This Document contains basic knowledge about Newtons Laws Of Motion with its application in real world.
It Also contains some of the examples and its working.
This Document contains basic knowledge about Newtons Laws Of Motion with its application in real world.
It Also contains some of the examples and its working.
Friction is a force that slows down moving objects or prevents stationary objects from moving .
Friction is a contact force .
Friction produces heat .
For example – A matchstick
Friction opposes the motion of an object
When one surface moves over another , these grooves and ridges get caught up with each other and slow down the motion . This causes friction .
Slides for teaching the factors affecting the magnitude of friction force, and how to calculate this for static and kinetic friction on horizontal surfaces and inclined planes.
Coaching Sprint Mechanics. What to look for. What to say. Mike Young
This is Dr. Mike Young's presentation from the 2014 Midwest Speed Summit. Dr. Young is the owner and Director of Performance at Athletic Lab sports performance training center and has coached multiple national champions in Track & Field along with working with some of the fastest athletes in soccer, football and baseball. This presentation focuses on applied sprinting mechanics and how coaches can best make technical changes. The presentation uses biomechanics and motor learning concepts and relates them to coaching the sprints.
Friction is a force that slows down moving objects or prevents stationary objects from moving .
Friction is a contact force .
Friction produces heat .
For example – A matchstick
Friction opposes the motion of an object
When one surface moves over another , these grooves and ridges get caught up with each other and slow down the motion . This causes friction .
Slides for teaching the factors affecting the magnitude of friction force, and how to calculate this for static and kinetic friction on horizontal surfaces and inclined planes.
Coaching Sprint Mechanics. What to look for. What to say. Mike Young
This is Dr. Mike Young's presentation from the 2014 Midwest Speed Summit. Dr. Young is the owner and Director of Performance at Athletic Lab sports performance training center and has coached multiple national champions in Track & Field along with working with some of the fastest athletes in soccer, football and baseball. This presentation focuses on applied sprinting mechanics and how coaches can best make technical changes. The presentation uses biomechanics and motor learning concepts and relates them to coaching the sprints.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
3. • Round! And remain round!
• Bouncy
But not too much!
• Water Proof
• Swift Through the Air
…Aaaand here comes the physics!
4. • Weight Acts downwards always
Depends on how heavy the ball is
• Magnus Force The direction depends on the motion of ball
Depends on the spin on the ball
Force is perpendicular
to both spin and velocity
Simple application of
Bernoulli’s principle
Higher
Pressure
Lower
Pressure
5. • Question: Is it always true that the harder you kick the ball, the faster it goes?
NO!
• A new force enters the scene: the Drag Force!
• Rule of thumb:
The greater the
turbulence, the
greater drag force!
• Drag Force is proportional to square of velocity. Faster the ball, greater the drag
• Surprise! Drag suddenly decreases as the separation points coincide!
(Image courtesy:
Ken Bray article –
A Fly Walks Around A Football)
6. A Rougher Ball is better than a Smooth One
• Drag Coefficient = Measure of how much drag there is
• Drag Coefficient falls sooner for a rougher ball than a smooth one
• Drag Crisis: The fall is rapid!
Which is a better football? A Smooth One or a Rough One?
The rougher ball moves
more smoothly than a
smooth one!!
Drag crisis
(Graph courtesy:
A Fly Walks Around A Football and
Journal fo Fluid Mechanics)
7. Taking a free-kick =
Aiming for a letterbox slit!
• Weight, spin and drag affect ball trajectory
• A free kick is not as easy as it seems!
• Smooth is not always desirable
10. • Rigidity of the stem and flexibility of the head increased
• Increase in the area of the head
• Greater adjustability of the tension in the strings
Wooden Aluminium Graphite
12. Impact! Translation Rotation Final movement= + =
If the ball is hit just right, there will be no impact on the grip
Standard Physics: Every movement can be broken down to a translation and a rotation
Vcm = V Vb = ω b Sweet spot:Vcm = VbBam!
13. • The racquet also vibrates!
Impact Vibration
• Third type of motion
• Gives rise to two sweet spots
• Can’t have both
14. Making the case for the central sweet spot even better!
Hit the ball right from the middle of the racquet!
Hold racquet at the proper grip position
15.
16. Sources:
http://sport.maths.org/content/
Articles on football flight by Ken Bray
Physics of racket-ball interaction – by H.Brody, University of Pennsylvania
Sweet spots of rackets – Hesston College article
Big Thanks to my friends – too many to name and they know!
Thanks to Arnab Sir and Kulkarni Sir