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Increasing the life of ultracold molecules

17.08.2021

The study of molecules cooled to very low temperatures is important for the development of quantum simulations, precision measurements, ultracold chemistry, and more. To do this, physicists need to learn how to cool them, collect and hold them, and also protect them from destruction. The latter factor significantly limits the range of experiments and phenomena that scientists could investigate in such systems.

The main channel for the decay of ultracold molecules is their inelastic collisions with each other. To avoid them, scientists use screening, that is, the creation of additional repulsion between molecules at distances at which inelastic interaction processes begin. To date, shielding of atoms and molecules has already been implemented by many different methods. For example, scientists have learned how to protect ultracold KRb molecules from each other using constant electric fields. Despite the progress made, physicists are constantly looking for new regimes that would increase the lifetime of such molecules.

Researchers from Korea and the US, with the participation of Tijs Karman from the University of Cambridge, used microwave radiation to shield two CaF molecules held by optical tweezers from each other. They showed that by controlling the parameters of the external fields, it is possible to switch molecules between the screening and anti-screening modes, changing their lifetime by a factor of 24.

The idea of ​​such screening is based on the concept of "dressed" states. If a two-level system is irradiated ("clothed") with a resonant alternating field, then the population of its states will oscillate with the Rabi frequency. By controlling the field parameters, it is possible to ensure that between molecules in "dressed" states, a strong long-range dipole-dipole interaction arises, which can be both attractive and repulsive. The latter depends, among other things, on which states are "dressed" by the field.

To implement this principle, the authors preliminarily prepared two CaF molecules, each caught in its own trap of optical tweezers, by applying a magnetic field of 27 gauss. After that, physicists for some time pushed them together in the presence of a microwave field, carried them in different directions and, using the lambda imaging method, looked at whether they fell apart or not. Thus, the scientists were able to plot the proportion of "surviving" molecules depending on the time of interaction. By changing the configuration of "dressed" states, the authors could influence this number by comparing it with the number of "naked" molecules that were not exposed to microwaves.

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About the planets of a star will tell its photosphere 05.03.2012

An international group of scientists came to the conclusion that the study of the composition of the photosphere of a star allows us to find out how its planets were formed, and what environmental conditions developed on them.

The new study is important for modeling the formation of planets, as well as determining the composition of their atmospheres and climatic conditions. Theoretical studies show that C/O (carbon/oxygen) and Mg/Si (magnesium/silicon) are the most important ratios of chemical elements in determining the mineralogy of terrestrial planets. The C/O ratio controls the distribution of silicon among carbides and oxides, while Mg/Si gives information about silicates.

In 2010, scientists ran simulations of planet formation that took the chemical composition of the protoplanetary cloud as an input. It has been found that the terrestrial planets can have very different chemical compositions and be very different from the Earth. The scientists then conducted the first detailed study of the abundances of C, O, Mg and Si in 61 stars with discovered planets and in 270 stars where no planets were found (using HARPS GTO data). As a result, it turned out that the ratios of the elements differ from the ratios that we observe on the Sun. Thus, there is a wide variety of planetary systems that are very different from our solar system.

Many stars have an Mg/Si ratio of less than 1, so their planets have an abundance of silicon, which forms compounds like MgSiO3 (magnesium silicate). This may have important implications for planetary processes such as plate tectonics, atmospheric composition and volcanism, i.e. ultimately influence the possibility of the origin of life.
Thus, there may be billions of terrestrial planets in the Universe, but the vast majority of them may have completely different internal and atmospheric features that we on Earth can hardly even imagine.

As an example, the researchers cite the 55Cnc planetary system, where it is possible with a high degree of probability to predict a decrease in the amount of aluminum and calcium as the planets move away from the central star. On the other hand, the inner terrestrial planets (within 0,5 AU of the star) contain significant amounts of refractory elements such as aluminum and calcium (about 47% of the planetary mass).

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