Discrepancy in dark matter: a cosmic conundrum in the standard cosmological model

Abstract astrophysics Dark matter cosmology

An international team of astrophysicists and cosmologists has presented five papers suggesting that the aggregate (S8 value) of the universe’s dark matter is 0.76, a figure that lines up with other gravitational lensing surveys but not with the 0 value. 83 derived from the Cosmic Microwave Background.

An international team of scientists used advanced techniques and the Hyper Suprime-Cam to study the aggregation of dark matter, finding an S8 value of 0.76, which conflicts with the Cosmic Microwave Background value of 0.83. This discrepancy could indicate measurement errors or an incomplete standard cosmological model.

An international team of astrophysicists and cosmologists from various institutes, including the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), presented a series of five papers, which measure a value for the aggregation of dark matter of the universe, known to cosmologists as S8, of 0.76, which aligns with the values ​​that other gravitational lensing surveys have found when looking at the relatively recent universe, but does not align with the value of 0.83 derived from the Cosmic Microwave Background, which dates back to the origins of the universe when the universe was about 380,000 years old. Their results were uploaded as pre-printed articles to arXiv.

The gap between these two values ​​is small, but as more and more studies confirm each of the two values, it does not appear to be coincidental. Chances are that there is some as-yet-unrecognized error or error in one of these two measurements, or that the standard cosmological model is incomplete in some interesting way.

Dark energy and dark matter make up 95% of our universe that we see today, yet we understand very little about what they actually are and how they evolved throughout the history of the universe. Lumps of dark matter distort the light of distant galaxies through weak gravitational lenses, a phenomenon predicted by Einstein’s General Theory of Relativity.

Example image SSP HSC

Figure 1: An example of an image obtained with HSC-SSP. Credit: HSC-SSP project and NAOJ

This distortion is a very small effect indeed. The shape of a single galaxy is distorted by an imperceptible amount. But combining the measurements for millions of galaxies allows the distortion to be measured with quite high accuracy, said Kavli IPMU professor Masahiro Takada.

The Standard Model is defined by only a handful of numbers: the rate of expansion of the universe, a measure of how lumpy dark matter (S8), the relative contributions of the constituents of the universe (matter, dark matter, and dark energy), the overall density of the universe, and a technical quantity describing how the aggregation of the universe at large scales relates to that at small scales.

Cosmologists are eager to test this model by limiting these numbers in various ways, such as observing fluctuations in the cosmic microwave background, modeling the expansion history of the universe, or measuring the mass of the universe in the relatively recent past.

A team led by astronomers from Kavli IPMU, the University of Tokyo,[{” attribute=””>Nagoya University, Princeton University, and astronomical communities of Japan and Taiwan, have spent the past year teasing out the secrets of this most elusive material, dark matter, using sophisticated computer simulations and data from the first three years of the Hyper Suprime-Cam survey. The observations from this survey used one of the most powerful astronomical cameras in the world, the Hyper Suprime-Cam (HSC) mounted on the Subaru Telescope on the summit of Maunakea in Hawaii.

Subaru HSC Year 3 Results

Figure 2: The measurement results of S8 parameter from HSC-SSP Year 3 data. The chart shows the results from four different methods, which used different parts of the HSC-SSP Year 3 data or combined the HSC-SSP Year 3 data with other data. For comparison, Planck CMB shows the measurement result for S8 from the cosmic microwave background data from the Planck satellite. Other weak lensing results shows the results from similar weak lensing measurements based on the Dark Energy Survey (DES) and Kilo-Degree Survey (KiDS) data. Credit: Kavli IPMU

Hiding and uncovering the data

The team performed a blinded analysis.

Scientists are human beings, and they do have preferences. Some would love to really find something fundamentally new, while others might feel comfortable if they find results that look consistent with foreseen results. Scientists have become self-aware enough to know that they will bias themselves, no matter how careful they are, unless they carry out their analysis without allowing themselves to know the results until the end, said Nagoya University Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI)Associate Professor Hironao Miyatake.

To protect the results from such biases, the HSC team hid their results from themselves and their colleagues for months. The team even added an extra obfuscating layer: they ran their analyses on three different galactic catalogs, one real and two fake with numerical values offset by random values. The analysis team didnt know which of them was real, so even if someone did accidentally see the values, the team wouldnt know if the results were based on the real catalog or not.

The team spent a year on the blind analysis. On December 3 2022, the team gathered together on Zoom one Saturday morning in Japan, Friday evening in Princeton for the unblinding. The team unveiled the data, and ran their plots, immediately they saw it was great according to Takada. Blinded analysis means you cannot take a peak at the results while running the analysis, which was extremely stressful, but as soon I saw the final result, all of that anxiety flew out of the window, said Kavli IPMU graduate student Sunao Sugiyama.

3D Distribution of Dark Matter Derived From HSC-SSP

Figure 3: An example of a 3D distribution of dark matter derived from HSC-SSP. This map is obtained by using the first years data, but the present study examined an area on the sky about three times larger than that. Credit: University of Tokyo/NAOJ

A huge survey with the worlds largest telescope camera

HSC is the largest camera on a telescope of its size in the world. The survey that the research team used covers about 420 square degrees of the sky, about the equivalent of 2000 full moons. It is not a single contiguous chunk of sky, but split among six different pieces, each about the size of a persons outstretched fist. The 25 million galaxies the researchers surveyed are so distant that instead of seeing these galaxies as they are today, the HSC recorded how they were billions of years ago.

Each of these galaxies glows with the fires of tens of billions of suns, but because they are so far away, they are extremely faint, as much as 25 million times fainter than the faintest stars we can see with the naked eye.

For more on this research, see Measuring Dark Matter With Hyper Suprime-Cam Reveals Discrepancy.

References:

Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model by Hironao Miyatake, Sunao Sugiyama, Masahiro Takada, Takahiro Nishimichi, Xiangchong Li, Masato Shirasaki, Surhud More, Yosuke Kobayashi, Atsushi J. Nishizawa, Markus M. Rau, Tianqing Zhang, Ryuichi Takahashi, Roohi Dalal, Rachel Mandelbaum, Michael A. Strauss, Takashi Hamana, Masamune Oguri, Ken Osato, Wentao Luo, Arun Kannawadi, Bau-Ching Hsieh, Robert Armstrong, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Lauren A. MacArthur, Satoshi Miyazaki, Hitoshi Murayama, Yuki Okura, Paul A. Price, Tomomi Sunayama, Philip J. Tait, Masayuki Tanaka and Shiang-Yu Wang, 3 April 2023, Astrophysics > Cosmology and Nongalactic Astrophysics.
arXiv:2304.00704

Hyper Suprime-Cam Year 3 Results: Measurements of Clustering of SDSS-BOSS Galaxies, Galaxy-Galaxy Lensing and Cosmic Shear by Surhud More, Sunao Sugiyama, Hironao Miyatake, Markus Michael Rau, Masato Shirasaki, Xiangchong Li, Atsushi J. Nishizawa, Ken Osato, Tianqing Zhang, Masahiro Takada, Takashi Hamana, Ryuichi Takahashi, Roohi Dalal, Rachel Mandelbaum, Michael A. Strauss, Yosuke Kobayashi, Takahiro Nishimichi, Masamune Oguri, Arun Kannawadi, Robert Armstrong, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Satoshi Miyazaki, Hitoshi Murayama, Yuki Okura, Paul A. Price, Philip J. Tait, Masayuki Tanaka and Shiang-Yu Wang, 3 April 2023, Astrophysics > Cosmology and Nongalactic Astrophysics.
arXiv:2304.00703

Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model by Sunao Sugiyama, Hironao Miyatake, Surhud More, Xiangchong Li, Masato Shirasaki, Masahiro Takada, Yosuke Kobayashi, Ryuichi Takahashi, Takahiro Nishimichi, Atsushi J. Nishizawa, Markus M. Rau, Tianqing Zhang, Roohi Dalal, Rachel Mandelbaum, Michael A. Strauss, Takashi Hamana, Masamune Oguri, Ken Osato, Arun Kannawadi, Robert Armstrong, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Satoshi Miyazaki, Hitoshi Murayama, Yuki Okura, Paul A. Price, Philip J. Tait, Masayuki Tanaka and Shiang-Yu Wang, 3 April 2023, Astrophysics > Cosmology and Nongalactic Astrophysics.
arXiv:2304.00705

Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra by Roohi Dalal, Xiangchong Li, Andrina Nicola, Joe Zuntz, Michael A. Strauss, Sunao Sugiyama, Tianqing Zhang, Markus M. Rau, Rachel Mandelbaum, Masahiro Takada, Surhud More, Hironao Miyatake, Arun Kannawadi, Masato Shirasaki, Takanori Taniguchi, Ryuichi Takahashi, Ken Osato, Takashi Hamana, Masamune Oguri, Atsushi J. Nishizawa, Andrs A. Plazas Malagn, Tomomi Sunayama, David Alonso, Ane Slosar, Robert Armstrong, James Bosch, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Lauren A. MacArthur, Satoshi Miyazaki, Hitoshi Murayama, Takahiro Nishimichi, Yuki Okura, Paul A. Price, Philip J. Tait, Masayuki Tanaka and Shiang-Yu Wang, 3 April 2023, Astrophysics > Cosmology and Nongalactic Astrophysics.
arXiv:2304.00701

Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions by Xiangchong Li, Tianqing Zhang, Sunao Sugiyama, Roohi Dalal, Markus M. Rau, Rachel Mandelbaum, Masahiro Takada, Surhud More, Michael A. Strauss, Hironao Miyatake, Masato Shirasaki, Takashi Hamana, Masamune Oguri, Wentao Luo, Atsushi J. Nishizawa, Ryuichi Takahashi, Andrina Nicola, Ken Osato, Arun Kannawadi, Tomomi Sunayama, Robert Armstrong, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Satoshi Miyazaki, Hitoshi Murayama, Takahiro Nishimichi, Yuki Okura, Paul A. Price, Philip J. Tait, Masayuki Tanaka, Shiang-Yu Wang, 3 April 2023, Astrophysics > Cosmology and Nongalactic Astrophysics.
arXiv:2304.00702


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