Add to ORKGSearch and identification of superheavy elements (SHE) of Z≥110 in a nature were carried out till now by registration in olivine from pallasites of super-long tracks- traces of braking of high-energy SHE nuclei formed a part of the galactic cosmic rays (GCR) [1-3]. For removal of a background from high track density due to iron nuclei (VH – group) before chemical etching the olivine crystals wer
The origin of galactic cosmic rays (GCRs) nuclei is still unknown. Precise observation of ultra heav...
Cosmic-ray-produced (cosmogenic) nuclides were studied in fragments of the Brenham pallasite, a larg...
We analyzed cosmogenic nuclides in metal and/or silicate (primarily olivine) separated from the main...
The main goal of the present work is the search for and identification of relatively stable nuclei o...
New approaches for investigation of relatively stable nuclei of super heavy element (SHE) (Z > 110) ...
The aim of the OLIMPIYA experiment is to search for and identify traces of heavy and superheavy nucl...
Abstract: An original method of studying chemically etched tracks of heavy nuclei in olivine from pa...
Investigations of recordable lengths (maximum etchable lengths) of fossil tracks in meteorites and i...
A one-step, three-component aqueous etchant was developed for revealing the tracks of charged partic...
Experiments were carried out on tracks of high energy U ions in olivine, a common meteoritic mineral...
The origin of the elements from Cu to As in the UH (ultra-heavy) cosmic rays is investigated and rel...
Superheavy elements have been searched for by neutron induced fission of mass separated samples. Var...
Fossil track studies in several meteorites and in lunar dust show that super-heavy (Z > 110) transur...
Observations of ultra-heavy (Z≥30) galactic cosmic rays (GCR) help to distinguish possible origins ...
There are many indications for the existence of superheavy elements (SHE) in the Earth's crust. The ...
The origin of galactic cosmic rays (GCRs) nuclei is still unknown. Precise observation of ultra heav...
Cosmic-ray-produced (cosmogenic) nuclides were studied in fragments of the Brenham pallasite, a larg...
We analyzed cosmogenic nuclides in metal and/or silicate (primarily olivine) separated from the main...
The main goal of the present work is the search for and identification of relatively stable nuclei o...
New approaches for investigation of relatively stable nuclei of super heavy element (SHE) (Z > 110) ...
The aim of the OLIMPIYA experiment is to search for and identify traces of heavy and superheavy nucl...
Abstract: An original method of studying chemically etched tracks of heavy nuclei in olivine from pa...
Investigations of recordable lengths (maximum etchable lengths) of fossil tracks in meteorites and i...
A one-step, three-component aqueous etchant was developed for revealing the tracks of charged partic...
Experiments were carried out on tracks of high energy U ions in olivine, a common meteoritic mineral...
The origin of the elements from Cu to As in the UH (ultra-heavy) cosmic rays is investigated and rel...
Superheavy elements have been searched for by neutron induced fission of mass separated samples. Var...
Fossil track studies in several meteorites and in lunar dust show that super-heavy (Z > 110) transur...
Observations of ultra-heavy (Z≥30) galactic cosmic rays (GCR) help to distinguish possible origins ...
There are many indications for the existence of superheavy elements (SHE) in the Earth's crust. The ...
The origin of galactic cosmic rays (GCRs) nuclei is still unknown. Precise observation of ultra heav...
Cosmic-ray-produced (cosmogenic) nuclides were studied in fragments of the Brenham pallasite, a larg...
We analyzed cosmogenic nuclides in metal and/or silicate (primarily olivine) separated from the main...