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Venki Ramakrishnan’s is the real-deal ‘pivot story’ — ‘pivoting’ being quite the fancy thing to do today. Born in Chidambaram in Tamil Nadu in 1952, Venki wanted to be a physicist, and by the time he decided to do something about his passion for Biology, he was already a PhD in Physics from Ohio University, USA. He then ‘pivoted’ and studied Biology at the University of California, San Diego, before he began his post-doctoral work at Yale University.

He went on to win the Nobel Prize in Chemistry in 2009 for his work on cellular particles called ribosomes. His first book, Gene Machine, captures this journey with the kind of honesty and self-deprecation one does not expect from an award-winning scientist.

With similar candour, in his second book, he examines recent scientific breakthroughs in longevity and ageing and raises uncomfortable questions about the ethical aspects of the research as well as the biological purpose of death.

Researchers at the University of Colorado Boulder have developed experiments to replicate the chemical reactions of the Interstellar Medium, using techniques like laser cooling and mass spectrometry to observe interactions between ions and molecules.

While it may not look like it, the interstellar space between stars is far from empty. Atoms, ions, molecules, and more reside in this ethereal environment known as the Interstellar Medium (ISM). The ISM has fascinated scientists for decades, as at least 200 unique molecules form in its cold, low-pressure environment. It’s a subject that ties together the fields of chemistry, physics, and astronomy, as scientists from each field work to determine what types of chemical reactions happen there.

Now, in the recently published cover article of the Journal of Physical Chemistry A, JILA Fellow and University of Colorado Boulder Physics Professor Heather Lewandowski and former JILA graduate student Olivia Krohn highlight their work to mimic ISM conditions by using Coulomb crystals, a cold pseudo-crystalline structure, to watch ions and neutral molecules interact with each other.

In a study recently published in Nature, researchers from the Max Born Institute in Berlin, Germany, and the Max-Planck Institute of Quantum Optics in Garching have unveiled a new technique for deciphering the properties of matter with light, that can simultaneously detect and precisely quantify many substances with a high chemical selectivity.

Their technique interrogates the atoms and molecules in the ultraviolet spectral region at very feeble light levels. Using two optical frequency combs and a photon counter, the experiments open up exciting prospects for conducting dual-comb spectroscopy in low-light conditions and they pave the way for novel applications of photon-level diagnostics, such as precision spectroscopy of single atoms or molecules for fundamental tests of physics and ultraviolet photochemistry in the Earth’s atmosphere or from space telescopes.

What is the mass of a neutrino at rest? This is one of the big unanswered questions in physics. Neutrinos play a central role in nature. A team led by Klaus Blaum, Director at the Max Planck Institute for Nuclear Physics in Heidelberg, has now made an important contribution in “weighing” neutrinos as part of the international ECHo collaboration. Their findings are published in Nature Physics.

Using a Penning trap, it has measured the change in mass of a holmium-163 isotope with extreme precision when its nucleus captures an electron and turns into dysprosium-163. From this, it was able to determine the Q value 50 times more accurately than before. Using a more precise Q-value, possible systematic errors in the determination of the neutrino mass can be revealed.

In the 1930s, it turned out that neither the energy nor the momentum balance is correct in the radioactive beta decay of an atomic nucleus. This led to the postulate of “ghost particles” that “secretly” carry away energy and momentum. In 1956, experimental proof of such neutrinos was finally obtained. The challenge: neutrinos only interact with other particles of matter via the weak interaction that is also underlying the beta decay of an atomic nucleus.