Эрдэмтэд их тэсрэлтийн дараа матери антиматериас илүүтэйгээр оршин тогтнох болсон шалтгааныг хүнд нейтриногийн нөлөөгөөр тайлбарлах шинэ таамаглал дэвшүүллээ.
Физикчид их тэсрэлтийн дараа матери болон антиматери тэнцүү хэмжээгээр үүсэж, хоорондоо устгалцан энерги ялгаруулсан гэж үздэг. Хэрэв тэдгээр нь бүрэн тэнцүү байсан бол ертөнцөд од, гариг эрхэс, амьдрал үүсэх матери үлдэхгүй байх байв. Саутхэмптоны их сургууль болон Энэтхэгийн Технологийн дээд сургуулийн (IIT) Канпурын судлаачид энэхүү нууцыг тайлах гол түлхүүр нь “тусгаарлагдсан” хүнд нейтрино байж болзошгүй гэж үзжээ.
Уламжлалт нейтринотой харьцуулахад энэхүү хүнд бөөм нь бусадтай маш сул харилцан үйлчлэлцдэг тул физикчид түүнийг ач холбогдолгүй гэж үзэж ирсэн. Гэвч судалгааны багийн тооцоолсноор, уг бөөм нь асар удаан задардаг тул их тэсрэлтийн дараа ертөнц хөрөх явцад эрчим хүчний нягтралыг түр зуур давамгайлж байжээ. Энэхүү богино хугацааны давамгайлал нь матери антиматериас илүүтэйгээр үлдэх нөхцөлийг бүрдүүлсэн байж болзошгүй юм.
Судлаачдын үзэж байгаагаар, хүнд нейтрино нь Хиггсийн бозонтой холбоотой бөөмсийн харилцан үйлчлэлийн температурын нөхцөлийг өөрчилсөн байна. Энэхүү температур нь матери ба антиматерийн тэнцвэргүй байдлыг бий болгох “шилжүүлэгч”-ийн үүрэг гүйцэтгэсэн гэж доктор Ришав Рошан тайлбарлав. Уг судалгааны үр дүн “Physical Review Letters” сэтгүүлд нийтлэгджээ.
Энэхүү онол нь ертөнцийн тэлэлтийн түүхийг ойлгоход чухал ач холбогдолтой бөгөөд эртний таталцлын долгионд тодорхой ул мөр үлдээсэн байж магадгүй гэж доктор Судипта Шоу онцолсон байна. Хэрэв эдгээр долгионы гарын үсгийг ирээдүйд илрүүлж чадвал уг таамаглалыг батлах боломжтой юм. Одоогоор энэхүү тайлбар нь онолын түвшинд байгаа бөгөөд физикийн хамгийн том нууцуудын нэгийг тайлах шинэ гарц болж байна.
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Scientists have proposed a surprising new explanation for why the universe exists, and it centers on a mysterious particle that physicists have largely overlooked for decades. Their theory suggests this forgotten particle may have played a crucial role in shaping the early cosmos and allowing matter to survive after the Big Bang.
The research addresses one of the most fundamental mysteries in physics: why does the universe contain matter instead of nothing at all? Scientists believe matter and antimatter were produced in nearly equal amounts in the early universe. When these opposites encounter one another, they annihilate and release energy. If they had existed in perfectly equal quantities, virtually all matter could have disappeared, leaving no material to form stars, planets, or life.
Now, researchers from the University of Southampton and the Indian Institute of Technology Kanpur believe they may have found an important piece of the puzzle. Their explanation involves a little-understood relative of the neutrino, an extremely lightweight particle that rarely interacts with ordinary matter.
A Forgotten Particle With a Powerful Role in the Early Universe
The team focused on a type of particle known as a ‘decoupled’ heavy neutrino. Unlike ordinary neutrinos, this hypothetical heavier relative has generally been considered too weakly connected to other particles to significantly influence the universe.
However, the researchers found that its unusually long lifetime could have made it far more important than previously thought. According to their calculations, the particle may have survived long enough to temporarily dominate the universe’s energy density as the cosmos cooled after the Big Bang.
That brief period of dominance could have altered how the early universe evolved, influencing the conditions that ultimately allowed matter to outnumber antimatter.
Dr. Rishav Roshan of the University of Southampton, an author of the study, explained:
“This decoupled heavy neutrino has long been dismissed as an irrelevant background detail in particle physics.
“However, it decays incredibly slowly. As the cosmos cooled after the Big Bang, the particle lived long enough that it temporarily took over the energy density of the universe and triggered a matter-dominated period.”
The findings were published in Physical Review Letters, a scientific journal of the American Physical Society.
How a Heavy Neutrino Could Explain Why Matter Survived
Previous attempts to explain why matter prevailed over antimatter generally left out the decoupled heavy neutrino. Because it interacts so weakly with other particles, scientists assumed it would have little influence on the processes responsible for creating the imbalance.
The new research challenges that assumption. The team found that even a particle with extremely weak interactions could indirectly affect the conditions under which matter gained its crucial advantage.
This imbalance, known as matter and antimatter asymmetry, is essential to understanding our existence. For reasons physicists are still trying to explain, the early universe ended up with slightly more matter than antimatter. That small difference allowed some matter to remain after most particles and their antiparticles annihilated one another.
“The fact that we are here at all proves that an asymmetry between matter and antimatter occurred,” added Dr. Roshan.
“The decoupled neutrino shifted the temperature in the early universe at which fundamental particles – like electrons and other leptons – interacted with their anti-particles with the help of Standard Model Higgs boson.
“This temperature acts like a switch that shapes how the matter-antimatter imbalance was built up.”
The Higgs boson is a fundamental particle associated with the mechanism that gives many elementary particles their mass. In the researchers’ proposed scenario, the heavy neutrino changed the temperature conditions governing important particle interactions involving the Higgs boson.
By shifting when these interactions occurred, the particle could have influenced how the imbalance between matter and antimatter developed. In other words, something long considered insignificant may have helped determine why the universe contains matter at all.
Ancient Gravitational Waves Could Reveal the Answer
The theory could also have important implications for understanding how the universe expanded in its earliest stages.
Study co-author Dr. Sudipta Show of the Indian Institute of Technology Kanpur said the findings suggest that the forgotten particle may have dramatically altered the expansion history of the young cosmos.
He added: “It offers us a new explanation for how matter won.
“The dramatic shift in the early expansion of the cosmos leaves distinct but detectable imprints of changes, for example on primordial gravitational waves.
“These gravitational wave signatures open up new avenues for us to unravel the evolution of the early universe after the Big Bang.”
Gravitational waves are ripples in the fabric of space and time. Scientists believe processes in the extremely early universe may have generated primordial gravitational waves that carry information about conditions from that distant era.
According to the new theory, the temporary dominance of the heavy neutrino could have left recognizable signatures in those ancient signals. Detecting such patterns could eventually provide a way to investigate whether the proposed particle really influenced the universe’s earliest evolution.
For now, the explanation remains theoretical. But it offers physicists a new possibility for solving one of cosmology’s deepest mysteries: how matter survived when its encounter with antimatter could have left the universe almost entirely empty.
