. The morphological-density relation (Dressler 1980) does not explain this away because it cannot account for the systematic part of the pattern. |
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When I started this topic, I did not have any speculation on what could cause an intrinsic blueshift in Type Ia supernovae. But I've come up with one just now.
In Arp's aging of matter hypothesis, and also in some other theories (notably certain Le Sage-type theories), there is an increase in the mass of baryons over time. To simplify the discussion let's focus on the Arp/Narlikar model. In that model quasars for instance are very young objects which thus have low mass. This accounts for their high redshifts, since the subatomic particles in these objects all have lower masses as well. The Type Ia SNe, however, are older objects, much older than our sun. They are explosions occurring at the end of the stars' normal lifetimes, so I assume they're 10 billion years old or thereabouts. Consequently, if these objects started off with the same mass as the Sun, then they should have had a higher mass than the Sun's prior to their explosion. If we looked at their spectra at this time we would expect to see a slight blueshift, according to Arp's theory. The lines we see in a supernova are different lines than we normally see in a star, but they effectively should be blueshifted too. Elliptical galaxies in general should also have a slight blueshift relative to non-ellipticals, since ellipticals are mostly older stars. They may look redder, since they are cooler, but their lines should be slightly blueshifted. We might not see this effect at low z, because it's small. (In Arp's model, the increase in mass is exponential, and so the difference between the spectra of a star like our sun and an older star could be much smaller than in the earlier 'quasar' phases). So perhaps there is a way of testing the idea by looking at ellipticals. Incidentally, if Arp's mechanism were true, a star that was less than 1.4 times the solar mass (the limiting mass for Type Ia SNe) might attain the necessary mass to explode simply through aging! It would not be necessary to hypothesize mass being drained off companion stars, etc. |
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I believe numerous times there were publications about neutrinos having mass, and numerous times such claims were soon shot down. Apparently this claim has finally been made for the right reasons, with accurate data, and the claim is standing... so far.
__________________
Everyone is entitled to his own opinion, but not his own facts. |
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