The age of the universe can be estimated in three ways: the age of chemical elements, the age of oldest star clusters, and the age of oldest white dwarf stars. Measurements from the Hubble Space Telescope and Wilkinson Microwave Anisotropy Probe have estimated the age of the universe to be approximately 13.8 billion years. However, this estimation depends on the underlying cosmological model being correct. The discovery of dark energy in 1998 revealed that the expansion of the universe is accelerating, contrary to expectations, and dark energy remains one of the greatest unsolved mysteries in physics today.
Contents
The Big Bang Theory
The Big Bang Phase
Expanding Universe
Testing Big Bang Model
Dark matter & Dark energy
Evidence of dark matter
After time period of Big Bang
Life cycle of star
Contents
The Big Bang Theory
The Big Bang Phase
Expanding Universe
Testing Big Bang Model
Dark matter & Dark energy
Evidence of dark matter
After time period of Big Bang
Life cycle of star
The universe began about 14.4 billion years ago.
The Big Bang Theory states that, in the beginning, the universe was all in one place.
To know more, see the presentation.
How the concept was introduced by the astrophycists and examples that provide the base for the existence of dark matter. Basic introduction to types of dark matter according to standard cosmological theory.
The universe began about 14.4 billion years ago.
The Big Bang Theory states that, in the beginning, the universe was all in one place.
To know more, see the presentation.
How the concept was introduced by the astrophycists and examples that provide the base for the existence of dark matter. Basic introduction to types of dark matter according to standard cosmological theory.
This article seeks to present the future of the Universe, as well as to point out the measures that lead to the survival of humanity in the face of the numerous threats that may occur at the level of the solar system and the Universe as a whole.
This is a self-made presentation about The Big Bang Theory (NOT the TV show :P) to be given to a lecturer and students of University level. Intended for all those to download who may have presentations to give and can't find a good enough topic :). Everyone else is free to download it for other purposes as well!!
This article aims to present the origin and evolution of Universe, Sun and Earth as well as alternative solutions for the survival of humanity with the end of Earth planet, Sun and Universe.
NEW HOT-to-COOL COSMOLOGY: Amazing Progress Yet Greater QuestionsPaul H. Carr
Astronomy has progressed from astrology to precision, hot-to-cool, cosmology. Georges Lemaitre, using Einstein’s General Relativity, predicted in 1930s that our universe expanded from a primeval atom in a hot big bang. In 1964, radio astronomers detected the whispering cosmic microwave background radiation from this hot cosmic explosion. Since 1993, an increasing number of satellites have measured that this Planck black-body radiation has cooled, as it expanded, to a very cool 2.725 K. It also has fluctuations of one part in 100,000.
Alan Guth’ inflationary universe theory predicted this as arising from quantum fluctuations at the “Beginning.”
The universe: why does it exist? Why is there something rather than nothing? Where and why did structure arise: galaxies, and clusters of galaxies. This slide show is a full history of enquiry into how structure arises in the universe. It goes from Plato and Aristotle to the Nobel Prize in Physics 2011. The title Heart of Darkness refers to a book that has the full story: Heart of Darkness, by Jeremiah P Ostriker and Simon Mitton, ISBN 978 0691134307
DevOps and Testing slides at DASA ConnectKari Kakkonen
My and Rik Marselis slides at 30.5.2024 DASA Connect conference. We discuss about what is testing, then what is agile testing and finally what is Testing in DevOps. Finally we had lovely workshop with the participants trying to find out different ways to think about quality and testing in different parts of the DevOps infinity loop.
Neuro-symbolic is not enough, we need neuro-*semantic*Frank van Harmelen
Neuro-symbolic (NeSy) AI is on the rise. However, simply machine learning on just any symbolic structure is not sufficient to really harvest the gains of NeSy. These will only be gained when the symbolic structures have an actual semantics. I give an operational definition of semantics as “predictable inference”.
All of this illustrated with link prediction over knowledge graphs, but the argument is general.
Epistemic Interaction - tuning interfaces to provide information for AI supportAlan Dix
Paper presented at SYNERGY workshop at AVI 2024, Genoa, Italy. 3rd June 2024
https://alandix.com/academic/papers/synergy2024-epistemic/
As machine learning integrates deeper into human-computer interactions, the concept of epistemic interaction emerges, aiming to refine these interactions to enhance system adaptability. This approach encourages minor, intentional adjustments in user behaviour to enrich the data available for system learning. This paper introduces epistemic interaction within the context of human-system communication, illustrating how deliberate interaction design can improve system understanding and adaptation. Through concrete examples, we demonstrate the potential of epistemic interaction to significantly advance human-computer interaction by leveraging intuitive human communication strategies to inform system design and functionality, offering a novel pathway for enriching user-system engagements.
UiPath Test Automation using UiPath Test Suite series, part 3DianaGray10
Welcome to UiPath Test Automation using UiPath Test Suite series part 3. In this session, we will cover desktop automation along with UI automation.
Topics covered:
UI automation Introduction,
UI automation Sample
Desktop automation flow
Pradeep Chinnala, Senior Consultant Automation Developer @WonderBotz and UiPath MVP
Deepak Rai, Automation Practice Lead, Boundaryless Group and UiPath MVP
Smart TV Buyer Insights Survey 2024 by 91mobiles.pdf91mobiles
91mobiles recently conducted a Smart TV Buyer Insights Survey in which we asked over 3,000 respondents about the TV they own, aspects they look at on a new TV, and their TV buying preferences.
Transcript: Selling digital books in 2024: Insights from industry leaders - T...BookNet Canada
The publishing industry has been selling digital audiobooks and ebooks for over a decade and has found its groove. What’s changed? What has stayed the same? Where do we go from here? Join a group of leading sales peers from across the industry for a conversation about the lessons learned since the popularization of digital books, best practices, digital book supply chain management, and more.
Link to video recording: https://bnctechforum.ca/sessions/selling-digital-books-in-2024-insights-from-industry-leaders/
Presented by BookNet Canada on May 28, 2024, with support from the Department of Canadian Heritage.
Connector Corner: Automate dynamic content and events by pushing a buttonDianaGray10
Here is something new! In our next Connector Corner webinar, we will demonstrate how you can use a single workflow to:
Create a campaign using Mailchimp with merge tags/fields
Send an interactive Slack channel message (using buttons)
Have the message received by managers and peers along with a test email for review
But there’s more:
In a second workflow supporting the same use case, you’ll see:
Your campaign sent to target colleagues for approval
If the “Approve” button is clicked, a Jira/Zendesk ticket is created for the marketing design team
But—if the “Reject” button is pushed, colleagues will be alerted via Slack message
Join us to learn more about this new, human-in-the-loop capability, brought to you by Integration Service connectors.
And...
Speakers:
Akshay Agnihotri, Product Manager
Charlie Greenberg, Host
LF Energy Webinar: Electrical Grid Modelling and Simulation Through PowSyBl -...DanBrown980551
Do you want to learn how to model and simulate an electrical network from scratch in under an hour?
Then welcome to this PowSyBl workshop, hosted by Rte, the French Transmission System Operator (TSO)!
During the webinar, you will discover the PowSyBl ecosystem as well as handle and study an electrical network through an interactive Python notebook.
PowSyBl is an open source project hosted by LF Energy, which offers a comprehensive set of features for electrical grid modelling and simulation. Among other advanced features, PowSyBl provides:
- A fully editable and extendable library for grid component modelling;
- Visualization tools to display your network;
- Grid simulation tools, such as power flows, security analyses (with or without remedial actions) and sensitivity analyses;
The framework is mostly written in Java, with a Python binding so that Python developers can access PowSyBl functionalities as well.
What you will learn during the webinar:
- For beginners: discover PowSyBl's functionalities through a quick general presentation and the notebook, without needing any expert coding skills;
- For advanced developers: master the skills to efficiently apply PowSyBl functionalities to your real-world scenarios.
2. There are at least 3 ways that the
age of the Universe can be
estimated:
The age of the chemical elements.
The age of the oldest star clusters.
The age of the oldest white dwarf
stars.
3. • The age of the Universe can also be
estimated from a cosmological model based on
the HUBBLE CONSTANT and the densities
of matter and dark energy. This model-
based age is currently 13.75 +/- 0.1 Gyr.
But this Web page will only deal with
actual age measurements, not estimates
from cosmological models. The actual age
measurements are consistent with the
model-based age which increases our
confidence in the Big Bang model.
4.
5. 1650: James Ussher, Archbishop of Armagh and Primate of All
Ireland, correlates Holy Writ and Middle Eastern histories to
“correct” the date to October 23, 4004 BC
6. 1831: Charles Lyell uses fossils of marine
mollusks to estimate age as 2.4x108 years
7. 1760: Buffon uses cooling of Earth from its
molten state to estimate age as 7.5x104 years
8. • Current Jewish calendar would
“suggest” a date of creation about
Sep/Oct 3760 BCE
• 1905: Lord Rutherford uses
radioactive decay of rocks to
estimate age as > 109 years (later
refined to 4.3x109 years)
9. • . In 1915 Albert Einstein published the theory
of general relativity.[16] Based on Einstein's
theory, Mgr. Georges Lemaître's work
showed that the Universe cannot be static
and must be either expanding or contracting.
Einstein himself did not believe this result
and so he added what he called a
Cosmological Constant to his equations in an
unsuccessful attempt to produce a theory
consistent with a Steady State Universe.
10. The Age of the Universe
No gravity: v = Hor to = r/v = Ho
-1
Newtonian gravity for a flat universe:
½ mv2 - GmM/r = 0 v = dr/dt = (2GM/r)½
so we can integrate r½adr = (2GM)½dt to get
to = 2/3 (r3/2GM)½ = 2/3 (r/v) = 2/3 Ho
-1
11. • The first direct observational
evidence that the Universe has a finite
age came from the observations of
astronomer Edwin Hubble published in
1929.Earlier in the 20th century, Hubble
and others resolved individual stars
within certain nebulae, thus
determining that they were galaxies,
similar to, but external to, our Milky
Way Galaxy.
12. • The first reasonably accurate
measurement of the rate of expansion
of the Universe, a numerical value now
known as the Hubble constant, was
made in 1958 by astronomer Allan
Sandage. His measured value for the
Hubble constant yielded the first good
estimate of the age of the Universe,
coming very close to the value range
generally accepted today.
13. NASA's Wilkinson Microwave Anisotropy Probe
(WMAP)
project's nine-year data release in 2012 estimated the
age of the universe to be 1.3772±0.0059×1010 years
(13.772 billion years old, with an uncertainty of plus
or minus 59 million years).
However, this age is based on the assumption that
the project's underlying model is correct; other
methods of estimating the age of the universe could
give different ages. Assuming an extra background of
relativistic particles, for example, can enlarge the
error bars of the WMAP constraint by one order of
magnitude.
BASED ON THE LIGHT TIME TRAVEL.
14. • The discovery MICROWAVE COSMIC
BACKGROUND RADIATION announced in
1965 finally brought an effective end to the
remaining scientific uncertainty over the
expanding Universe. The space probe WMAP,
launched in 2001, produced data that
determines the Hubble Constant and the age
of the Universe independent of galaxy
distances, removing the largest source of
error.
15. This number represents the first accurate
"direct" measurement of the age of the
universe (other methods typically involve
HUBBLE’S LAW and age of the oldest stars in
globular clusters, etc.). It is possible to use
different methods for determining the same
parameter (in this case – the age of the
universe) and arrive at different answers with
no overlap in the "errors".
21. • In the early 1990's, one thing was
fairly certain about the expansion of the
Universe. It might have enough energy
density to stop its expansion and
recollapse, it might have so little energy
density that it would never stop
expanding, but gravity was certain to
slow the expansion as time went on.
Granted, the slowing had not been
observed, but, theoretically, the
Universe had to slow.
22. • Then came 1998 and the Hubble Space
Telescope (HST) observations of very distant
supernovae that showed that, a long time
ago, the Universe was actually expanding
more slowly than it is today. So the
expansion of the Universe has not been
slowing due to gravity, as everyone thought,
it has been accelerating. No one expected
this, no one knew how to explain it. But
something was causing it.
23.
24.
25.
26.
27.
28.
29.
30.
31.
32.
33. Eventually theorists came up with
three sorts of explanations. Maybe there is
something wrong with Einstein's theory of
gravity and a new theory could include
some kind of field that creates this cosmic
acceleration. Theorists still don't know
what the correct explanation is, but they
have given the solution a name. It is called
dark energy.
34.
35. More is unknown than is known.
We know how much dark energy
there is because we know how it
affects the Universe's expansion.
Other than that, it is a complete
mystery. But it is an important
mystery. It turns out that roughly 70%
of the Universe is dark energy.
36.
37.
38. quantum theory of matter
• In this theory, "empty space" is actually full
of temporary ("virtual") particles that
continually form and then disappear. But
when physicists tried to calculate How much
energy this would give empty space, the
answer came out wrong - wrong by a lot.
• The number came out 10 times too big.
That's a 1 with 120 zeros after it. It's hard to
get an answer that bad. So the mystery
continues.
39. • Another explanation for dark energy is
that it is a new kind of dynamical
energy fluid or field, something that
fills all of space but something
whose effect on the expansion of
the Universe is the opposite of that
of matter and normal energy.
40. • A last possibility is that Einstein's
theory of gravity is not correct. That
would not only affect the expansion of
the Universe, but it would also affect
the way that normal matter in galaxies
and clusters of galaxies behaved. This
fact would provide a way to decide if
the solution to the dark energy problem
is a new gravity theory or not: we could
observe how galaxies come together in
clusters.
41. • AND FINALLY; the last thing that
we needed to decide between
dark energy possibilities –is that a
property of space, a new
dynamic fluid, or a new theory of
gravity - is more data, better
data.