| Jan 28, 2026 |
Researchers developed a method to reduce uncertainty in cosmic birefringence, sharpening the angle tied to parity violation, dark matter, and dark energy.
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(Nanowerk News) A team of researchers studying the uncertainties associated with a phenomenon known as cosmic birefringence has developed a method to reduce uncertainties in its observational measurements, according to a new study published in Physical Review Letters (“𝑛𝜋 Phase Ambiguity of Cosmic Birefringence”).
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This study is the first to quantitatively address the uncertainty surrounding the birefringence angle, which is a crucial observational quantity that could provide clues to unknown physical theories breaking the universe’s left-right symmetry, and to understanding dark matter and dark energy.
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| Figure 1: Conceptual diagram of the 180-degree phase indeterminacy arising when measuring the rotation angle of cosmic birefringence. Light (represented by the yellow character in the diagram) possesses a direction called polarization (shown as red lines in the diagram). The phenomenon where this direction rotates during light propagation is called “cosmic birefringence.” Since researchers can only observe the current state, they cannot distinguish between all the states depicted in the diagram. Although the light character in the diagram has a face, it obviously has no face in reality, so researchers must judge solely based on the direction of polarization. (Image: Naokawa, Namikawa, higgstan.com)
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The cosmic microwave background, the afterglow of the Big Bang, carries crucial information about the universe’s earliest moments. Recent observations have found hints of a subtle rotation in the polarization of this ancient light – a phenomenon known as cosmic birefringence. This rotation is thought to conceal unknown elementary particles called axions. Accurately measuring the rotation angle of cosmic birefringence (the birefringence angle) is important for unraveling the underlying unknown physical theory. The rotation angle can be investigated by measuring the amplitude of a signal called the CMB EB correlation (Figure 2). Previous measurements have reported it to be approximately 0.3 degrees.
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A research team led by the University of Tokyo Graduate School of Science PhD candidate Fumihiro Naokawa, together with Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI) Project Associate Professor Toshiya Namikawa, conducted a detailed investigation into the uncertainties associated with cosmic birefringence. The study found that the rotation angle may be larger than the previously reported value of about 0.3 degrees.
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| Figure 2: Theoretically calculated EB correlations. The EB correlation signal is similar for all rotation angles shown here and is nearly indistinguishable (top figure). However, enlarging the leftmost region of the top figure (indicated by the arrow) reveals differences in the signal shape (bottom figure). (Image: Naokawa et al.)
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“Can you tell what day it is, just by looking at a clock? No, you cannot. To determine the date from the clock hands, you need to know how many times the hands have rotated since a specific reference date and time. In scientific terms, a situation like this clock’s hands—where observing only the current state does not reveal how many rotations occurred in the past—is described as having 360-degree phase ambiguity.
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“Like a clock, the CMB we can observe is only in its current state. Therefore, rotation angles such as 0.3 degrees, 180.3 degrees, and 360.3 degrees should be indistinguishable. This means the birefringence angle has a phase ambiguity of 180 degrees,” said Naokawa.
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The researchers developed a way to resolve this ambiguity, after finding that the shape of the EB correlation signal can encode information about how many rotations the polarization direction underwent. Looking at the details of the EB correlation could resolve this ambiguity.
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The uncertainty reduction method developed by the researchers will provide a technique for future observations of cosmic birefringence using high-precision data and for verifying the underlying physical theories such as those from the Simons Observatory and LiteBIRD.
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Furthermore, the team has newly discovered that when phase uncertainty is taken into account, cosmic birefringence also affects another type of CMB signal known as the EE correlation. The EE correlation is a key observable used to determine the Universe’s “optical depth” that can be used to explore cosmic reionization. As a result, this finding may require revisions to previously reported measurements of the optical depth.
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In a separate paper also published in Physical Review Letters (“Universal Profile for Cosmic Birefringence Tomography with Radio Galaxies”), author Naokawa studied methods to overcome errors generated by a telescope itself when observing cosmic birefringence. He uncovered a new method to confirm the phenomenon using specific types of celestial objects, including radio galaxies powered by supermassive black holes, which may help future researchers uncover the nature of dark energy.
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