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200 papers

If gamma-ray bursts have a cosmological origin, the sources are expected to trace the large-scale structure of luminous matter in the universe. I use a new likelihood method that compares the counts-in-cells distribution of gamma-ray bursts…

Astrophysics · Physics 2007-05-23 Jean M. Quashnock

The bolometric radiation from a central body is potentially a powerful driver of atmospheric escape from planets or satellites. When heated above their equilibrium temperatures those satellites, due to their low surface gravity, are be…

Earth and Planetary Astrophysics · Physics 2025-03-25 Matthäus Schulik , James E. Owen , Richard A. Booth , Shun Fai Ling , Shun Ping Wong

We present a new calculation of neutrino emissivities and energy spectra from a massive star going through the advanced stages of nuclear burning (presupernova) in the months before becoming a supernova. The contributions from beta decay…

Solar and Stellar Astrophysics · Physics 2023-03-15 Kelly M. Patton , Cecilia Lunardini , Robert J. Farmer

Small asteroids intersecting Earth's orbit can deliver extraterrestrial rocks to the Earth, called meteorites. This process is accompanied by a luminous phenomena in the atmosphere, called bolides or fireballs. Observations of bolides…

Earth and Planetary Astrophysics · Physics 2016-08-31 Jiří Borovička , Pavel Spurný , Peter Brown

As of today, there is no official definition of a meteor cluster. It is usually identified as a large number of meteors sharing a similar radiant and velocity, all occurring within a few seconds. Only eight clusters have been reported so…

Earth and Planetary Astrophysics · Physics 2025-04-08 A. Ashimbekova , J. Vaubaillon , P. Koten

Young and forming planetesimals experience impacts from particles present in a protostellar disk. Using crater scaling laws, we integrate ejecta distributions for oblique impacts. For impacts at 10 to 65 m/s, expected for impacts associated…

Earth and Planetary Astrophysics · Physics 2025-07-11 Stephen Li , Maggie Ju , A. C. Quillen , Adam E. Rubinstein

Many experiments have been carried out to study the beta-decay rates of a variety of nuclides, and many - but not all - of these experiments yield evidence of variability of these rates. While there is as yet no accepted theory to explain…

Nuclear Experiment · Physics 2015-10-22 P. A. Sturrock , E. Fischbach , A. Parkhomov , J. D. Scargle , G. Steinitz

We calculate the X-ray emission from both constant and time evolving shocked fast winds blown by the central stars of planetary nebulae (PNs) and compare with observations. Using spherically symmetric numerical simulations with radiative…

Astrophysics · Physics 2008-11-26 Muhammad Akashi , Noam Soker , Ehud Behar , John Blondin

The dearth of planets with sizes around 1.8 $\mathrm{R_\oplus}$ is a key demographic feature discovered by the $Kepler$ mission. Two theories have emerged as potential explanations for this valley: photoevaporation and core-powered…

Earth and Planetary Astrophysics · Physics 2023-02-02 Travis A. Berger , Joshua E. Schlieder , Daniel Huber , Thomas Barclay

Beta-delayed proton emission in the lower half of the sd-shell will involve deformed nuclei. We derive the normalized matrix element connecting emission of one particle from an initial rotational nuclear state to another final rotating…

Nuclear Theory · Physics 2025-01-22 K. Riisager , E. A. M. Jensen , A. S. Jensen

We re-examine solar emission of hidden photons gamma' (mass m) caused by kinetic mixing. We calculate the emission rate with thermal field theory methods and with a kinetic equation that includes "flavor oscillations" and photon absorption…

High Energy Physics - Phenomenology · Physics 2015-02-02 Javier Redondo , Georg Raffelt

We characterize the performance of a fixed grid of solar panels on the basis of data taken under clear sky conditions over 12 months. We confirm that the power output is linearly proportional to cos(theta), where theta is the angular…

Instrumentation and Methods for Astrophysics · Physics 2022-06-09 Kevin Krisciunas

Planetesimals are born fragile and are subject to destruction by wind erosion as they move through the gas of a protoplanetary disk. In microgravity experiments, we determined the shear stress necessary for erosion of a surface consisting…

Earth and Planetary Astrophysics · Physics 2023-05-08 Laurent Schönau , Jens Teiser , Tunahan Demirci , Kolja Joeris , Tetyana Bila , F. Chioma Onyeagusi , Miriam Fritscher , Gerhard Wurm

The $^{14}$C production of shock-accelerated particles is calculated in terms of the total energy released in energetic particles. The recently reported 1.2% jump in the $^{14}$C content of the atmosphere in the year C.E. 775, it is found,…

Earth and Planetary Astrophysics · Physics 2015-06-12 David Eichler , David Mordecai

We phenomenologically put local constraints on the rotation of distant masses by using the planets of the solar system. First, we analytically compute the orbital secular precessions induced on the motion of a test particle about a massive…

General Relativity and Quantum Cosmology · Physics 2011-03-28 Lorenzo Iorio

A failed core-collapse supernova from a non-rotating progenitor can eject mass due to a weakening of gravity associated to neutrino emission by the protoneutron star. This mechanism yields observable transients and sets an upper limit to…

High Energy Astrophysical Phenomena · Physics 2021-04-14 Mario Ivanov , Rodrigo Fernández

We describe a new version (numbered 3.1) of NASA's Meteoroid Engineering Model (MEM) in which we extend the model to handle locations that lie more than a few degrees in latitude off the ecliptic plane. We provide our algorithms for…

Earth and Planetary Astrophysics · Physics 2025-12-11 Althea V. Moorhead , Petr Pokorný , Marcus A. Holden , William Kosmann

Nuclear $\beta$ decay is a key element of the astrophysical rapid neutron capture process ($r$-process). In this paper, we present state-of-the-art global $\beta$-decay calculations based on the quantified relativistic nuclear energy…

Nuclear Theory · Physics 2025-11-20 A. Ravlić , Y. Saito , W. Nazarewicz

We discuss several constraints on the properties of gamma-ray bursts (GRB) at cosmological distances. First we use the requirement that burst sources must be optically thin to pair production by photon-photon collisions in order to produce…

Astrophysics · Physics 2009-10-28 Eric Woods , Abraham Loeb

Protoplanetary disks fragment due to gravitational instability when there is enough mass for self-gravitation, described by the Toomre parameter, and when heat can be lost at a rate comparable to the local dynamical timescale, described by…

Earth and Planetary Astrophysics · Physics 2015-12-08 Hans Baehr , Hubert Klahr