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Hydrodynamic Lift on Boats

Boats float supported only by buoyancy at rest and at very low speeds. As the speed increases, a hull capable of planing makes a sharp transition to a lifting surface while plowing up the bow wave. As the speed increases further the boat planes, and at a high enough speed buoyancy becomes negligible; hydrodynamic lift carries the weight. More generally, any flow past a lifting surface generates a force perpendicular to the flow once the flow separates from the trailing edge without backflow (without vortex formation). Wings, hydrofoils, sails, and propellers are examples of lifting surfaces. The idea of a planing hull as lifting surface has been discussed inconclusively in the literature. We provide evidence for the onset of lift before planing and also produce an empirically correct lift coefficient for the planing of a v-bottom (prismatic shape) hull at high enough speeds that the wet surface area is confined roughly to a triangular shape near the transom. Our model follows our calculation of the lift on a fully submerged delta wing hydrofoil. The lift is reduced once the hydrofoil pierces the air-water interface.

physics.pop-ph↗

Conceptual Design of Mars Lander with Novel Impact Intriguing System

Landing robotic spacecrafts and humans on Mars has become one of the inevitable technological necessities for humans. Effectuating perfect Mars expedition requires landing of enormous cargoes, crewed modules, ascent vehicles, and scientific laboratories. Crash-landing destructs landing modules due to a lack of adequate impact absorbers. Moreover, the existence of deformable shock absorbers like Aluminium honeycomb and carbon fibers within landing gears are defeasible for large-scale mass and crewed landing. Further in the EDL scenario, switching of events within a limited span of 5 to 8 minutes appears to be the most challenging task for landers. Scrutinizing these concerns, we propose a novel impact intriguing system that will be more achievable for extensive landing missions. This paper represents the conceptual design of Mars lander and we expect that subject to any obstruction in EDL sequence, this mechanical system will endorse soft-landing in forthcoming missions. Hence our ultimate aim is to protect lander modules and their instruments over the defective landing.

physics.pop-ph↗

Snellius meets Schwarzschild - Refraction of brachistochrones and time-like geodesics

The brachistochrone problem can be solved either by variational calculus or by a skillful application of the Snellius' law of refraction. This suggests the question whether also other variational problems can be solved by an analogue of the refraction law. In this paper we investigate the physically interesting case of free fall in General Relativity that can be formulated as a variational problem w. r. t. proper time. We state and discuss the corresponding refraction law for a special class of spacetime metrics including the Schwarzschild metric.

physics.pop-ph↗

Recommendations from the Ad Hoc Committee on SETI Nomenclature

The Ad Hoc Committee on SETI Nomenclature was convened at the suggestion of Frank Drake after the Decoding Alien Intelligence Workshop at the SETI Institute in March 2018. The purpose of the committee was to recommend standardized definitions for terms, especially those that are used inconsistently in the literature and the scientific community. The committee sought to recommend definitions and terms that are a compromise among several desirable but occasionally inconsistent properties for such terms: 1) Consistency with the historical literature and common use in the field; 2) Consistency with the present literature and common use in the field; 3) Precision of meaning; 4) Consistency with the natural (i.e. everyday, non-jargon) meanings of terms; 5) Compatibility with non-English terms and definitions. The definitions in this report are restricted to technical, SETI contexts, where they may have jargon senses different from their everyday senses. In many cases we include terms only to deprecate them (in the sense of "to withdraw official support for or discourage the use of...in favor of a newer or better alternative", Merriam-Webster sense 4). This is a consensus document that the committee members all endorse; however, in many cases the individual members have (or have expressed in the past) more nuanced opinions on these terms that are not fully reflected here, for instance Almár (2008, Acta Astronautica, 68, 351), Denning (2008, NASA-SP-2009-4802 Ch. 3 pp.63-124), and Wright (2018, arXiv:1803.06972).

physics.pop-ph↗

A fast model based on muffin-tin approximation to study charge transfer effects in time-dependent quantum transport simulations: doped Si-SiO2 quantum-dot systems

In order to quickly study quantum devices in transient problems, this work demonstrates an analytical algorithm to solve the Hartree potential associated with charge fluctuations in the time-dependent non-equilibrium green function (TDNEGF) method. We implement the calculations in the heterojunction system of gold metals and silicon quantum dots for applications of photoelectric semiconductors in the future. Numerical results for the transient solutions are shown to be valid by comparing with the steady solutions calculated by the standard time-independent density functional method.

physics.pop-ph↗

Fermi and Lotka: The Long Odds of Survival in a Dangerous Universe

Fermi's Paradox is the contradiction between the fact that it would seem to be highly probable that there are other technologically advanced species beyond the Earth, and the fact that there is no generally accepted evidence for their existence. Hanson and Bostrom have proposed that there may be a Great Filter, a survival challenge so lethal that it prevents virtually all species from evolving to an advanced stage. This paper argues that the Great Filter would be not one single factor, but rather simply the statistics of survival in an always-dangerous universe. The frequency of species that survive multiple existential threats would likely obey a power law such as Lotka's Law, such that the frequency of survivors would diminish as an inverse power of the number of threats. Since any species that advances to the point at which it is detectable on an interstellar scale likely must survive a large number of existential threats, by Lotka's Law the number of such survivors would be a very small fraction of the candidate species that evolve on various planets. Some sobering implications of this picture are outlined.

physics.pop-ph↗

Algol as Horus in the Cairo Calendar: the possible means and the motives of the observations

An ancient Egyptian Calendar of Lucky and Unlucky Days, the Cairo Calendar (CC), assigns luck with the period of 2.850 days. Previous astronomical, astrophysical and statistical analyses of CC support the idea that this was the period of the eclipsing binary Algol three millennia ago. However, next to nothing is known about who recorded Algol's period into CC and especially how. Here, we show that the ancient Egyptian scribes had the possible means and the motives for such astronomical observations. Their principles of describing celestial phenomena as activity of gods reveal why Algol received the title of Horus.

physics.hist-ph↗

Passion for Gravitational Waves

This is a popular lecture about the history of gravitational wave research. Without any doubt, the discovery of gravitational waves is the most important event in the physics of the last decade along with the discovery of the Higgs boson. This landmark discovery is another confirmation of the general theory of relativity, on the basis of which Albert Einstein predicted the existence of gravitational waves in 1916. However, the history of gravitational wave research includes, besides Einstein, many other important players. The author thanks Mikhail Korobko for pointing out the inaccuracy in the first version of the manuscript and Olga Chashchina for her kind help with the text of the manuscript. Any remaining errors and inaccuracies are solely the fault of the author.

physics.pop-ph↗

Non-Hermitian Optics

Non-Hermitian optics, mostly known as 'Parity-time symmetric optics', is considered as one of the frontiers areas of research in optical sciences at present. This area is largely inspired by the so-called non-Hermitian quantum physics. While the non-Hermitian quantum mechanics is yet to be accepted widely, parity-time symmetric optics is already a craze among physicists with many experimental results and demonstrations to its support. In this article, keeping under graduate students in mind, in particular, we are giving a brief introduction to this promising area of research in physics.

physics.pop-ph↗

Remarks on the uncertainty relations

We analyze general uncertainty relations and we show that there can exist such pairs of non--commuting observables $A$ and $B$ and such vectors that the lower bound for the product of standard deviations $ΔA$ and $ΔB$ calculated for these vectors is zero: $ΔA\,\cdot\,ΔB \geq 0$. We show also that for some pairs of non--commuting observables the sets of vectors for which $ΔA\,\cdot\,ΔB \geq 0$ can be complete (total). The Heisenberg, $Δt \,\cdot\, ΔE \geq \hbar/2$, and Mandelstam--Tamm (MT), $ τ_{A}\,\cdot \,ΔE \geq \hbar/2$, time--energy uncertainty relations ($τ_{A}$ is the characteristic time for the observable $A$) are analyzed too. We show that the interpretation $τ_{A} = \infty$ for eigenvectors of a Hamiltonian $H$ does not follow from the rigorous analysis of MT relation. We show also that contrary to the position--momentum uncertainty relation, the validity of the MT relation is limited: It does not hold on complete sets of eigenvectors of $A$ and $H$.

quant-ph↗

Reexamining the Chain Fountain

We show via proof-by-construction that the chain fountain, also known as the Mould effect, is a generic consequence of energy conserving dynamics of linear chains, similar to the extra acceleration observed for hanging or falling chains. Extracting a chain from its unentangled slack sitting on a table is much less energy dissipative than the claim of the classical scenario, postulated by Biggins and Warner [Proc. R. Soc. A 470, 20130689(2014)] as the starting point of their explanation of the chain fountain. As a result, their alleged upward kicks on the chain from the table as the chain is uplifted can at best be one of the possible factors in driving the fountain, if not totally irrelevant. We construct an efficient chain fountain with no upward kicks in Biggins and Warnerś sense, rather relying on the hanging chain dynamics. Simply put, the centrifugal force at the top of the fountain is responsible for maintaining the fountain. We argue that lateral motion of the chain in the slack plays a decisive role in the Mould effect.

physics.pop-ph↗

Engaging the Public with Supernova and Supernova Remnant Research Using Virtual Reality

On 21 April 2018, the citizens of Wako, Japan, interacted in a novel way with research being carried out at the Astrophysical Big Bang Laboratory (ABBL) at RIKEN. They were able to explore a model of a supernova and its remnant in an immersive three-dimentional format by using virtual reality (VR) technology. In this article, we explain how this experience was developed and delivered to the public, providing practical tips for and reflecting on the successful organisation of an event of this kind.

astro-ph.IM↗

Creating music based on quantitative data from variable stars

In this work we show a technique that allows for the musical interpretation of the brightness variations of stars. This method allows composers a lot of freedom to incorporate their own ideas into the score, based on the melodic line generated from the quantitative data obtained from the stars. There are a wide number of possible applications for this technique, including avant-garde music creation, teaching and promotion of the association between music and science.

astro-ph.IM↗

One flight over the quantum chromodynamics. Part Two: Quantum Mechanics

This is the second of a series of popular lectures on quantum chromodynamics. The first (introductory) lecture can be found here: https://scfh.ru/blogs/O_fizike_i_fizikah/polet-nad-kvantovoy-khromodinamikoy/ The lecture deals with the one of the main pillars of quantum chromodynamics --- quantum mechanics . Non-physicists usually consider quantum mechanics as an extremely weird subject far from the everyday common sense. Partly this is true. However we will try to argue in this lecture that in its essence quantum mechanics is, in a some sense, even more natural than classical mechanics, and it is not so far from the common sense as a layman usually assumes.

physics.pop-ph↗

Diving Body Shape Coefficient Setting Based on Moment of Inertia Analysis

In the diving competition rules, FINA specifies the code of different diving movements and its difficulty coefficient. The rule simply relies on the complexity of the action to determine the difficulty. In the formulation of the diving difficulty coefficient, the athlete's body shape has not been fully considered, so it is difficult to fully guarantee the fairness of the diving competition. Based on the above problems, this paper analyzes the rules of the FINA's 10-meter platform diving difficulty coefficient, establishes the multi-rigid-body model of the human body, obtains the relationship between the moment of inertia and the completion time of the athletes to complete each diving action and the athlete's body shape, and determines the index to measure the athlete's body shape. The Lagrange Interpolation Polynomial is used to establish the functional relationship between the body shape correction coefficient and the body shape correction index, and the body shape correction coefficient corresponding to different body type athletes is determined accordingly. Finally, a new 10-meter platform diving difficulty coefficient scheme was developed.

physics.pop-ph↗

Artificial Intelligence for Interstellar Travel

The large distances involved in interstellar travel require a high degree of spacecraft autonomy, realized by artificial intelligence. The breadth of tasks artificial intelligence could perform on such spacecraft involves maintenance, data collection, designing and constructing an infrastructure using in-situ resources. Despite its importance, existing publications on artificial intelligence and interstellar travel are limited to cursory descriptions where little detail is given about the nature of the artificial intelligence. This article explores the role of artificial intelligence for interstellar travel by compiling use cases, exploring capabilities, and proposing typologies, system and mission architectures. Estimations for the required intelligence level for specific types of interstellar probes are given, along with potential system and mission architectures, covering those proposed in the literature but also presenting novel ones. Finally, a generic design for interstellar probes with an AI payload is proposed. Given current levels of increase in computational power, a spacecraft with a similar computational power as the human brain would have a mass from dozens to hundreds of tons in a 2050-2060 timeframe. Given that the advent of the first interstellar missions and artificial general intelligence are estimated to be by the mid-21st century, a more in-depth exploration of the relationship between the two should be attempted, focusing on neglected areas such as protecting the artificial intelligence payload from radiation in interstellar space and the role of artificial intelligence in self-replication.

physics.pop-ph↗

The black hole fifty years after: Genesis of the name

Black holes are extreme spacetime deformations where even light is imprisoned. There is an extensive astrophysical evidence for the real and abundant existence of these prisons of matter and light in the Universe. Mathematically, black holes are described by solutions of the field equations of the theory of general relativity, the first of which was published in 1916 by Karl Schwarzschild. Another highly relevant solution, representing a rotating black hole, was found by Roy Kerr in 1963. It was only much after the publication of the Schwarzschild solution, however, that the term black hole was employed to describe these objects. Who invented it? Conventional wisdom attributes the origin of the term to the prominent North American physicist John Wheeler who first adopted it in a general audience article published in 1968. This, however, is just one side of a story that begins two hundred years before in an Indian prison colloquially known as the Black Hole of Calcutta. Robert Dicke, also a distinguished physicist and colleague of Wheeler at Princeton University, aware of the prison's tragedy began, around 1960, to compare gravitationally completely collapsed stars to the black hole of Calcutta. The whole account thus suggests reconsidering who indeed coined the name black hole and commends acknowledging its definitive birth to a partnership between Wheeler and Dicke.

physics.hist-ph↗