Aeon Ideas
published at RCP on November 29, 2016
 
 
Has dogma derailed  the scientific search for dark matter?

 
Paul Kroupa
 
 
 


 
According to mainstream researchers, the vast majority of the matter in  
the Universe is invisible: it consists of dark-matter particles that do not  
interact with radiation and cannot be seen through any telescope. The case 
for  dark matter is regarded as so overwhelming that its existence is often 
reported  as fact. Lately, though, cracks of doubt have started to appear. In 
July, the  LUX experiment in South Dakota came up _empty_ 
(https://news.brown.edu/articles/2016/07/lux)  in its search for dark particles 
– the  latest 
failure in a planet-wide, decades-long effort to find them. Some cosmic  
surveys also suggest that dark particles cannot be there, which is especially  
confounding since astronomical observations were the original impetus for 
the  dark-matter hypothesis. 
The issues at stake are huge. Acceptance of dark matter has influenced  
scientific thinking about the birth of the Universe, the evolution of galaxies  
and black holes, and the fundamental laws of physics. Yet even within 
academic  circles, there is a lot of confusion about dark matter, with evidence 
and  interpretation often conflated in misleading and unproductive ways. 
The modern argument for dark matter begins with the assumption that the  
Universe is described by Albert Einstein’s field equation of general 
relativity,  and that Newtonian gravitation (that is, gravity as we measure it 
on 
Earth) is  valid in all places at all times. It further assumes that all the 
matter in the  Universe was produced at the Big Bang. Simulations based on 
that scenario make  specific predictions about how quickly cosmic structures 
form, and also about  the motions of galaxies and stars within galaxies. When 
compared with  observations, those simulations indicate that gravitational 
effects in the real  world must be stronger than can be accounted for by the 
matter we know. Dark  matter provides the additional gravitational pull to 
bring model and reality  broadly into alignment. Researchers now routinely 
take this model – Einstein  plus dark matter, often called the ‘null 
hypothesis’ – as their starting point  and then perform detailed calculations 
of 
galactic systems to test  it. 
 
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This is how I stumbled into the _field_ 
(https://astro.uni-bonn.de/~pavel/kroupa_SciLogs.html)  in the late 1990s. I 
was studying the  dynamics of 
small satellite galaxies as they orbit our galaxy, the Milky Way.  From 
observation, we expected that these satellite galaxies must contain a lot  of 
dark 
matter, from 10 to 1,000 times as much as their visible, normal matter.  
During my calculations, I made a perplexing discovery. My simulations produced  
satellite galaxies that look much like the ones actually observed, but they  
contained no dark matter. It seemed that observers had made wrong 
assumptions  about the way the stars move within the satellite galaxies; dark 
matter 
was not  required to explain their structures. 
I _published_ (http://adsabs.harvard.edu/abs/2010A&A...523A..32K)  these 
results and quickly learned what  it meant to not follow the mainstream. 
Despite the critiques I received, I  followed up on these results some years 
later and _uncovered_ (http://adsabs.harvard.edu/abs/2012PASA...29..395K) 
another major inconsistency. The known  satellite galaxies of the Milky Way are 
distributed in a vast polar disk running  perpendicular to the orientation of 
our galaxy. But dark-matter dominated models  predict that primordial dwarf 
galaxies should have fallen into the Milky Way  from random directions, so 
should follow a spheroidal distribution. This finding  set off a major 
debate, with the mainstream researchers arguing that this disk  of satellites 
does 
not really exist; that it is not significant; or that it  cannot be used to 
test models. 
Meanwhile, astronomers kept identifying new dwarf satellite galaxies that  
made the disk structure even more pronounced. Rodrigo Ibata at Strasbourg  
Observatory _showed_ (http://adsabs.harvard.edu/abs/2013Natur.493...62I)  
that our neighbouring galaxy,  Andromeda, has an even more pronounced disk of 
satellite galaxies. My team at the University  of Bonn then _found_ 
(http://adsabs.harvard.edu/abs/2013MNRAS.435.1928P)  that the disks of 
satellites 
around  Andromeda and the Milky Way appear to be aligned, and that the whole 
structure  of our Local Group of galaxies is highly symmetrical. Ibata and his 
team  subsequently confirmed that the observed distribution of matter does 
not match  dark-matter predictions out to distances of 24 million light 
years. 
More problems: when a dwarf galaxy with a dark-matter halo passes through  
the dark-matter halo of a large galaxy, the dark-matter halos should absorb 
the  energy of motion such that the dwarf galaxy would fall to the centre of 
the  large galaxy, somewhat like a marble dropped in honey. This is a 
well-studied  process known as dynamical friction but it is not evident in the 
astronomical  data, suggesting that the expected dark-matter haloes do not 
exist. Most  recently, Stacy McGaugh at Case Western Reserve University in Ohio 
and his  team _documented_ (https://arxiv.org/abs/1609.05917)  that the 
pattern of rotation in spiral  galaxies seems to precisely follow the pattern 
of the visible matter alone,  posing yet another challenge to the null 
hypothesis. 
In light of these findings, I  argue that the null hypothesis must be 
discarded. What can it be replaced with?  The first step is that we need to 
revisit the validity of Newton’s universal law  of gravitation. Starting in the 
1980s, Mordehai Milgrom at the Weizmann  Institute in Israel _showed_ 
(http://adsabs.harvard.edu/abs/1999PhLA..253..273M)  that a small 
generalisation of 
Newton’s  laws can yield the observed dynamics of matter in galaxies and in 
galaxy  clusters without dark matter. This approach is broadly known as 
MOND (MOdified  Newtonian Dynamics). Milgrom’s _correction_ 
(http://adsabs.harvard.edu/abs/2009ApJ...698.1630M)  allows gravitational 
attraction to fall  
off with distance more slowly than expected (rather than falling off with the 
 square of distance as per Newton) when the local gravitational 
acceleration  falls below an extremely low threshold. This threshold could be 
linked to 
other  cosmological properties such as the ‘dark energy’ that accounts for 
the  accelerating expansion of the Universe. 
These links suggest a deeper fundamental theory of space, time and  matter, 
which has not yet been formulated. Few researchers have pursued such an  
alternative hypothesis, partly because it seems to question the validity of  
general relativity. However, this need not be the case; additional physical  
effects related to the quantum physics of empty space and to the nature of 
mass  might be playing a role. MOND also faces its own challenges, both 
observational  and theoretical. Its biggest drawback is that MOND is not yet 
well-anchored to  general relativity. Because of the prevailing dark-matter 
dogma, few scientists  dare to build on Milgrom’s ideas. Young researchers risk 
not getting a job;  senior researchers face losing out on grants. 
Together with Benoit Famaey in Strasbourg, my small group in Bonn is  
moving ahead anyway. Yes, we are being punished by not being granted some  
research money, but in our computers we are _discovering_ 
(https://arxiv.org/abs/1610.03854)  a universe full of galaxies that look  just 
like the real things 
– and this is awfully exciting. MOND could be the next  great advance in 
gravitational research, building on the work of Newton and  Einstein. This year
’s detection of gravitational waves allows exciting new  possibilities. 
Those waves have travelled cosmological distances, and so have  passed through 
regions where Milgrom’s low-threshold effect should be  significant. 
Gravitational wave studies will provide the kind of data needed to  refine our 
ideas about MOND, and to explore cosmological thinking outside the  constraints 
of dogma

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