Myosin-I nomenclature

We suggest that the vertebrate myosin-I field adopt a common nomenclature system based on the names adopted by the Human Genome Organization (HUGO). At present, the myosin-I nomenclature is very confusing; not only are several systems in use, but several different genes have been given the same name. Despite their faults, we believe that the names adopted by the HUGO nomenclature group for genome annotation are the best compromise, and we recommend universal adoption

A mutation associated with centronuclear myopathy enhances the size and stability of dynamin 2 complexes in cells

BACKGROUND: Dynamin 2 (Dyn2) is a ~100 kDa GTPase that assembles around the necks of nascent endocytic and Golgi vesicles and catalyzes membrane scission. Mutations in Dyn2 that cause Centronuclear Myopathy (CNM) have been shown to stabilize Dyn2 polymers against GTP-dependent disassembly in vitro. Precisely timed regulation of assembly and disassembly is believed to be critical for Dyn2 function in membrane vesiculation, and the CNM mutations interfere with this regulation by shifting the equilibrium toward the assembled state. METHODS: In this study we use two fluorescence fluctuation spectroscopy (FFS) approaches to show that a CNM mutant form of Dyn2 also has a greater propensity to self-assemble in the cytosol and on the plasma membrane of living cells. RESULTS: Results obtained using brightness analysis indicate that unassembled wild-type Dyn2 is predominantly tetrameric in the cytosol, although different oligomeric species are observed, depending on the concentration of expressed protein. In contrast, an R369W mutant identified in CNM patients forms higher-order oligomers at concentrations above 1 μM. Investigation of Dyn2-R369W by Total Internal Reflection Fluorescence (TIRF) FFS reveals that this mutant forms larger and more stable clathrin-containing structures on the plasma membrane than wild-type Dyn2. CONCLUSIONS AND GENERAL SIGNIFICANCE: These observations may explain defects in membrane trafficking reported in CNM patient cells and in heterologous systems expressing CNM-associated Dyn2 mutants

Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network

Gravitational lensing by massive objects along the line of sight to the source causes distortions of gravitational wave-signals; such distortions may reveal information about fundamental physics, cosmology and astrophysics. In this work, we have extended the search for lensing signatures to all binary black hole events from the third observing run of the LIGO--Virgo network. We search for repeated signals from strong lensing by 1) performing targeted searches for subthreshold signals, 2) calculating the degree of overlap amongst the intrinsic parameters and sky location of pairs of signals, 3) comparing the similarities of the spectrograms amongst pairs of signals, and 4) performing dual-signal Bayesian analysis that takes into account selection effects and astrophysical knowledge. We also search for distortions to the gravitational waveform caused by 1) frequency-independent phase shifts in strongly lensed images, and 2) frequency-dependent modulation of the amplitude and phase due to point masses. None of these searches yields significant evidence for lensing. Finally, we use the non-detection of gravitational-wave lensing to constrain the lensing rate based on the latest merger-rate estimates and the fraction of dark matter composed of compact objects

Search for eccentric black hole coalescences during the third observing run of LIGO and Virgo

Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass M>70 M⊙) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities 0<e≤0.3 at 0.33 Gpc−3 yr−1 at 90\% confidence level

Ultralight vector dark matter search using data from the KAGRA O3GK run

Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for U(1)B−L gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the U(1)B−L gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

Structural and Enzti1atic Studies of Dopamine-ß-Hydroxylase from Bovine Adrenal Chromaffin Granules

Dopamine-ß-hydroxylase (DßH), an enzyme which catalyzes the conversion of dopamine to norepinephrine, is the only enzyme of the catecholamine biosynthetic pathway located in the chromaffin granules of adrenal medulla. Within the granules, two populations of DßH exist: a water-soluble fraction found within the granule matrix and a membrane-bound, amphiphilic fraction embedded in the surrounding bilayer. The amphiphilic form was purified to homogeneity following its extraction from the membrane with the non-ionic detergent BRIJ 58. Three steps were required to achieve complete purification: adsorption to ConA-Sepharose, adsorption to DEAE Sephadex A-25, and chromatography on Sephacryl S-200, Sepharose 6B, or Sepharose CL-4B. The presence of 0.1-0.2 mg/ml BRIJ 58 was essential for protein recovery. The enzymatic and structural characteristics of membrane-bound DßH were found to be similar to those of soluble DßH. Initial velocity data indicated a Ping-pong or double-displacement reaction with Km for the substrates, tyramine and ascorbate, of 2.13 mM and 0.88 mM, respectively. Dicarboxylic acids activated the enzyme but halides inhibited both forms of DßH at the optimal pH range of 5.0-5.5. The chromatographic elution profiles, fluorescence and circular dichroism spectra, and migration on sucrose density gradients were indistinguishable for the two forms of the enzyme. Although not identical, the amino acid compositions of the two forms also displayed considerable similarity. As determined by sedimentation equilibrium, molecular weight values of 295,000 ± 15,000 were obtained for both forms of DßH. Despite these similarities, membrane-bound DßH possesses amphiphilic properties lacking in the soluble form. Whereas purified amphiphilic DßH may be incorporated into egg phosphatidylcholine vesicles with a 75% efficiency, the soluble form does not interact with vesicles

Membrane fusion: stalk model revisited.

Membrane fusion is believed to proceed via intermediate structures called stalks. Mathematical analysis of the stalk provided the elastic energy involved in this structure and predicted the possible evolution of the overall process, but the energies predicted by the original model were suspiciously high. This was due to an erroneous assumption, i.e., that the stalk has a figure of revolution of a circular arc. Here we abandon this assumption and calculate the correct shape of the stalk. We find that it can be made completely stress free and, hence, its energy, instead of being positive and high can become negative, thus facilitating the fusion process. Based on our new calculations, the energies of hemifusion, of complete fusion, and of the pore in a bilayer were analyzed. Implications for membrane fusion and lipid phase transitions are discussed