Matter - Antimatter Split Hints at Physics
نویسنده
چکیده
Nature may have handed scientists a new clue in a longstanding mystery: how matter beat out antimatter for dominance of the universe. Early data from twin experiments at the Tevatron, the world's reigning particle accelerator at Fermi National Accelerator Laboratory (Fermilab) in Batavia, Ill., suggest an unexpected chink in the hugely successful standard model of particle physics. The twist comes from odd behavior in a particle called the B S (pronounced "B-sub-S"), which flips back and forth between its matter and antimatter forms three trillions times per second. Researchers believe that such a breakdown, known as CP violation, is required to explain why matter is so abundant. Researchers say the finding is well worth following up to make sure it is not a random clump in the data, as frequently happens in particle physics experiments. "This is exciting, definitely," says physicist Jacobo Konigsberg of the University of Florida in Gainesville, cospokesperson for CDF, one of two detectors that may have glimpsed the effect. Antimatter is well-known to science fiction fans as the stuff that explodes on contact with regular particles such as protons and electrons, which have the same mass as their antiparticles but the opposite charge. The hot, early universe contained equal parts matter and antimatter. Yet somehow, as the cosmos cooled, matter was not completely annihilated. Researchers strongly suspect that the key to this riddle lies in the weak nuclear force, which governs radioactive decay, along with more exotic reactions created in particle accelerators. In nearly all cases, matter obeys something called CP symmetry, which states that a particle ought to behave identically to the mirror image of its antiparticle. Not so when acted on by the weak nuclear force.
منابع مشابه
Neutralino Dark Matter Detection in Split Supersymmetry Scenarios
We study the phenomenology of neutralino dark matter within generic supersymmetric scenarios where the Gaugino and Higgsino masses are much lighter than the scalar soft breaking masses (Split Supersymmetry). We consider a low-energy model-independent approach and show that the guidelines in the definition of this general framework come from cosmology, which forces the lightest neutralino to hav...
متن کاملPrimordial Antimatter in the Contemporary Universe
In some baryogenesis scenarios, the universe acquires a non-vanishing average baryonic charge, but the baryon to photon ratio is not spatially constant and can be even negative in some space regions. This allows for existence of lumps of antimatter in our neighborhood and the possibility that very compact antimatter objects make a part of cosmological dark matter. Here I discuss the peculiar si...
متن کاملSeeable Matter; Unseeable Antimatter
The universe we see gives every sign of being composed of matter. This is considered a major unsolved problem in theoretical physics. Using the mathematical modeling based on the algebra T := C ⊗ H ⊗ O, an interpretation is developed that suggests that this seeable universe is not the whole universe; there is an unseeable part of the universe composed of antimatter galaxies and stuff, and an ex...
متن کاملA Classical Isodual Theory of Antimatter
An inspection of the contemporary physics literature reveals that, while matter is treated at all levels of study, from Newtonian mechanics to quantum field theory, antimatter is solely treated at the level of second quantization. For the purpose of initiating the restoration of full equivalence in the treatments of matter and antimatter in due time, in this paper we present a classical represe...
متن کاملThe Alpha Magnetic Spectrometer (AMS): search for antimatter and dark matter on the International Space Station
The disappearance of cosmological antimatter and the pervasive presence of dark matter are two of the greatest puzzles in the current understanding of the universe. The Big Bang model assumes that, at its very beginning, half of the universe was made out of antimatter. The validity of this model is based on three key experimental observations: the recession of galaxies (Hubble expansion), the h...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008