Being a physicist, I have a deep appreciation for all small particles. Each particle plays a crucial role in the universe, and by studying them, we gain a better understanding of the fundamental laws of nature that govern our existence. However, as a researcher in the field of Dark Matter, I must confess that Neutrinos present a unique challenge.

Neutrinos are elusive little particles. From their inception, they defied all expectations.

Confronted with this dilemma, physicists had two unsatisfactory options: either abandon the conservation of energy or posit the existence of invisible particles that could not be detected by conventional means. They opted for the latter, eventually coining the term “Little Neutral” for these new particles, which possessed no charge and were abundant in quantity.

The absence of charge was the defining feature – without charge, the particles do not interact at all through electromagnetic force. This led physicist Wolfgang Pauli to famously remark, “I have done a terrible thing. I have postulated a particle that cannot be detected.”

Fortunately, Pauli’s skepticism about detectability was proven wrong in the end. Neutrinos, though notoriously resistant to interactions with other particles, do pass through our planet on a daily basis without our notice. It took a truly heroic effort to develop instruments capable of detecting them.

Even now, we are still struggling to capture neutrinos. The standard detection method involves constructing large water tanks deep underground or filled with other liquids (to shield them from cosmic rays). Each day, researchers anxiously wait for one of the four neutrinos that pass through the Earth to directly collide with an atom underwater.

If such a collision occurs, a flash of light is produced as the charged particles in the water move quickly. This light flash acts like an electromagnetic version of the Sonic boom, encoding information about neutrinos and providing insights into these invisible particles that constantly permeate the Earth.

Read more:

Most of the neutrinos detected on Earth come from the solar nucleus. When hydrogen fuses with helium, neutrinos are produced as by-products. They emanate in all directions as soon as they are generated, mostly unaffected by the sun’s mass, and escape into space.

The reason neutrinos pose a specific challenge to dark matter detectors is their similarity to the hypothetical dark matter particles we seek known as Weakly Interacting Massive Particles (WIMPs). Like neutrinos, these “weakly interacting massive particles” have no charge and can traverse the Earth unnoticed.

If they do interact with other matter, it is through weak nuclear force – the same force that may (albeit rarely) cause neutrinos to interact with the underwater particles in the neutrinoscope. Similar to neutrino detectors, dark matter detectors are situated deep underground to shield them from cosmic rays, designed to register any interactions occurring within the detector with these invisible particles.

The challenge arises from the fact that the dark matter detector has become incredibly sensitive, picking up signals caused by neutrinos. Both types of detectors have now produced evidence of solar neutrinos colliding with target materials. The amount of rock cover cannot adequately shield experiments from neutrinos.

It may take several decades for a dark matter signal detector unaffected by solar neutrino interference to achieve total clarity. Currently, most detectors are only sensitive to high-energy solar neutrinos, which have been causing complications thus far.

Some physicists are intrigued by the phenomenon of “coherent neutrino scattering” and see it as an opportunity to overcome the challenges of both dark matter detection and neutrino interference. Ultimately, dark matter may be composed of an entirely different substance.

Nevertheless, if dark matter does indeed comprise WIMPs, we will need to think outside the box in our experiments. For those of us delving into the mysteries of the universe’s dark side, the seemingly bright future of neutrinos may blind us to the realities of dark matter.

Read more: