Cosmic-Ray Positrons: Are There Primary Sources?

Cosmic rays at the Earth include a secondary component originating in collisions of primary particles with the diffuse interstellar gas. The secondary cosmic rays are relatively rare but carry important information on the Galactic propagation of the primary particles. The secondary component includes a small fraction of antimatter particles, positrons and antiprotons. In addition, positrons and antiprotons may also come from unusual sources and possibly provide insight into new physics. For instance, the annihilation of heavy supersymmetric dark matter particles within the Galactic halo could lead to positrons or antiprotons with distinctive energy signatures. With the High-Energy Antimatter Telescope (HEAT) balloon-borne instrument, we have measured the abundances of positrons and electrons at energies between 1 and 50 GeV. The data suggest that indeed a small additional antimatter component may be present that cannot be explained by a purely secondary production mechanism. Here we describe the signature of the effect and discuss its possible origin.Comment: 15 pages, Latex, epsfig and aasms4 macros required, to appear in Astroparticle Physics (1999

Reprogramming the assembly of unmodified DNA with a small molecule

The ability of DNA to store and encode information arises from base pairing of the four-letter nucleobase code to form a double helix. Expanding this DNA ‘alphabet’ by synthetic incorporation of new bases can introduce new functionalities and enable the formation of novel nucleic acid structures. However, reprogramming the self-assembly of existing nucleobases presents an alternative route to expand the structural space and functionality of nucleic acids. Here we report the discovery that a small molecule, cyanuric acid, with three thymine-like faces reprogrammes the assembly of unmodified poly(adenine) (poly(A)) into stable, long and abundant fibres with a unique internal structure. Poly(A) DNA, RNA and peptide nucleic acid all form these assemblies. Our studies are consistent with the association of adenine and cyanuric acid units into a hexameric rosette, which brings together poly(A) triplexes with a subsequent cooperative polymerization. Fundamentally, this study shows that small hydrogen-bonding molecules can be used to induce the assembly of nucleic acids in water, which leads to new structures from inexpensive and readily available materials

DNA Replication across α-l-(3-2)-Threofuranosyl Nucleotides Mediated by Human DNA Polymerase η.

α-l-(3-2)-Threofuranosyl nucleic acid (TNA) pairs with itself, cross-pairs with DNA and RNA, and shows promise as a tool in synthetic genetics, diagnostics, and oligonucleotide therapeutics. We studied in vitro primer insertion and extension reactions catalyzed by human trans-lesion synthesis (TLS) DNA polymerase η (hPol η) opposite a TNA-modified template strand without and in combination with O4-alkyl thymine lesions. Across TNA-T (tT), hPol η inserted mostly dAMP and dGMP, dTMP and dCMP with lower efficiencies, followed by extension of the primer to a full-length product. hPol η inserted dAMP opposite O4-methyl and -ethyl analogs of tT, albeit with reduced efficiencies relative to tT. Crystal structures of ternary hPol η complexes with template tT and O4-methyl tT at the insertion and extension stages demonstrated that the shorter backbone and different connectivity of TNA compared to DNA (3 → 2 versus 5 → 3, respectively) result in local differences in sugar orientations, adjacent phosphate spacings, and directions of glycosidic bonds. The 3-OH of the primers terminal thymine was positioned at 3.4 Å on average from the α-phosphate of the incoming dNTP, consistent with insertion opposite and extension past the TNA residue by hPol η. Conversely, the crystal structure of a ternary hPol η·DNA·tTTP complex revealed that the primers terminal 3-OH was too distant from the tTTP α-phosphate, consistent with the inability of the polymerase to incorporate TNA. Overall, our study provides a better understanding of the tolerance of a TLS DNA polymerase vis-à-vis unnatural nucleotides in the template and as the incoming nucleoside triphosphate

Cosmic ray electrons and positrons from 4.5 to 100 GeV.

The HEAT (High Energy Antimatter Telescope) balloon borne cosmic ray experiment is described. The design, construction, flight and data analysis are discussed. The positron fraction (e\rm\sp+/(e\sp+ +e\sp-) and the fluxes of electrons and positrons from 4.5 to 50 GeV and the flux of all electrons (electrons and positrons) from 4.5 to 100 GeV are presented. The positron fraction results do not confirm the previously observed rise. There is evidence for a statistically significant excess of positrons in the energy region of 7 GeV to 20 GeV. This excess is analyzed in the context of a Big Bang relic supersymmetric weakly interacting particle. The fluxes are found to be intermediate to previously reported measurements. The shape of all electron the spectrum is analyzed in the context of the Leaky Box cosmic ray propagation model.Ph.D.AstronomyPure SciencesUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://deepblue.lib.umich.edu/bitstream/2027.42/130441/2/9732051.pd

Beyond guanine quartets: cation-induced formation of homogenous and chimeric DNA tetraplexes incorporating iso-guanine and guanine

AbstractBackground:iso-Guanine (iso-G) is the purine component of an isomeric Watson-Crick base pair that may have existed prebiotically. By comparing the abiotic molecular recognition properties of iso-G and its complement, iso-cytosine (iso-C), with those of genomic nucleotide bases, it may be possible to explain the exclusion of the iso-G-iso-C base pair from modern genomes. Whether a nucleobase forms quartets may have a key role in determining its functionality. Biotically, nucleic acid tetraplexes have been implicated in cellular functions; prebiotically, tetraplexes would probably interfere with replication. Recently, in vitro selection has yielded receptors and catalysts that incorporate G quartets. The versatility of these structures could be enhanced by expanding the range of bases that can form the quartet motif.Results: Native polyacrylamide gel electrophoresis of oligonucleotides bearing runs of iso-G provides strong support for tetraplex formation via cation-promoted DNA strand association. In particular, when strands of different lengths bearing the same iso-G tetrad recognition element were combined, five bands were observed after electrophoresis, corresponding to all possible heterotetraplexes with parallel strand alignment. An analogous experiment with a mixture of strands bearing iso-G or G tetrad recognition domains supports the existence of mixed iso-G/G tetraplexes with antiparallel strand alignment at chimeric junctions. iso-G tetraplex and quartet structure has also been probed by a photo-crosslinking experiment, ultra-violet spectroscopy and theoretical calculations.Conclusions: As iso-G and G both have a marked tendency to form tetraplexes, their tandem inclusion in genetic material may be problematic, leading to double-stranded DNA half composed of bases that have a tendency to auto-associate. The resulting density of ‘selfish’ bases could undermine Watson-Crick pair formation, especially in a prebiotic context devoid of enzymes. Nevertheless, the ability of iso-G to form mixed quartets with G may provide a basis for altering the properties of tetraplexes in the domain of artificial receptors or catalysts from in vitro selections