Crossword Solver > found answer > DECELERATE

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CROSSWORD
ANSWER

decelerate

Searching in Crosswords ...

The answer DECELERATE has 23 possible clue(s) in existing crosswords.

Searching in Word Games ...

The word DECELERATE is VALID in some board games. Check DECELERATE in word games in Scrabble, Words With Friends, see scores, anagrams etc.

Searching in Dictionaries ...

Definitions of decelerate in various dictionaries:

verb - lose velocity

verb - reduce the speed of

To decrease the velocity of.

more

Word Research / Anagrams and more ...

Keep reading for additional results and analysis below.

Possible Crossword Clues
Brake
Slow down
Reduce speed
Move more slowly
Slow machine finally sticks, but not entirely stuck in time
Slow eel reacted when tickled
English salad plant needing to be cut in time? Slow down
Slow down in river when treacle's poured in
Check one's speed

Last Seen in these Crosswords & Puzzles
Apr 17 2018 New York Times
Jun 19 2017 The Guardian - Quick crossword
Feb 17 2017 The Times - Concise
Nov 25 2015 The Guardian - Cryptic crossword
Sep 4 2015 The Guardian - Quick crossword
Mar 28 2015 The Times - Concise
May 4 2013 The Times - Concise
Sep 1 2012 The Times - Cryptic
Dec 3 2010 The Times - Concise
Nov 23 2010 The Telegraph - Toughie

Possible Jeopardy Clues
Slow down, as in a car

Possible Dictionary Clues
reduce or cause to reduce in speed.
Reduce or cause to reduce in speed.
reduce the speed of
lose velocity move more slowly
To decrease the velocity of.
To slow down the rate of advancement of: measures intended to decelerate the arms buildup.
To decrease in velocity.
to reduce the speed that a vehicle is travelling at:
to happen or make something happen more slowly
to become slower:

Decelerate might refer to
The Deceleration parameter * * * * q * * * {\displaystyle q} * in cosmology is a dimensionless measure of the cosmic acceleration of the expansion of space in a Friedmann–Lemaître–Robertson–Walker universe. It is defined by:* * * * q * * * * * * = * * * * d * e * f * * * * * * * − * * * * * * * a * ¨ * * * * a * * * * * * a * ˙ * * * * * 2 * * * * * * * {\displaystyle q\ {\stackrel {\mathrm {def} }{=}}\ -{\frac {{\ddot {a}}a}{{\dot {a}}^{2}}}} * where * * * * a * * * {\displaystyle a} * is the scale factor of the universe and the dots indicate derivatives by proper time. The expansion of the universe is said to be "accelerating" if * * * * * * * a * ¨ * * * * > * 0 * * * {\displaystyle {\ddot {a}}>0} * (recent measurements suggest it is), and in this case the deceleration parameter will be negative. The minus sign and name "deceleration parameter" are historical; at the time of definition * * * * * * * a * ¨ * * * * * * {\displaystyle {\ddot {a}}} * was expected to be negative, so a minus sign was inserted in the definition to make * * * * q * * * {\displaystyle q} * positive in that case. Since the evidence for the accelerating universe in the 1998–2003 era, it is now believed that * * * * * * * a * ¨ * * * * * * {\displaystyle {\ddot {a}}} * is positive therefore the present-day value * * * * * q * * 0 * * * * * {\displaystyle q_{0}} * is negative (though * * * * q * * * {\displaystyle q} * was positive in the past before dark energy became dominant). In general * * * * q * * * {\displaystyle q} * varies with cosmic time, except in a few special cosmological models; the present-day value is denoted * * * * * q * * 0 * * * * * {\displaystyle q_{0}} * . * The Friedmann acceleration equation can be written as * * * * * ...

Decelerate might refer to

The Deceleration parameter
*
*
*
* q
*
*
* {\displaystyle q}
* in cosmology is a dimensionless measure of the cosmic acceleration of the expansion of space in a Friedmann–Lemaître–Robertson–Walker universe. It is defined by:*
*
*
* q
*
*
*
*
*
* =
*
*
*
* d
* e
* f
*
*
*
*
*
*
* −
*
*
*
*
*
*
* a
* ¨
*
*
*
* a
*
*
*
*
*
* a
* ˙
*
*
*
*
* 2
*
*
*
*
*
*
* {\displaystyle q\ {\stackrel {\mathrm {def} }{=}}\ -{\frac {{\ddot {a}}a}{{\dot {a}}^{2}}}}
* where
*
*
*
* a
*
*
* {\displaystyle a}
* is the scale factor of the universe and the dots indicate derivatives by proper time. The expansion of the universe is said to be "accelerating" if
*
*
*
*
*
*
* a
* ¨
*
*
*
* >
* 0
*
*
* {\displaystyle {\ddot {a}}>0}
* (recent measurements suggest it is), and in this case the deceleration parameter will be negative. The minus sign and name "deceleration parameter" are historical; at the time of definition
*
*
*
*
*
*
* a
* ¨
*
*
*
*
*
* {\displaystyle {\ddot {a}}}
* was expected to be negative, so a minus sign was inserted in the definition to make
*
*
*
* q
*
*
* {\displaystyle q}
* positive in that case. Since the evidence for the accelerating universe in the 1998–2003 era, it is now believed that
*
*
*
*
*
*
* a
* ¨
*
*
*
*
*
* {\displaystyle {\ddot {a}}}
* is positive therefore the present-day value
*
*
*
*
* q
*
* 0
*
*
*
*
* {\displaystyle q_{0}}
* is negative (though
*
*
*
* q
*
*
* {\displaystyle q}
* was positive in the past before dark energy became dominant). In general
*
*
*
* q
*
*
* {\displaystyle q}
* varies with cosmic time, except in a few special cosmological models; the present-day value is denoted
*
*
*
*
* q
*
* 0
*
*
*
*
* {\displaystyle q_{0}}
* .
* The Friedmann acceleration equation can be written as
*
*
*
*
* ...

Related Answers
DECELERATOR
LAG
LETUP
SLOW
SLOWDOWN
SNAG

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