Saturday, October 28, 2017

Latest research findings suggest we need new physics./ 29 october2017.


Hubble Discovery Suggests We May Need New Physics to Explain Dark Matter

NASA/ESA
In Brief
Scientists have observed galaxy clusters moving in a way that's inconsistent with what we know about dark matter. This might suggest that we need to rethink our current models, or that an entirely unknown phenomenon has been discovered.

What’s the Matter?

It’s thought that dark matter makes up as much as a quarter of all matter in the universe, but we know very little about it because it has never been directly observed and it is exceedingly difficult to study. Now, new research might indicate that entirely new physics is required to properly understand its behavior.
A team of Swiss, French, and British astronomers has used the Hubble Space Telescope to analyze galaxy clusters. The current cold dark matter model suggests that the brightest cluster galaxy (BCG) located in the center of one of these clusters will stay in place after a merging event, thanks to the gravitational influence of dark matter.
However, this study found that BCGs actually “wobble” long after the cluster has returned to a relaxed state. The visible area of each cluster and the center of its mass were observed to be offset by as much as 40,000 lightyears.
The researchers were able to determine this because the clusters serve as gravitational lenses, as their sheer scale means that they warp spacetime, which affects the light coming from objects beyond their location. This makes it possible to ascertain the exact position of the center of mass, and measure how far offset the BCG is.

A Shot in the Dark

The wobbling that was observed by this study is a fairly mysterious phenomenon, which offers up its own questions. However, if it is being caused by dark matter, then our current understanding of its properties is inaccurate.
Dark matter particles, if they are indeed responsible, would have to be able to interact with one another to cause this motion, which contradicts current thinking on the nature and behavior of the particles. This would suggest that we need to establish entirely new physics to properly explain our many remaining questions about dark matter.
The next step for this investigation is to look at larger datasets that might reveal more about the observed activity. The ESA’s Euclid spacecraft could provide this information – but it’s set to launch in late 2020, so it will be a few years before this vein of study is used to advance our understanding of dark matter.
“We’re looking forward to larger surveys — such as the Euclid survey — that will extend our dataset,” commented co-author Frederic Courbin of the EPFL. “Then we can determine whether the wobbling of BGCs is the result of a novel astrophysical phenomenon or new fundamental physics. Both of which would be exciting!”

Breakthrough Treatment Restores Voluntary Movement to Paralyzed Man’s Legs

Getty Images
In Brief
A new type of implant helped a patient who became paralyzed after a spinal cord injury recover movement in his legs. The new method uses electric stimulation through an implant on the spine, combined with traditional rehabilitation techniques for patients with spinal cord injuries.

Reversing the Irreversible

28 years ago, Andrew Meas broke his neck after a fall from a motorcycle — an accident that left him unable to move his limbs. Spinal cord injuries of this nature invariably lead to some form of paralysis (if not complete debilitation) that are usually deemed to be irreversible.
Meas, however, can now stand and move his legs. He was one of several patients with varying degrees of spinal injury who were given a novel treatment as part of research at the University of Louisville’s Kentucky Spinal Cord Injury Research Center (KSCIRC). In the study, researchers paired standard rehabilitation techniques with a fairly invasive method called spinal cord epidural stimulation (scES).
A device was implanted over Meas’ spinal column to electrically stimulate the lumbosacral enlargement during his physical therapy sessions. After just 44 months of regular physical training and the scES, Meas was able to move his lower limbs without any help. “Activity-dependent plasticity can re-establish voluntary control of movement and standing after complete paralysis in humans even years after injury,” KSCIRC researcher Susan Harkema, senior author of the study that appears in the journal Scientific Reports, said in a press release.

Recovery-Based Rehabilitation

The conventional wisdom touted by experts has long been that, for patients who have suffered an injury like Meas’, recovery is highly unlikely. As lead researcher Enrico Rejc said in the press release, “It is commonly believed that one year from injury, you are classified as chronic and it’s likely that you will not improve any more. This data is proof of principle that the human nervous system has much greater recovery capabilities than expected.”
It’s particularly worth noting how the treatment involved is not just electrical stimulation (a growing field in rehabilitation medicine) but rather, a combination of the new method with regular physical therapy. Meas went through both a period of assisted therapy and standard training at home, and the research team credited his recovery as much to the amount of effort he put in as they did to their implant.
Indeed, the new research surpasses the limits of current recovery treatments. As Harkema noted, “This should open up new opportunities for recovery-based rehabilitation as an agent for recovery, not just learning how to function with compensatory strategies, even for those with the most severe injuries.”

We May Need New Physics to Explain Dark Matter 28 october 2017.

https://futurism.com/hubble-discovery-suggests-we-may-need-new-physics-to-explain-dark-matter/

Hubble Discovery Suggests We May Need New Physics to Explain Dark Matter

NASA/ESA
In Brief
Scientists have observed galaxy clusters moving in a way that's inconsistent with what we know about dark matter. This might suggest that we need to rethink our current models, or that an entirely unknown phenomenon has been discovered.

What’s the Matter?

It’s thought that dark matter makes up as much as a quarter of all matter in the universe, but we know very little about it because it has never been directly observed and it is exceedingly difficult to study. Now, new research might indicate that entirely new physics is required to properly understand its behavior.
A team of Swiss, French, and British astronomers has used the Hubble Space Telescope to analyze galaxy clusters. The current cold dark matter model suggests that the brightest cluster galaxy (BCG) located in the center of one of these clusters will stay in place after a merging event, thanks to the gravitational influence of dark matter.
However, this study found that BCGs actually “wobble” long after the cluster has returned to a relaxed state. The visible area of each cluster and the center of its mass were observed to be offset by as much as 40,000 lightyears.
The researchers were able to determine this because the clusters serve as gravitational lenses, as their sheer scale means that they warp spacetime, which affects the light coming from objects beyond their location. This makes it possible to ascertain the exact position of the center of mass, and measure how far offset the BCG is.

A Shot in the Dark

The wobbling that was observed by this study is a fairly mysterious phenomenon, which offers up its own questions. However, if it is being caused by dark matter, then our current understanding of its properties is inaccurate.
Dark matter particles, if they are indeed responsible, would have to be able to interact with one another to cause this motion, which contradicts current thinking on the nature and behavior of the particles. This would suggest that we need to establish entirely new physics to properly explain our many remaining questions about dark matter.
The next step for this investigation is to look at larger datasets that might reveal more about the observed activity. The ESA’s Euclid spacecraft could provide this information – but it’s set to launch in late 2020, so it will be a few years before this vein of study is used to advance our understanding of dark matter.
“We’re looking forward to larger surveys — such as the Euclid survey — that will extend our dataset,” commented co-author Frederic Courbin of the EPFL. “Then we can determine whether the wobbling of BGCs is the result of a novel astrophysical phenomenon or new fundamental physics. Both of which would be exciting!”



Hubble Discovery Suggests We May Need New Physics to Explain Dark Matter

NASA/ESA
In Brief
Scientists have observed galaxy clusters moving in a way that's inconsistent with what we know about dark matter. This might suggest that we need to rethink our current models, or that an entirely unknown phenomenon has been discovered.

What’s the Matter?

It’s thought that dark matter makes up as much as a quarter of all matter in the universe, but we know very little about it because it has never been directly observed and it is exceedingly difficult to study. Now, new research might indicate that entirely new physics is required to properly understand its behavior.
A team of Swiss, French, and British astronomers has used the Hubble Space Telescope to analyze galaxy clusters. The current cold dark matter model suggests that the brightest cluster galaxy (BCG) located in the center of one of these clusters will stay in place after a merging event, thanks to the gravitational influence of dark matter.
However, this study found that BCGs actually “wobble” long after the cluster has returned to a relaxed state. The visible area of each cluster and the center of its mass were observed to be offset by as much as 40,000 lightyears.
The researchers were able to determine this because the clusters serve as gravitational lenses, as their sheer scale means that they warp spacetime, which affects the light coming from objects beyond their location. This makes it possible to ascertain the exact position of the center of mass, and measure how far offset the BCG is.

A Shot in the Dark

The wobbling that was observed by this study is a fairly mysterious phenomenon, which offers up its own questions. However, if it is being caused by dark matter, then our current understanding of its properties is inaccurate.
Dark matter particles, if they are indeed responsible, would have to be able to interact with one another to cause this motion, which contradicts current thinking on the nature and behavior of the particles. This would suggest that we need to establish entirely new physics to properly explain our many remaining questions about dark matter.
The next step for this investigation is to look at larger datasets that might reveal more about the observed activity. The ESA’s Euclid spacecraft could provide this information – but it’s set to launch in late 2020, so it will be a few years before this vein of study is used to advance our understanding of dark matter.
“We’re looking forward to larger surveys — such as the Euclid survey — that will extend our dataset,” commented co-author Frederic Courbin of the EPFL. “Then we can determine whether the wobbling of BGCs is the result of a novel astrophysical phenomenon or new fundamental physics. Both of which would be exciting!”
























N.Kores rocket fools was warned by Chinese Geologists.28 octo . 2017


WORLD

NORTH KOREA ON VERGE OF CATASTROPHE AT NUCLEAR TEST SITE, CHINA WARNS

By John Haltiwanger On Friday, October 27, 2017 - 15:38

Chinese geologists have warned North Korea that if it conducts another test at the mountainous Punggye-ri nuclear facility, the consequences could be catastrophic.PHOTO: GETTY IMAGES

Chinese geologists have warned North Korea that the consequences could be catastrophic if it conducts another test at the mountainous Punggye-ri nuclear facility, the South China Morning Postreports. 

North Korea conducted its sixth nuclear test at the facility, situated roughly 50 miles from China's border, in early September. After the test, a senior Chinese nuclear scientist warned that another test could blow off the top of the mountain and lead to a massive collapse, which could allow radioactive waste to be blown across the border into China. This warning came as a North Korean delegation met with the Chinese Academy of Sciences’ Institute of Geology in Beijing on September 20. 

Pyongyang's September nuclear test was its most powerful yet. It was estimated to have a yield of 100 kilotons, which would make it roughly seven times as strong as the U.S. atomic bomb that decimated the Japanese city of Hiroshima during World War II in 1945. 

Keep Up With This Story And More By Subscribing Now

Since the test, North Korea has threatened to test a hydrogen bomb over the Pacific Ocean, which could pose a huge risk to aircraft and shipping. During an interview that aired on CNN Wednesday, an official representing North Korea's government, Ri Yong Pil, told the U.S. it must take the North Korean test threat "literally." 

As U.S. Defense Secretary James Mattis visited the Demilitarized Zone that divides South Korea from North Korea on Friday, he decried Pyongyang's recent actions. But he also emphasized that the U.S. desires a "diplomatic solution" to the two nation's differences. 

"North Korean provocations continue to threaten regional and world peace, and despite unanimous condemnation by the United Nations’ Security Council, they still proceed," Mattis said. "As Secretary of State [Rex] Tillerson has made clear, our goal is not war but rather the complete, verifiable and irreversible denuclearization of the Korean Peninsula."

The U.S. and North Korea have been enemies for over half a century, but tensions have been particularly high in recent months as Pyongyang has ramped up its long-range missile tests and refused to give into global pressure to end its nuclear program. 

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Monday, October 23, 2017

Ripples of Rohinjya atrocities.





10/21/2017 12:51 pm ET Updated 8 hours ago

Oxford Students To Alumna Aung San Suu Kyi: Rohingya Inaction Is 'Inexcusable'Myanmar’s civilian leader is under increasing scrutiny for her failure to address the humanitarian crisis.

By Jesselyn Cook

Students at St. Hugh’s College in Oxford have joined an international chorus of critics in condemning their alumna Aung San Suu Kyi, now the de facto leader of Myanmar, for her response to the crisis engulfing the Rohingya in the country’s Rakhine State.

Undergraduates at St. Hugh’s, where Suu Kyi studied in the 1960s, voted this week to remove her name from the title of their junior common room. The gesture is a protest against her unwillingness to address the state-sponsored persecution of Myanmar’s Muslim-minority Rohingya communities.

The college, which also removed her portrait from its main entrance earlier this year, granted Suu Kyi an honorary doctorate as one of its “most distinguished and remarkable alumni” in 2012.

At the time, Suu Kyi, a Nobel Peace Prize laureate and former political prisoner, was still widely idolized as a champion of democracy and non-violent human rights advocacy. She spent nearly 15 years under house arrest while campaigning against Myanmar’s decades-long military dictatorship, and became the nation’s state counselor in 2016, a position equivalent to prime minister in many countries.

SOE ZEYA TUN/REUTERS

Myanmar State Counselor Aung San Suu Kyi delivers a speech in Naypyitaw, Myanmar. on Sept. 19.

But the activist-turned-politician has been conspicuously silent as a military campaign denounced by the United Nations as a “textbook example of ethnic cleansing” continues to push Rohingyas out of the country at a staggering rate. At least 537,000 refugees ― more than half of Myanmar’s Rohingya population ― have fled to neighboring Bangladesh in a matter of weeks.

Crimes against humanity

In late August, a Rohingya insurgency attacked a number of government security posts in Buddhist-majority Myanmar, where Rohingyas have endured decades of discrimination and extremely limited rights. Twelve officers were killed.

The military unleashed a retaliatory crackdown, which international observers have decried as barbaric and disproportionate. State actors have committed atrocities amounting to crimes against humanity, according to Amnesty International.

After conducting more than 150 interviews with survivors and eyewitnesses, the human rights group released a report this week alleging that Rohingya men, women and children have been indiscriminately killed, burned, tortured, raped and shot, among other abuses.

COURTESY OF UNICEF

A drawing by a Rohingya boy illustrates the horrific experiences he endured while fleeing from Myanmar to Bangladesh.

“In this orchestrated campaign, Myanmar’s security forces have brutally meted out revenge on the entire Rohingya population of northern Rakhine State, in an apparent attempt to permanently drive them out of the country,” said Tirana Hassan, Amnesty’s crisis response director. “These atrocities continue to fuel the region’s worst refugee crisis in decades.” 

The report features testimonies from Rohingya refugees recounting horrific tales of being burned alive and watching loved ones die before their eyes while attempting to escape security forces’ gunfire.

Suu Kyi’s silence

Bangladesh is grappling with insufficient resources to accommodate the influx of desperate Rohingyas. Many have traveled by land or sea for days without food.

In September, a boat carrying more than 60 refugees capsized off the Bangladeshi coast. All were presumed dead, including several babies.

As many as 1,800 Rohingya children are making the perilous journey across the border per day, according to a new report from UNICEF.

KEVIN FRAYER VIA GETTY IMAGES

A Rohingya boy cries as he climbs on a truck distributing aid for a local NGO near the Balukali refugee camp on Sept. 20 in Cox's Bazar, Bangladesh.

But as the crisis escalates, Suu Kyi has remained tight-lipped on the Rohingyas’ plight, despite mounting pressure to speak out and take action. 

She skipped the 2017 U.N. General Assembly in New York, where world leaders discussed Myanmar’s Rohingya exodus in her absence. 

Suu Kyi has even dismissed accusations of state-sponsored crimes against the minority group as “misinformation.” The government “has already started defending all the people in Rakhine in the best way possible,” her office claimed in a Facebook post last month.

But Myanmar’s government has tightened restrictions on urgently needed aid supplies and services in Rakhine State. It has also denied access to humanitarian groups as well as a U.N. fact-finding mission in the country and other attempted investigations into the alleged and documented persecution.

International outrage

Suu Kyi’s inaction has sparked protests around the world and calls for her Nobel Prize to be revoked.

“I am still waiting for my fellow Nobel Laureate Aung San Suu Kyi” to condemn the “tragic and shameful treatment” of Myanmar’s Rohingya Muslims, 20-year-old activist Malala Yousafzai wrote on Twitter. “The world is waiting and the Rohingya Muslims are waiting.”

South African anti-apartheid leader Desmond Tutu, another Nobel laureate, also issued an emotional plea to his “dear sister” Suu Kyi.

“I am now elderly, decrepit and formally retired, but breaking my vow to remain silent on public affairs out of profound sadness about the plight of the Muslim minority in your country, the Rohingya,” he wrote. “If the political price of your ascension to the highest office in Myanmar is your silence, the price is surely too steep.”

NURPHOTO VIA GETTY IMAGES

An Indonesian protester burns a picture of Suu Kyi during a rally in front of the Myanmar embassy in Jakarta on Sept. 2.

Less than two weeks after the military crackdown erupted, Yanghee Lee, the U.N.’s special rapporteur on human rights in Myanmar, called the situation in Rakhine “really grave,” and said it was time for Suu Kyi to “step in.”

“That is what we would expect from any government: to protect everybody within their own jurisdiction,” Lee added.

The students at St. Hugh’s are urging others to join them in denouncing their disgraced alumna’s “inexcusable and unacceptable” negligence.

“We must condemn Aung San Suu Kyi’s silence and complicity on this issue and her condonation of the human rights offenses [in] her own land,” they said. “In doing so, she has gone against the very principles and ideals she had once righteously promoted.”

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Friday, October 20, 2017

bASICS OF Physics. 214 octo. 2017


Contents

Definition

Pressure is the amount of force applied perpendicular to the surface of an object per unit area. The symbol for it is p or P.[1] The IUPAC recommendation for pressure is a lower-case p.[2] However, upper-case P is widely used. The usage of P vs p depends upon the field in which one is working, on the nearby presence of other symbols for quantities such as power and momentum, and on writing style.

Formula

Pressure force area.svg
Mathematically:
{\displaystyle p={\frac {F}{A}},}
where:
p is the pressure,
F is the normal force,
A is the area of the surface on contact.
Pressure is a scalar quantity. It relates the vector surface element (a vector normal to the surface) with the normal force acting on it. The pressure is the scalar proportionality constant that relates the two normal vectors:
{\displaystyle d\mathbf {F} _{n}=-p\,d\mathbf {A} =-p\,\mathbf {n} \,dA.}
The minus sign comes from the fact that the force is considered towards the surface element, while the normal vector points outward. The equation has meaning in that, for any surface S in contact with the fluid, the total force exerted by the fluid on that surface is the surface integral over S of the right-hand side of the above equation.
It is incorrect (although rather usual) to say "the pressure is directed in such or such direction". The pressure, as a scalar, has no direction. The force given by the previous relationship to the quantity has a direction, but the pressure does not. If we change the orientation of the surface element, the direction of the normal force changes accordingly, but the pressure remains the same.
Pressure is distributed to solid boundaries or across arbitrary sections of fluid normal to these boundaries or sections at every point. It is a fundamental parameter in thermodynamics, and it is conjugate to volume.

Units

Mercury column
The SI unit for pressure is the pascal (Pa), equal to one newton per square metre (N/m2, or kg·m−1·s−2). This name for the unit was added in 1971;[3] before that, pressure in SI was expressed simply in newtons per square metre.
Other units of pressure, such as pounds per square inch and bar, are also in common use. The CGS unit of pressure is the barye (Ba), equal to 1 dyn·cm−2, or 0.1 Pa. Pressure is sometimes expressed in grams-force or kilograms-force per square centimetre (g/cm2 or kg/cm2) and the like without properly identifying the force units. But using the names kilogram, gram, kilogram-force, or gram-force (or their symbols) as units of force is expressly forbidden in SI. The technical atmosphere (symbol: at) is 1 kgf/cm2 (98.0665 kPa, or 14.223 psi).
Since a system under pressure has the potential to perform work on its surroundings, pressure is a measure of potential energy stored per unit volume. It is therefore related to energy density and may be expressed in units such as joules per cubic metre (J/m3, which is equal to Pa). Mathematically:
{\displaystyle p={\frac {F\times {\text{distance}}}{A\times {\text{distance}}}}={\frac {\text{work}}{\text{volume}}}={\frac {\text{energy (J)}}{{\text{volume }}({\text{m}}^{3})}}.}
Some meteorologists prefer the hectopascal (hPa) for atmospheric air pressure, which is equivalent to the older unit millibar (mbar). Similar pressures are given in kilopascals (kPa) in most other fields, where the hecto- prefix is rarely used. The inch of mercury is still used in the United States. Oceanographers usually measure underwater pressure in decibars (dbar) because pressure in the ocean increases by approximately one decibar per metre depth.
The standard atmosphere (atm) is an established constant. It is approximately equal to typical air pressure at Earth mean sea level and is defined as 101325 Pa.
Because pressure is commonly measured by its ability to displace a column of liquid in a manometer, pressures are often expressed as a depth of a particular fluid (e.g., centimetres of water, millimetres of mercury or inches of mercury). The most common choices are mercury (Hg) and water; water is nontoxic and readily available, while mercury's high density allows a shorter column (and so a smaller manometer) to be used to measure a given pressure. The pressure exerted by a column of liquid of height h and density ρ is given by the hydrostatic pressure equation p = ρgh, where g is the gravitational acceleration. Fluid density and local gravity can vary from one reading to another depending on local factors, so the height of a fluid column does not define pressure precisely. When millimetres of mercury or inches of mercury are quoted today, these units are not based on a physical column of mercury; rather, they have been given precise definitions that can be expressed in terms of SI units.[citation needed] One millimetre of mercury is approximately equal to one torr. The water-based units still depend on the density of water, a measured, rather than defined, quantity. These manometric units are still encountered in many fields. Blood pressure is measured in millimetres of mercury in most of the world, and lung pressures in centimetres of water are still common.
Underwater divers use the metre sea water (msw or MSW) and foot sea water (fsw or FSW) units of pressure, and these are the standard units for pressure gauges used to measure pressure exposure in diving chambers and personal decompression computers. A msw is defined as 0.1 bar (= 100000 Pa = 10000 Pa), is not the same as a linear metre of depth. 33.066 fsw = 1 atm[4] (1 atm = 101325 Pa / 33.066 = 3064.326 Pa). Note that the pressure conversion from msw to fsw is different from the length conversion: 10 msw = 32.6336 fsw, while 10 m = 32.8083 ft.[5]
Gauge pressure is often given in units with "g" appended, e.g. "kPag", "barg" or "psig", and units for measurements of absolute pressure are sometimes given a suffix of "a", to avoid confusion, for example "kPaa", "psia". However, the US National Institute of Standards and Technology recommends that, to avoid confusion, any modifiers be instead applied to the quantity being measured rather than the unit of measure.[6] For example, "pg = 100 psi" rather than "p = 100 psig".
Differential pressure is expressed in units with "d" appended; this type of measurement is useful when considering sealing performance or whether a valve will open or close.
Presently or formerly popular pressure units include the following:
  • atmosphere (atm)
  • manometric units:
    • centimetre, inch, millimetre (torr) and micrometre (mTorr, micron) of mercury,
    • height of equivalent column of water, including millimetre (mm H
      2
      O
      ), centimetre (cm H
      2
      O
      ), metre, inch, and foot of water;
  • imperial and customary units:
  • non-SI metric units:
    • bar, decibar, millibar,
      • msw (metres sea water), used in underwater diving, particularly in connection with diving pressure exposure and decompression,
    • kilogram-force, or kilopond, per square centimetre (technical atmosphere),
    • gram-force and tonne-force (metric ton-force) per square centimetre,
    • barye (dyne per square centimetre),
    • kilogram-force and tonne-force per square metre,
    • sthene per square metre (pieze).
Pressure units
Pascal Bar Technical atmosphere Standard atmosphere Torr Pounds per square inch
(Pa) (bar) (at) (atm) (Torr) (psi)
1 Pa ≡ 1 N/m2 10−5 1.0197×10−5 9.8692×10−6 7.5006×10−3 1.450377×10−4
1 bar 105 ≡ 100 kPa ≡ 106 dyn/cm2
1.0197 0.98692 750.06 14.50377
1 at 9.80665×104 0.980665 ≡ 1 kp/cm2 0.9678411 735.5592 14.22334
1 atm 1.01325×105 1.01325 1.0332 1 760 14.69595
1 Torr 133.3224 1.333224×10−3 1.359551×10−3 ≡ 1/760 ≈ 1.315789×10−3 ≡ 1 Torr ≈ 1 mmHg
1.933678×10−2
1 psi 6.8948×103 6.8948×10−2 7.03069×10−2 6.8046×10−2 51.71493 ≡ 1 lbf /in2

Examples

The effects of an external pressure of 700 bar on an aluminum cylinder with 5 mm wall thickness
As an example of varying pressures, a finger can be pressed against a wall without making any lasting impression; however, the same finger pushing a thumbtack can easily damage the wall. Although the force applied to the surface is the same, the thumbtack applies more pressure because the point concentrates that force into a smaller area. Pressure is transmitted to solid boundaries or across arbitrary sections of fluid normal to these boundaries or sections at every point. Unlike stress, pressure is defined as a scalar quantity. The negative gradient of pressure is called the force density.
Another example is a knife. If we try to cut a fruit with the flat side, the force is distributed over a large area, and it will not cut. But if we use the edge, it will cut smoothly. The reason is that the flat side has a greater surface area (less pressure), and so it does not cut the fruit. When we take the thin side, the surface area is reduced, and so it cuts the fruit easily and quickly. This is one example of a practical application of pressure.
For gases, pressure is sometimes measured not as an absolute pressure, but relative to atmospheric pressure; such measurements are called gauge pressure. An example of this is the air pressure in an automobile tire, which might be said to be "220 kPa (32 psi)", but is actually 220 kPa (32 psi) above atmospheric pressure. Since atmospheric pressure at sea level is about 100 kPa (14.7 psi), the absolute pressure in the tire is therefore about 320 kPa (46.7 psi). In technical work, this is written "a gauge pressure of 220 kPa (32 psi)". Where space is limited, such as on pressure gauges, name plates, graph labels, and table headings, the use of a modifier in parentheses, such as "kPa (gauge)" or "kPa (absolute)", is permitted. In non-SI technical work, a gauge pressure of 32 psi is sometimes written as "32 psig", and an absolute pressure as "32 psia", though the other methods explained above that avoid attaching characters to the unit of pressure are preferred.[7]
Gauge pressure is the relevant measure of pressure wherever one is interested in the stress on storage vessels and the plumbing components of fluidics systems. However, whenever equation-of-state properties, such as densities or changes in densities, must be calculated, pressures must be expressed in terms of their absolute values. For instance, if the atmospheric pressure is 100 kPa, a gas (such as helium) at 200 kPa (gauge) (300 kPa [absolute]) is 50% denser than the same gas at 100 kPa (gauge) (200 kPa [absolute]). Focusing on gauge values, one might erroneously conclude the first sample had twice the density of the second one.

Scalar nature

In a static gas, the gas as a whole does not appear to move. The individual molecules of the gas, however, are in constant random motion. Because we are dealing with an extremely large number of molecules and because the motion of the individual molecules is random in every direction, we do not detect any motion. If we enclose the gas within a container, we detect a pressure in the gas from the molecules colliding with the walls of our container. We can put the walls of our container anywhere inside the gas, and the force per unit area (the pressure) is the same. We can shrink the size of our "container" down to a very small point (becoming less true as we approach the atomic scale), and the pressure will still have a single value at that point. Therefore, pressure is a scalar quantity, not a vector quantity. It has magnitude but no direction sense associated with it. Pressure force acts in all directions at a point inside a gas. At the surface of a gas, the pressure force acts perpendicular (at right angle) to the surface.
A closely related quantity is the stress tensor σ, which relates the vector force \mathbf {F} to the vector area \mathbf {A} via the linear relation {\displaystyle \mathbf {F} =\sigma \mathbf {A} }.
This tensor may be expressed as the sum of the viscous stress tensor minus the hydrostatic pressure. The negative of the stress tensor is sometimes called the pressure tensor, but in the following, the term "pressure" will refer only to the scalar pressure.
According to the theory of general relativity, pressure increases the strength of a gravitational field (see stress–energy tensor) and so adds to the mass-energy cause of gravity. This effect is unnoticeable at everyday pressures but is significant in neutron stars, although it has not been experimentally tested.[8]

Types

Fluid pressure

Fluid pressure is most often the compressive stress at some point within a fluid. (The term fluid refers to both liquids and gases – for more information specifically about liquid pressure, see section below.)
Fluid pressure occurs in one of two situations:
  1. An open condition, called "open channel flow", e.g. the ocean, a swimming pool, or the atmosphere.
  2. A closed condition, called "closed conduit", e.g. a water line or gas line.
Pressure in open conditions usually can be approximated as the pressure in "static" or non-moving conditions (even in the ocean where there are waves and currents), because the motions create only negligible changes in the pressure. Such conditions conform with principles of fluid statics. The pressure at any given point of a non-moving (static) fluid is called the hydrostatic pressure.
Closed bodies of fluid are either "static", when the fluid is not moving, or "dynamic", when the fluid can move as in either a pipe or by compressing an air gap in a closed container. The pressure in closed conditions conforms with the principles of fluid dynamics.
The concepts of fluid pressure are predominantly attributed to the discoveries of Blaise Pascal and Daniel Bernoulli. Bernoulli's equation can be used in almost any situation to determine the pressure at any point in a fluid. The equation makes some assumptions about the fluid, such as the fluid being ideal[9] and incompressible.[9] An ideal fluid is a fluid in which there is no friction, it is inviscid [9] (zero viscosity).[9] The equation for all points of a system filled with a constant-density fluid is[10]
{\displaystyle {\frac {p}{\gamma }}+{\frac {v^{2}}{2g}}+z=\mathrm {const} ,}
where:
p = pressure of the fluid,
γ = ρg = density · acceleration of gravity = specific weight of the fluid,[9]
v = velocity of the fluid,
g = acceleration of gravity,
z = elevation,
{\frac {p}{\gamma }} = pressure head,
\frac{v^2}{2g} = velocity head.

Applications

Explosion or deflagration pressures

Explosion or deflagration pressures are the result of the ignition of explosive gases, mists, dust/air suspensions, in unconfined and confined spaces.

Negative pressures

Low-pressure chamber in Bundesleistungszentrum Kienbaum, Germany
While pressures are, in general, positive, there are several situations in which negative pressures may be encountered:
  • When dealing in relative (gauge) pressures. For instance, an absolute pressure of 80 kPa may be described as a gauge pressure of −21 kPa (i.e., 21 kPa below an atmospheric pressure of 101 kPa).
  • When attractive intermolecular forces (e.g., van der Waals forces or hydrogen bonds) between the particles of a fluid exceed repulsive forces due to thermal motion. These forces explain ascent of sap in tall plants. An apparent negative pressure must act on water molecules at the top of any tree taller than 10 m, which is the pressure head of water that balances the atmospheric pressure. Intermolecular forces maintain cohesion of columns of sap that run continuously in xylem from the roots to the top leaves.[11]
  • The Casimir effect can create a small attractive force due to interactions with vacuum energy; this force is sometimes termed "vacuum pressure" (not to be confused with the negative gauge pressure of a vacuum).
  • For non-isotropic stresses in rigid bodies, depending on how the orientation of a surface is chosen, the same distribution of forces may have a component of positive pressure along one surface normal, with a component of negative pressure acting along another surface normal.
    • The stresses in an electromagnetic field are generally non-isotropic, with the pressure normal to one surface element (the normal stress) being negative, and positive for surface elements perpendicular to this.
  • In the cosmological constant.

Stagnation pressure

Stagnation pressure is the pressure a fluid exerts when it is forced to stop moving. Consequently, although a fluid moving at higher speed will have a lower static pressure, it may have a higher stagnation pressure when forced to a standstill. Static pressure and stagnation pressure are related by:
p_{0} = \frac{1}{2}\rho v^2 + p
where
p_{0} is the stagnation pressure
v is the flow velocity
p is the static pressure.
The pressure of a moving fluid can be measured using a Pitot tube, or one of its variations such as a Kiel probe or Cobra probe, connected to a manometer. Depending on where the inlet holes are located on the probe, it can measure static pressures or stagnation pressures.

Surface pressure and surface tension

There is a two-dimensional analog of pressure – the lateral force per unit length applied on a line perpendicular to the force.
Surface pressure is denoted by π:
\pi = \frac{F}{l}
and shares many similar properties with three-dimensional pressure. Properties of surface chemicals can be investigated by measuring pressure/area isotherms, as the two-dimensional analog of Boyle's law, πA = k, at constant temperature.
Surface tension is another example of surface pressure, but with a reversed sign, because "tension" is the opposite to "pressure".

Pressure of an ideal gas

In an ideal gas, molecules have no volume and do not interact. According to the ideal gas law, pressure varies linearly with temperature and quantity, and inversely with volume:
{\displaystyle p={\frac {nRT}{V}},}
where:
p is the absolute pressure of the gas,
n is the amount of substance,
T is the absolute temperature,
V is the volume,
R is the ideal gas constant.
Real gases exhibit a more complex dependence on the variables of state.[12]

Vapour pressure

Vapour pressure is the pressure of a vapour in thermodynamic equilibrium with its condensed phases in a closed system. All liquids and solids have a tendency to evaporate into a gaseous form, and all gases have a tendency to condense back to their liquid or solid form.
The atmospheric pressure boiling point of a liquid (also known as the normal boiling point) is the temperature at which the vapor pressure equals the ambient atmospheric pressure. With any incremental increase in that temperature, the vapor pressure becomes sufficient to overcome atmospheric pressure and lift the liquid to form vapour bubbles inside the bulk of the substance. Bubble formation deeper in the liquid requires a higher pressure, and therefore higher temperature, because the fluid pressure increases above the atmospheric pressure as the depth increases.
The vapor pressure that a single component in a mixture contributes to the total pressure in the system is called partial vapor pressure.

Liquid pressure

When a person swims under the water, water pressure is felt acting on the person's eardrums. The deeper that person swims, the greater the pressure. The pressure felt is due to the weight of the water above the person. As someone swims deeper, there is more water above the person and therefore greater pressure. The pressure a liquid exerts depends on its depth.
Liquid pressure also depends on the density of the liquid. If someone was submerged in a liquid more dense than water, the pressure would be correspondingly greater. The pressure due to a liquid in liquid columns of constant density or at a depth within a substance is represented by the following formula:
{\displaystyle p=\rho gh,}
where:
p is liquid pressure,
g is gravity at the surface of overlaying material,
ρ is density of liquid,
h is height of liquid column or depth within a substance.
Another way of saying the same formula is the following:
{\displaystyle p={\text{weight density}}\times {\text{depth}}.}
The pressure a liquid exerts against the sides and bottom of a container depends on the density and the depth of the liquid. If atmospheric pressure is neglected, liquid pressure against the bottom is twice as great at twice the depth; at three times the depth, the liquid pressure is threefold; etc. Or, if the liquid is two or three times as dense, the liquid pressure is correspondingly two or three times as great for any given depth. Liquids are practically incompressible – that is, their volume can hardly be changed by pressure (water volume decreases by only 50 millionths of its original volume for each atmospheric increase in pressure). Thus, except for small changes produced by temperature, the density of a particular liquid is practically the same at all depths.
Atmospheric pressure pressing on the surface of a liquid must be taken into account when trying to discover the total pressure acting on a liquid. The total pressure of a liquid, then, is ρgh plus the pressure of the atmosphere. When this distinction is important, the term total pressure is used. Otherwise, discussions of liquid pressure refer to pressure without regard to the normally ever-present atmospheric pressure.
It is important to recognize that the pressure does not depend on the amount of liquid present. Volume is not the important factor – depth is. The average water pressure acting against a dam depends on the average depth of the water and not on the volume of water held back. For example, a wide but shallow lake with a depth of 3 m (10 ft) exerts only half the average pressure that a small 6 m (20 ft) deep pond does (note that the total force applied to the longer dam will be greater, due to the greater total surface area for the pressure to act upon, but for a given 5-foot section of each dam, the 10 ft deep water will apply half the force of 20 ft deep water). A person will feel the same pressure whether his/her head is dunked a metre beneath the surface of the water in a small pool or to the same depth in the middle of a large lake. If four vases contain different amounts of water but are all filled to equal depths, then a fish with its head dunked a few centimetres under the surface will be acted on by water pressure that is the same in any of the vases. If the fish swims a few centimetres deeper, the pressure on the fish will increase with depth and be the same no matter which vase the fish is in. If the fish swims to the bottom, the pressure will be greater, but it makes no difference what vase it is in. All vases are filled to equal depths, so the water pressure is the same at the bottom of each vase, regardless of its shape or volume. If water pressure at the bottom of a vase were greater than water pressure at the bottom of a neighboring vase, the greater pressure would force water sideways and then up the narrower vase to a higher level until the pressures at the bottom were equalized. Pressure is depth dependent, not volume dependent, so there is a reason that water seeks its own level.
Restating this as energy equation, the energy per unit volume in an ideal, incompressible liquid is constant throughout its vessel. At the surface, gravitational potential energy is large but liquid pressure energy is low. At the bottom of the vessel, all the gravitational potential energy is converted to pressure energy. The sum of pressure energy and gravitational potential energy per unit volume is constant throughout the volume of the fluid and the two energy components change linearly with the depth.[13] Mathematically, it is described by Bernoulli's equation, where velocity head is zero and comparisons per unit volume in the vessel are
{\displaystyle {\frac {p}{\gamma }}+z=\mathrm {const} .}
Terms have the same meaning as in section Fluid pressure.

Direction of liquid pressure

An experimentally determined fact about liquid pressure is that it is exerted equally in all directions.[14] If someone is submerged in water, no matter which way that person tilts his/her head, the person will feel the same amount of water pressure on his/her ears. Because a liquid can flow, this pressure isn't only downward. Pressure is seen acting sideways when water spurts sideways from a leak in the side of an upright can. Pressure also acts upward, as demonstrated when someone tries to push a beach ball beneath the surface of the water. The bottom of a boat is pushed upward by water pressure (buoyancy).
When a liquid presses against a surface, there is a net force that is perpendicular to the surface. Although pressure doesn't have a specific direction, force does. A submerged triangular block has water forced against each point from many directions, but components of the force that are not perpendicular to the surface cancel each other out, leaving only a net perpendicular point.[14] This is why water spurting from a hole in a bucket initially exits the bucket in a direction at right angles to the surface of the bucket in which the hole is located. Then it curves downward due to gravity. If there are three holes in a bucket (top, bottom, and middle), then the force vectors perpendicular to the inner container surface will increase with increasing depth – that is, a greater pressure at the bottom makes it so that the bottom hole will shoot water out the farthest. The force exerted by a fluid on a smooth surface is always at right angles to the surface. The speed of liquid out of the hole is \scriptstyle \sqrt{2gh}, where h is the depth below the free surface.[14] Interestingly, this is the same speed the water (or anything else) would have if freely falling the same vertical distance h.

Kinematic pressure

P=p/\rho_0
is the kinematic pressure, where p is the pressure and \rho _{0} constant mass density. The SI unit of P is m2/s2. Kinematic pressure is used in the same manner as kinematic viscosity \nu in order to compute Navier–Stokes equation without explicitly showing the density \rho _{0}.
Navier–Stokes equation with kinematic quantities
{\displaystyle {\frac {\partial u}{\partial t}}+(u\nabla )u=-\nabla P+\nu \nabla ^{2}u.}

See also

Notes


  1. The preferred spelling varies by country and even by industry. Further, both spellings are often used within a particular industry or country. Industries in British English-speaking countries typically use the "gauge" spelling.

References


  • Giancoli, Douglas G. (2004). Physics: principles with applications. Upper Saddle River, N.J.: Pearson Education. ISBN 0-13-060620-0.
    1. Hewitt 251 (2006)


      Pressure

      From Wikipedia, the free encyclopedia
      Pressure
      Common symbols
      p, P
      SI unit Pascal [Pa]
      In SI base units N/m2, 1 kg/(m·s2), or 1 J/m3
      SI dimension L^{-1}MT^{-2}
      Derivations from
      other quantities
      p = F / A
      A figure showing pressure exerted by particle collisions inside a closed container. The collisions that exert the pressure are highlighted in red.
      Pressure as exerted by particle collisions inside a closed container
      Pressure (symbol: p or P) is the force applied perpendicular to the surface of an object per unit area over which that force is distributed. Gauge pressure (also spelled gage pressure)[a] is the pressure relative to the ambient pressure.
      Various units are used to express pressure. Some of these derive from a unit of force divided by a unit of area; the SI unit of pressure, the pascal (Pa), for example, is one newton per square metre; similarly, the pound-force per square inch (psi) is the traditional unit of pressure in the imperial and US customary systems. Pressure may also be expressed in terms of standard atmospheric pressure; the atmosphere (atm) is equal to this pressure, and the torr is defined as 1760 of this. Manometric units such as the centimetre of water, millimetre of mercury, and inch of mercury are used to express pressures in terms of the height of column of a particular fluid in a manometer.



    External links


  • McNaught, A. D.; Wilkinson, A.; Nic, M.; Jirat, J.; Kosata, B.; Jenkins, A. (2014). IUPAC. Compendium of Chemical Terminology, 2nd ed. (the "Gold Book"). 2.3.3. Oxford: Blackwell Scientific Publications. ISBN 0-9678550-9-8. doi:10.1351/goldbook.P04819.
  • "14th Conference of the International Bureau of Weights and Measures". Bipm.fr. Retrieved 2012-03-27.
  • US Navy (2006). US Navy Diving Manual, 6th revision. United States: US Naval Sea Systems Command. pp. 2–32. Retrieved 2008-06-15.
  • "U.S. Navy Diving Manual (Chapter 2:Underwater Physics)" (PDF). p. 2.32.
  • "Rules and Style Conventions for Expressing Values of Quantities". NIST. Retrieved 2009-07-07.
  • NIST, Rules and Style Conventions for Expressing Values of Quantities, Sect. 7.4.
  • "Einstein's gravity under pressure". Astrophysics and Space Science. 321: 151–156. Bibcode:2009Ap&SS.321..151V. arXiv:0705.0825Freely accessible. doi:10.1007/s10509-009-0016-8. Retrieved 2012-03-27.
  • Finnemore, John, E. and Joseph B. Franzini (2002). Fluid Mechanics: With Engineering Applications. New York: McGraw Hill, Inc. pp. 14–29. ISBN 978-0-07-243202-2.
  • NCEES (2011). Fundamentals of Engineering: Supplied Reference Handbook. Clemson, South Carolina: NCEES. p. 64. ISBN 978-1-932613-59-9.
  • Karen Wright (March 2003). "The Physics of Negative Pressure". Discover. Retrieved 31 January 2015.
  • P. Atkins, J. de Paula Elements of Physical Chemistry, 4th Ed, W. H. Freeman, 2006. ISBN 0-7167-7329-5.
  • Streeter, V. L., Fluid Mechanics, Example 3.5, McGraw–Hill Inc. (1966), New York.