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We propose a laser-driven near-solid density nano-structured micro-reactor concept operating with mixed nuclear fusion fuels. The micro-reactor is capable of making use of a range of neutronic and aneutronic fuels. Its core parts consists…

Plasma Physics · Physics 2022-04-26 Hartmut Ruhl , Georg Korn

A natural nuclear fission reactor with a power output of 3- 10 terawatt at the center of the earth has been proposed as the energy source of the earth's magnetic field. The proposal can be directly tested by a massive liquid scintillation…

High Energy Physics - Experiment · Physics 2007-05-23 R. S. Raghavan

Long-term neutrino-radiation hydrodynamics simulations in full general relativity are performed for the collapse of rotating massive stars that are evolved from He-stars with their initial mass of $20$ and $32M_\odot$. It is shown that if…

High Energy Astrophysical Phenomena · Physics 2021-10-04 Sho Fujibayashi , Koh Takahashi , Yuichiro Sekiguchi , Masaru Shibata

A model is proposed for the origin of cosmic rays (CRs) from ~10^14 eV to the highest energies, >10^20 eV. Gamma-Ray Bursts (GRBs) are assumed to inject CR protons and ions into the interstellar medium of star-forming galaxies--including…

Astrophysics · Physics 2008-11-26 Stuart D. Wick , Charles D. Dermer , Armen Atoyan

We investigate neutrino-driven convection in core collapse supernovae and its ramifications for the explosion mechanism, for a 15 solar mass model. Our two-dimensional simulation begins at 12 ms after bounce and proceeds for 500 ms. We…

Simple arguments concerning power and acceleration efficiency show that ultra-high energy cosmic rays (UHECRS) with energies >~ 10^{19} eV could originate from GRBs. Neutrons formed through photo-pion production processes in GRB blast waves…

Astrophysics · Physics 2009-11-06 C. D. Dermer

The core collapse of massive, rapidly-rotating stars are thought to be the progenitors of long-duration gamma-ray bursts (GRB) and their associated hyper-energetic supernovae (SNe). At early times after the collapse, relatively low angular…

Solar and Stellar Astrophysics · Physics 2020-10-07 Yossef Zenati , Daniel M. Siegel , Brian D. Metzger , Hagai B. Perets

The hypothesis that ultra-high energy (>~ 10^19 eV) cosmic rays (UHECRs) are accelerated by gamma-ray burst (GRB) blast waves is assumed to be correct. Implications of this assumption are then derived for the external shock model of…

Astrophysics · Physics 2009-10-31 Charles D. Dermer

(shortened) We perform 3D hydrodynamic simulations of gas flowing around a planetary core of mass \mplan=10\me embedded in a near Keplerian background flow, using a modified shearing box approximation. We employ a nested grid hydrodynamic…

Earth and Planetary Astrophysics · Physics 2015-01-13 Andrew F. Nelson , Maximilian Ruffert

High-energy heavy-ion particle accelerators have long served as proxies for the harsh space radiation environment, enabling both fundamental life-science research and applied testing of flight hardware. Traditionally, monoenergetic…

Space Physics · Physics 2026-02-05 Luca Lunati , Enrico Pierobon , Uli Weber , Tim Wagner , Tabea Pfuhl , Marco Durante , Christoph Schuy

Excluding speculations about future breakthrough discoveries in physics, it is shown that with what is at present known, and also what is technically feasible, manned space flight to the limits of the solar system and beyond deep into the…

Plasma Physics · Physics 2009-06-04 Dr. Friedwardt Winterberg

One consequence of the application of superconductivity to accelerator construction is that the power consumption of accelerators will become much smaller. This raises the old possibility of using high energy protons to make neutrons which…

Accelerator Physics · Physics 2010-08-02 R. R. Wilson

Active Galactic Nuclei (AGNs) and their relativistic jets belong to the most promising class of ultra-high-energy cosmic ray (UHECR) accelerators. This compact review summarises basic experimental findings by recent instruments, and…

High Energy Astrophysical Phenomena · Physics 2022-11-23 Frank M. Rieger

Large-payload deep space missions are impractical with current rocket propulsion technologies in use. Chemical thrusters yield a high thrust but low efficiency while ion thrusters are efficient but provide too little thrust for large…

Plasma Physics · Physics 2022-11-18 Ishaan Mishra

Core-collapse supernovae are, despite their spectacular visual display, neutrino events. Virtually all of the 10^53 ergs of gravitational binding energy released in the formation of the nascent neutron star is carried away in the form of…

Astrophysics · Physics 2009-09-25 O. E. B. Messer , A. Mezzacappa , S. W. Bruenn , M. W. Guidry

Ultra-cold neutrons (UCN), neutrons with energies low enough to be confined by the Fermi potential in material bottles, are playing an increasing role in measurements of fundamental properties of the neutron. The ability to manipulate UCN…

The theory of diffusive particle acceleration explains the spectral properties of the cosmic rays below energies of approx. 10^6 GeV as produced at strong shocks in supernova remnants (SNR's). To supply the observed flux of cosmic rays, a…

Astrophysics · Physics 2007-05-23 U. D. J. Gieseler , T. W. Jones , Hyesung Kang

The author applies, develops and researches mini-sized Micro- AB Thermonuclear Reactors for space propulsion and space power systems. These small engines directly convert the high speed charged particles produced in the thermonuclear…

General Physics · Physics 2007-05-23 Alexander Bolonkin

Three-dimensional (3D) simulations in recent years have shown severe difficulties producing 10^51 erg explosions of massive stars with neutrino based mechanisms while on the other hand demonstrated the large potential of mechanical effects,…

Solar and Stellar Astrophysics · Physics 2015-06-18 Oded Papish , Jason Nordhaus , Noam Soker

This research is to determine at Earth the high-energy neutrino flux coming from the galactic core, and from the many other accretion disks within the galactic core. It is estimated there are 10,000 such accretion disk within the cubic…

High Energy Astrophysical Phenomena · Physics 2023-08-01 Ayshea Bains , Trent English , Nickolas Solomey